THE BYRSA'S SECOND DEATH:
RECONSTRUCTION AND ERASURE IN THE HEART OF
COLONIAL CARTHAGE
by
Joseph Burkhart
B.A., St. Olaf College, 2017
A THESIS SUBMITTED IN PARTIAL FULFILLMENT OF
THE REQUIREMENTS FOR THE DEGREE OF
Master of Arts
in
The Faculty of Graduate and Postdoctoral
Studies
(Classical and Near Eastern Archaeology)
The University of British Columbia
(Vancouver)
August 2021
© Joseph Burkhart 2021
The following individuals certify that they have read, and recommend to
the Faculty of Graduate and Postdoctoral Studies for acceptance, the thesis entitled:
The Byrsa's Second Death: Reconstruction and Erasure in the Heart of Colonial Carthage
submitted by Joseph
Burkhart in partial
fulfillment of the requirements for
the degree of Master of
Arts
in Classical and Near Eastern
Archaeology
Examining Committee:
Prof. Kevin Fisher; Classical, Near Eastern and Religious Studies; UBC
Supervisor
Prof. Matt McCarty; Classical, Near Eastern and Religious Studies; UBC
Supervisory Committee Member
Abstract
As the spatial, historical, and cultural nucleus of Carthage, the Byrsa
Hill is a stark illustration of the erasure inherent in the city’s colonial reconstructions. In 146 BC, Romans
obliterated the last resisting Punic forces in the acropolis on the hill’s summit, completing the genocide that
was the third Punic War. A century later, Roman colonists radically reshaped the hill into the organizational
nexus of a new colony, removing and burying Punic remains to form an enormous monumental platform . Although
this platform was occupied throughout Carthage’s Roman, Byzantine, and Islamic periods, following its
“discovery” by European explorers in the early 1800s, it became the center of French colonial excavations in the
ancient city. In the last 160 years, the hill has been excavated by many different project directors, and the
published archaeological datasets for the site vary widely in accessibility, quality, and completeness.
In this thesis, I use the Byrsa Hill as a case study to investigate
systemic problems in the ways that archaeologists traditionally organize and publish their data. By integrating
previously published architectural datasets from the Byrsa Hill, I uncover many inconsistencies and gaps,
including vague, contradictory, and missing descriptions of Roman features from older and newer excavations. My
restructured dataset enables new interpretations of the development of the site in the Roman period, in
particular revealing the diversity of construction strategies employed during the complex’s Augustan-era
construction. This
interpretation contrasts with previous studies, which
have uncritically and selectively used
the problematic datasets to emphasize the unity of the complex’s design and construction. This lack of prior
critical engagement, I will argue, shows that research on the site has been limited by divisions of labor and
publication norms that remain common in archaeological research today.
Lay Summary
In this thesis, I investigate the Byrsa Hill, a site in the ancient
Mediterranean city of Carthage (located in modern-day Tunisia). This site was the center of the ancient city for
thousands of years, and, perhaps consequently, it has been a target for erasure by colonizers. Such erasure has
been closely associated with the work of reconstruction, both during the foundation of the Roman colony 2000
years ago, and during the French occupation of Tunisia (1881-1956).
By digitizing previously published maps and profile drawings for the
Byrsa Hill, I draw new conclusions about the site’s early Roman occupation, and I uncover many errors that have
not been pointed out or corrected since the maps and profiles were published. The errors themselves, and the
lack of prior corrections, point to deep and systemic problems in the ways that archaeologists of this site (and
in general) traditionally manage and publish their data.
Preface
This thesis is my own original, unpublished, and independent work. All
maps, diagrams, and other figures were made by me, unless otherwise specified.
All figures which were sourced from previous publications have been
reproduced with permission from their respective publishers. Permission for figures from the volumes
Byrsa
I,
Byrsa II, and
Byrsa III was granted by École Française de Rome. Permission for
figures from
Deneauve (
1983) was granted by Cahiers des Études Anciennes. Permission for figures from
Deneauve (
1990) was granted by l'Comité des Travaux Historiques et Scientifiques. In the
chapters and appendices below, all of these figures are identified either by a conventional in-text citation
(e.g.,
Deneauve 1983,
105 fig. 8), or a Figure ID (e.g.,
). For an explanation of the Figure ID system,
see Chapter
2,
Section
2.1.
In-text citations and the bibliography of this thesis follow a modified
Harvard format. In the interest of clarity, in-text citations referencing
Byrsa I,
II, and
III use the short title of the volumes, rather than the author and year. Thus, a citation that would
normally read (
Lancel et al. 1979,
103) instead reads (
Byrsa I,
103). This is to ensure that readers who are familiar with the site and
accustomed to the title-based citation systems common in Francophone archaeological publications can easily
identify these volumes.
A brief note is warranted on the internal-linking functionality
embedded in the digital version of this thesis. In the PDF file, all cross-references are internal
hyperlinks—i.e.,
clicking on them will take you to the locations they
reference. Cross-references include
references to chapters, sections, subsections, footnotes, as well as most in-text citations. In many PDF
readers, after clicking on a cross-reference, you can return to the previous page by pressing alt-leftarrow
(command-leftarrow on Mac).
List of Supplementary Files
- AxesOfReconstructionMetadata.csv
- FeatureMetadata.csv
- ProfileMetadata.csv
- ReproducedFigures.zip
- Shapefiles.zip
Acknowledgments
In scale, complexity, and pacing, this thesis has been by far the most
difficult project I have ever done. It is the culmination of five years of working, learning and dreaming, and
yet the vast majority of the project was compressed into the last five months and conducted mostly in solitude.
After losing two vibrant communities and many, many friends to the COVID-19 pandemic, I spent thousands of hours
alone in my bedroom, cataloging and correcting errors in other people's data, and trying to understand why so
many generations of archaeologists have suffered under such similar circumstances and struggled with such
similar problems. Words cannot express how prohibitively solitary the experience has been.
And yet, this thesis would not—could not—exist without the support of
many other people. If not for the love, wisdom, and generosity of my family, my partner, my friends, and my
colleagues, I would not be writing these words today.
Thanks first must go to my family, my partner, and my closest friends:
Chris, David, Rebekah, Gus, Amber, Leif, Walker, Jaye, and Ben. These people loved me, encouraged me, and held
me through some of the hardest days of my life.
Thanks also goes to my faculty advisors and mentors. My advisor, Prof.
Kevin Fisher, and my second reader, Prof. Matt McCarty, provided insightful guidance and patient support
throughout every stage of this project. They believed in me, my ideas, and my
abilities, even when my project
felt terribly overwhelming. Without them, I could not have brought this thesis to fruition. Prof. Fisher also
provided partial financial support, in the form of money from the following grants: SSHRC #895-2018-1015 and
SSHRC #435-2018-0463. Prof. Florence Yoon provided advice and support during the early stages of this project,
and (perhaps unintentionally) she inspired my strategy to address one of its earliest challenges: the
sustainable translation of large, highly-structured documents. Prof. Alison Wylie provided late-stage
consultation on some of the systemic issues that I uncovered.
Thanks also are due to my friends from Green College, including Azhar,
Sophie, Alison, Noga, Yotam, Hannah-Ruth, Saori, Sadia, Alicia, Steve, Aisha, Elahe, Alex, and many, many
others. Much of the sentiment and conviction underlying this thesis were born in conversations with these
friends, and their continual curiosity and kindness have been a source of great comfort and inspiration.
No less thanks are due to my friends from the CNERS department,
especially Brianne, Lara, Anna, Gillian, Liz, Safia, and Ben (a different one). No one—not faculty, family, or
(non-grad student) friends—will ever be able to understand what we went through this past year. Their openness,
supportiveness, and utter grit comforted me, grounded me, and gave me the strength to keep pushing my project
forward, even when it seemed that it would never end. A very special shoutout goes to Brianne, Lara, and Liz,
who kept me sane during many long workdays in the Reading Room.
There are so many others I could thank here. My very good friends
Danny, Wed, Anthony, and Jacob also listened to me and supported me and never failed to bring a smile to my
face. UBC's librarians were invaluable—Evan Thornberry, Paul Lesack, Stephanie
Savage, and Steve Bunnell, all of
them provided very helpful consulting on this project. Help also came from staff at various publishers. Richard
Figuier (from École Française de Rome), Pascale Fleury (from Cahiers des Études Anciennes), Patricia Millier
(from Persée), and Agnès MacGillivray (Comité des Travaux Historiques et Scientifiques) all helped me to obtain
the permissions I needed to reproduce many of the maps and profiles in my initial dataset, and their generosity
is deeply appreciated.
I could go on for pages more, but I will end my list here. To all those
whom I've neglected to name, thank you so very much. Your contribution to this project is not forgotten.
for my family
Chapter 1 Introduction: Reforming the
Lifecycle of Archaeological Data
“Thus, we find ourselves in the contradictory position of
being encouraged to
pursue steady fieldwork, reminded in publications on the ethics of the profession that it is our
obligation to publish our work promptly [...], yet the system of rewards and constraints under which
academics labor pushes us against fulfilling standard publication requirements.” (
Pollock 2010,
201)
This project started out as an inquiry into the role that the Roman
reconstruction of the Byrsa Hill played in Augustus’ consolidation of power and legitimacy during the early
years of his reign. The foundation of the
Colonia Iulia Karthago was a massive logistical undertaking,
involving
the clearing, sorting, and reworking of vast quantities of stone rubble, and the excavation and
transportation of hundreds of thousands of cubic meters of earth. The Byrsa was at the center of this
tremendous labor: its summit, which had housed the Punic city’s acropolis, was graded down to virgin soil,
and the sides of the hill were buried in a layer of backfill 2 to 3 stories high, creating a rectangular
platform that covered an area of at least 35,000 m
2, which is 3 times
the area of the forum of Augustus
at Rome (
Gros 1992,
101). This monumental complex served as the organizational nexus for the new colony’s uncompromising
orthogonal grid, establishing the axes of the
cardo maximus and
decumanus maximus and
constraining the dimensions of the
insulae. In my original proposal, I laid out a plan for using
the Roman Byrsa complex as a proxy to study the social and political ramifications of the foundation of the
Colonia Iulia in the context of the early Roman empire.
The COVID-19 pandemic created many barriers to this research. Some
barriers were expected: the Canadian government essentially banned travel to Tunisia, which precluded any
form of ground-truthing, and to Italy and France, which precluded in-person archival research. There does
not seem to be a centralized archive for the archaeological excavations on the Byrsa, not even for the
UNESCO-backed excavations of the 1970s and 80s, and no smaller archive has been digitized or published
online. Thus, I was limited to data which were published in books or
articles—particularly the volumes
Byrsa I, II, and
III, which are the primary excavation reports from the 1970s and 80s, and
which lacked the completeness and precision that may have been found in unpublished archives. Other barriers
were unexpected: with the closure of libraries across the world, the Interlibrary Loan service stopped
accepting requests for physical items, and it did not resume accepting requests until January of 2021—thus,
for the first 3 months of this project I was limited to data which was published in books and articles
that had been digitized and re-published online. This
became a major cause for concern once I
learned that Persée, the repository on which I depended for digital copies of
Byrsa I and
III (as well as many other articles), had digitized their sources using methods that created major
distortions in maps, profiles, and other types of figures. It was only in January, when I was finally in
possession of all of the physical books from the UNESCO-backed excavations, that I was able to diagnose the
cause of the distortion problem and resolve it (see Appendix
A).
Even as I resolved this pandemic-imposed problem, I began to
encounter other roadblocks to data collection that were inherent in my sources, such as inconsistent data
recording schemes, incomplete and selective site plans, and cursory or opaque analyses. I became
increasingly preoccupied with the causes of those problems, many of which I have come to see as deeply
rooted in the systems that have long structured—and still continue to structure—the lifecycle of
archaeological data. These are systems of inquiry, by which excavations are conceived and planned to achieve
specific priorities (i.e., to prioritize certain kinds of data); systems of excavation, by which data in the
field are collected and organized, and by which the locations and final depths of excavation units are
decided; systems of analysis, by which those data are turned into evidence for specific interpretations or
claims; and systems of dissemination and storage, by which those data, evidence, interpretations, and claims
are entangled together in figures (maps, profiles, photos, etc.), tables, and text, arranged in documents or
other structured media (presentations, archives, databases, etc.) and made available to other scholars or
the general public.
These problems are embedded in the practice of archaeological
research today, particularly as it is conducted by western researchers working in the ancient Near East and
North Africa. Problems of inquiry are evident, for example, in the
neocolonial fixation on narrowly-conceived times
and cultures—often “Roman” or “Greek,” or defined in opposition
thereto—and the desire to selectively
preserve their material remains as “cultural heritage,” to the
intellectual neglect and physical destruction of others that are of more
relevance and interest
to local communities and stakeholders. Given the ubiquity of this
problem, it is impossible to discuss
representative examples in detail within the constraints of this
thesis, but it has been identified in
recent and on-going archaeological projects in Afghanistan, Egypt,
Iraq, Tunisia, and many other countries.
In excavations on the
Byrsa, these problems of inquiry first
manifested in the early excavators’ obsession with the site’s Punic
remains. In their quest to uncover Punic features, especially tombs,
these excavators tore through the
hillside, giving only cursory attention to Roman levels and
essentially ignoring medieval Islamic remains.
The later excavators of the 1970s and 80s attempted to rectify these shortcomings: they recorded
Islamic
remains when they found them (though these were relatively few and
far between), and they carefully documented the Roman backfill and occupation layers in the few locations where
their stratigraphy was undisturbed. Ironically, these lacunae in Roman and medieval remains at times forced them to focus most of their
attention on Punic features and artifacts, unavoidably reprising the proclivities of their forebears. This
association was strengthened by the tone of their mission, which was situated within UNESCO’s larger
campaign to “Save Carthage” from encroaching urban development. On the Byrsa, that meant mostly saving ruins from the Punic city, since prior excavations had greatly
diminished or outright destroyed the Roman, Byzantine, and Islamic remains.
Problems of excavation involve deficiencies inherent in the
techniques and decisions that directly govern the collection and recording of data. In the UNESCO-backed
excavations on the Byrsa, these issues are evident, e.g., in the lack of proper stratigraphic illustrations
in certain sectors (Section
6.1), the lack of comparative data
on the construction of the foundation piles (Section
5.1.2), and
the lack of technical description of the only extant remains of the Augustan apses (Section
5.1.3). As I will explore in Sections
6.3 and
7.1, these
problems are linked to traditional divisions of labor and publication norms in
archaeological research. In
other words, these are systemic problems, not personal ones.
Problems of analysis involve the opaque creation of “archaeological
fact”, in which the distinctions between “data” and “interpretation” become blurry or disappear entirely.
For example, as I discuss in Chapters
5 and
7, it is sometimes very difficult (if not impossible), in the maps of
Byrsa I,
II, and
III to see which features were found
in situ and which
were speculative or reconstructed. This sort of ambiguity makes it very challenging to independently
evaluate the excavators’ analyses and reuse their topographical data.
Because problems of excavation and analysis can only be identified
through the careful review and analysis of excavation records, they can become obscured by problems of
dissemination and storage, which are more intractable and farther reaching. On the Byrsa Hill, the problem
can be put simply: the results of excavations can be accessed only by a few dozen scattered articles and
several books. These sources, even those from the UNESCO-backed excavations, contain major gaps, and yet there are
no centralized archives for the unpublished excavation records. This problem is situated within a broader “publication crisis” in archaeology, which has remained
entrenched despite numerous attempts to address it over the last 50 years. This crisis is complicated by the
fact that book publication continues to be a crucial (and increasingly difficult) barrier to professional
entry into academic archaeology.
The published results of the UNESCO-backed excavations are
essentially limited to Byrsa I, Byrsa II, and Byrsa III. Each of these volumes was published no more than 5 years after the last of its data was collected:
Byrsa I (published 1979) covers excavations in 1974–1976, Byrsa II (published 1982) covers
excavations in 1977–1978, Byrsa III (published 1985) covers excavations in 1977–1980. Within the
literature on Carthage more broadly, this timeframe is unusual, as most publications were delayed by 10
years or more. The volumes for the British excavations (1974–1979) were delayed by 5 years (1984) and 15
years (1994). The volumes for the German excavations (1974–1980) were delayed by 11 years (1991) and 17 years
(1997). The volumes for the Swedish excavations (1979–1983) were delayed by 19 years (2002 ) and 35 years
(2018). These large publication delays can be found at many other sites across the Mediterranean, and they reflect the fact that it is enormously difficult and expensive to prepare excavation records
for publication as a book.
The protracted delays in preparing such books are not helped by the
fact that they are often unsatisfactory, either because they are impersonal (
Hodder 1989), or “boring”
(
Boivin 1997 quoted in
Opitz 2018),
or incomplete (as I explore in the chapters below). Implicit in
these problems is a sort of tension between the need to acknowledge
the narrativity inherent in
archaeological observations and analyses, and the need to
transparently document those observations and the
logic of those analyses for other scholars and the general public.
The idea that a book-centric approach to site publication is inadequate
for addressing this tension
has been debated since the early 20th century (
Richards 2004), but it first
received widespread consideration (at least among British scholars) in the late 1970s with the publication
of the Frere report (
Frere 1975). Since then, it has occasionally been examined by committees (see
especially
Cunliffe 1983 and
Carver et al. 1992) and written
up in personal observations (e.g.,
Pollock 2010;
Morgan 2013). Prior to the 2000s, these efforts were largely ineffective, because the technologies necessary for
quickly connecting distant researchers with excavation archives were either inaccessible or did not exist
(
Richards 2004). As the internet has matured and digital publication tools have
proliferated, some excavations have adopted hybrid research schemes that attempt to balance open or
accessible archiving with more conventional publication media (e.g.,
Opitz, Mogetta, and
Terrenato 2016), but these are still exceedingly rare. In
general, for a variety of reasons, traditional books remain the standard for site publication.
Previous treatments of this issue have largely viewed it through
theoretical and methodological (and sometimes economic) lenses: what is the nature of archaeological data
and interpretation, and how should they be disseminated to be more accessible and useful
(and more
cost-effective for taxpayers)? Somewhat less discussed is the problem’s professional dimension. As academic Review, Promotion, and Tenure (RPT) requirements have steadily increased at north
American institutions over the last 20-30 years (
Schimanski and Alperin 2018;
Alperin et al. 2021), book publication has continued to be the “gold standard” of
applications for tenure within the humanities (
Estabrook and Warner 2003). This is in spite of the fact that a majority of academics do not believe book publication should be a
requirement, nor that a book is necessary to present their scholarship; moreover, failure to complete a
monograph correlates overwhelmingly with departure without tenure (
Estabrook and Warner
2003).
I believe this problem can be tied to a lack of training and
institutional support in archaeological data management. Archaeologists deal with an incredibly diverse
array of data types from a myriad of sources and contexts, and they have the singular responsibility, to an
extent perhaps unique among the sciences, to serve simultaneously as excavator, curator, archivist, and
writer—to which may be added
programmer or
webmaster, if they intend to digitally publish
their excavation archives. These roles are simultaneous, not sequential. The plans of the writer depend on
the plans of the excavator, curator and
archivist: the publication of a
site report that is integrated with
a digitally accessible excavation archive (e.g.,
Opitz, Mogetta, and Terrenato (
2016),
whose project design is discussed in
Opitz 2018) is logistically impossible
if the excavation plans, data recording
plans, and data organizational frameworks are not constructed with it in mind. This means that even before
the archaeologist sets foot onsite, she needs to have decided how she will meet the needs of scholars who
will read her report and reuse her data. These requirements make it clear that archaeologists are, in a very real sense,
data
scientists. Yet while we are taught how to collect, critique, and analyze data, we are not formally
trained to organize, structure, or store it.
In this way, the aim of my project has become two-fold: to use the
site of the Byrsa Hill as a case study for systemic problems in archaeological data management, in order (I
hope) to improve the state of the publication of the site, opening it to wider inquiry. After digitizing
and collating most of the previously published cartographic data, I will integrate the data into a single
georeferenced dataset. From this initial dataset, I will extract the georeferenced extents of the most
important Roman and Punic architectural features, and I will synthesize the existing data on each of them.
This combination of extraction and synthesis will produce a new, restructured dataset of most of the Roman
and some of the Punic features, which will allow me to pose new interpretations and ask new questions of the
site. The entire restructured dataset will be openly published online, enabling readers to replicate my maps
and measurements.
A last note. The colonialism inherent in my project should be
acknowledged plainly. Firstly, I am a white, settler-colonial, cis-het-identifying man, living and working
in Vancouver, British Columbia, on land that was taken by force from the hənqəminəm-speaking xʷməθkʷəyəm
(Musqueam) people, who have lived here for many thousands of years, and whose heritage, knowledge, and ways
of being are still actively being destroyed today. I directly benefit from the oppression of these people,
even though I have tried hard to learn about their history and culture, and to work against the systems
which oppress them. Secondly, much of the data I use in my project was collected within colonialist and/or
racist systems of thought, which saw Greeks and Romans as beacons of civilization enlightening dark and
savage peoples through colonization and assimilation, and which positioned the European colonizers of the
18th, 19th, and 20th centuries as their direct descendants and rightful successors in this quest. These
schools of thought had diminished by the time of the UNESCO-backed investigations of the 1970s and 80s, but
aspects of them still persisted, and continue to persist today. Thirdly, I am using these data primarily to
investigate the social and political implications of imperial Roman colonization. The deaths of Carthage,
first in the genocide of 146 BC, and second in the razing and reconstruction of the imperial colony,
constitute one of the most profound acts of colonial erasure in all of Roman history. As the observant
reader may note in the sections below, the past 160 years of excavation on the Byrsa Hill have in some ways
reprised that second death, largely erasing thousands of years of material history through destructive
excavation and incomplete publication. It is my earnest hope that this project may set at least a small
amount of that
injustice to rights.
Chapter 2
Notation Systems Used in this Thesis
“Plan, dû à A. Thouverey, des fouilles du P. Lapeyre (Revue Africaine,
1934, pl. 2, entre p. 345 et p. 346)”
“Plan, by A. Thouverey, of the excavations by P. Lapeyre
(
Revue
Africaine, 1934, pl. 2, between p. 345 and p. 346)” (
Byrsa I,
24)
“On trouvera, joint à cette notice, un plan des fouilles (Pl. XI) [sic]
Il a été exécuté par M. Bonnet-Labranche, architecte diocésain. Les lettres et les numéros insérés dans le
texte renvoient au dit plan.”
“A plan of the excavations (Pl. XI) will be found attached to this notice. It was
executed by M. Bonnet-Labranche, a diocesan architect. The letters and numbers inserted in the text refer to
the said plan.” (
Delattre 1893a,
95)
“Nous donnons une description sommaire des divers vestiges conservés ou reconnus,
en les répartissant par paliers que nous désignerons par le chiffre de leur altitude”
“We give a summary description of the various remains preserved or recognized, by
dividing them in stages which we will designate by the number of their altitude” (
Saumagne 1924b,
178).
The three quotes above illustrate some of the different approaches that
previous researchers have taken to identifying figures, features, and feature locations on the Byrsa
Hill. Since
excavations began in the 1850s, the site has seen more than a dozen project directors, and about as many
notation systems. Generally, each new system has been presented as a matter of course, with little to no
rationale for its design or explanation of its function. As I will show in Chapter
5, more care is needed when attempting to work with data on the
scale of an entire site. In the sections below, I will explain the systems that I use to specify figures,
features, and feature locations.
2.1 Figure ID System
The past centuries of excavation on the Byrsa Hill have produced a
truly dizzying quantity of maps, sections, and other geospatial illustrations. The fraction of these that saw
the light of publication are scattered across many dozens of articles, bulletins, and books, although the
majority of them can be found in the Byrsa volumes. In order to create an integrated dataset of the
Roman and Punic structures on the Byrsa, I must draw upon well over a hundred of these graphics, considering
their ambiguities and inconsistencies, determining their original geospatial extents, and clearly linking them
to the data and feature traces that I derive from them. Due to publishing restrictions, I cannot reproduce all
of these figures in my thesis; for most of them I can only provide a citation. It is critical that these
citations be meticulous, since my results cannot be reproducible if my dataset is not clear.
Proper citation is made more difficult by
the fact I must identify not
just the publication and the location of the figure within it, but also the person or entity who digitized that
publication. As I discussed in Chapter
1, for most of this work I have been
limited not just to drawings that have been published, but
to drawings that have been digitized and
re-published online. During digitization, figures can become distorted by random or systematic errors,
to the point where they become unusable—this problem is abundantly clear, e.g., in Persée's digitized editions
of
Gros and Deneauve
(
1980) and
Byrsa I and
III (see Appendix
A). While I have done my best to rid all of my data of such errors,
identifying the person or entity who performed the digitization is still necessary to ensure that other scholars
can potentially identify errors that I have missed, so that they do not propagate to other studies that draw
from my results.
As a result of these requirements, it is difficult to include enough
citation information for every figure while maintaining overall readability. To obtain a balance, I will employ
a figure ID system that clearly identifies a figure's original publication, location within that publication,
and the publication's digitizing entity, all within a unique, compact code. Each code is composed of three
identifiers separated by a full stop:
- source (B1, B2, GD1980, etc.): the figure's original publication. The full
citation for each code is given in Table 2.1.
- scanner (J, P, etc.): the person or entity who digitized source. The
meaning of each code is given in Table 2.2.
- page (006, 010a, 151-1, etc.): the page number of the figure in
source. This identifier always begins with three digits (including leading zeros if necessary) to aid in
sorting. When the digits are followed by 'a' the figure is a foldout page (that has not been assigned its
own number) immediately following the page specified by the three digits; 'b' indicates a second foldout
page after 'a'. If there are multiple figures on page, then '-1', '-2', or '-3' will indicate the
place of the identified figure in the order (by ascending figure number)
of figures on that page (in very
rare cases, this is used to indicate a specific subsection of a figure—see e.g., , , ;
, ; , ). If a figure occupies multiple numbered pages, it is identified by the page on
which it begins (this only occurs once: ).
Table 2.1: Source codes used in
Figure IDs.
Scanner
code
|
Scanner
identity
|
G
|
Gallica
(https://gallica.bnf.fr)
|
J
|
Joseph
Burkhart (author)
|
K
|
Staff of
Walter C. Koerner Library
|
P
|
Persée
(https://www.persee.fr/)
|
Table 2.2: Scanner codes used in
Figure IDs.
Several examples may prove helpful. refers to the only figure
on page 123 of the copy of Byrsa I digitized by Persée (P = Persée). Likewise, refers to the
second figure on page 151 of the copy of Byrsa II digitized by me (J = Joseph). Finally,
refers to the second foldout figure after page 10 of the copy of Byrsa II digitized by me.
All figures digitized by Persée (scanner
code P) had their pixel aspect
ratios corrected
as shown in Appendix
A.
2.2 Feature ID System
There are thousands of Punic and Roman features in prior publications
on the Byrsa Hill. Many of them are never identified unambiguously, and many are shown on maps with ambiguous
symbology that makes it difficult to distinguish features that were actually found from features that
were merely reconstructed or hypothesized by the excavators.
I have attempted to resolve these problems in two ways: first, by
limiting myself to digitizing only large structural features (walls, cisterns, etc) and mostly omitting
architectural fragments; second, by creating a new organizational framework in which each feature is given a
unique alphanumeric ID that encodes its ontological category. I am acutely aware that the creation of a new
identification system for a site with decades of data may prove naïve, if not futile, so in designing this
system I have sought to prioritize accessibility to francophone scholars and compatibility with previous IDs.
Each ID is composed of a type code, subtype code (optional), number, and ontological code:
- Type and subtype codes distinguish
features by general architectural
categories and subcategories, which are indicated in Table 2.3.
Each subtype is specific to its parent type. Some types do not have a subtype. Wherever possible, the codes
reflect wording that is similar in both English and French, and where this is not possible, the codes
reflect the French.
- Numbers are assigned sequentially to features within each subtype from 1 to
9999, and each number is given leading zeros to ensure that there are always 4 digits (this helps with
sorting). If a feature had a previous ID that indicated its order in a type or subtype (e.g., piles
C1, C2, C3, or walls a, b, c of Punic block D), whenever
possible a number was chosen to reflect that previous order (e.g., pile C1 becomes , wall
b of Punic block D becomes ).
- Ontological category codes indicate whether a feature is extant (e),
reconstructed (r), or hypothesized (h). These terms require some clarification.
- By extant, I mean a feature that is shown in situ in my
initial dataset because it was directly described in a publication in a geolocatable fashion.
- By reconstructed, I mean either
- a feature that was shown as a probable reconstruction within my initial
dataset,
- a feature that was directly described in a publication, but not in a
geolocatable fashion,
- a feature that is neither shown in my initial dataset, nor described in
a publication, but whose presence, position, and form can nevertheless be judged to be
“probable” from the initial dataset.
- By hypothesized, I mean a feature that is neither shown in my initial
dataset, nor described in a publication, whose presence and position is supported by the initial
dataset, but whose form can only be judged to be “possible.”
These codes and numbers are combined in the format
[type]-[subtype][####][Ontology], so that, for example, refers to an extant apse semicircular wall
(or piece of a wall), and refers to a
reconstructed cistern (or piece of a cistern).
All of these feature IDs are presented in tabular form with
corresponding maps in Appendix
C. In these tables, I identify the map
from which the feature was traced, and any underlying assumptions that were necessary to complete the trace.
In the interest of full transparency, I have also created unique IDs
for the axes I used in my reconstructions. When the reconstruction of a feature involves the use of one of these
Type
|
Subtype
|
English
|
French
|
CI
|
-
|
cistern
|
cisterne
|
ES
|
-
|
stairs
|
escalier
|
MU
|
AR
|
apse
rectilinear wall
|
mur
rectiligne d’apside
|
|
AS
|
apse
semicircular wall
|
mur
semi-circulaire d’apside
|
|
FA
|
façade
wall
|
mur de
façade
|
|
IA
|
wall in
(Punic) block A
|
mur de
l’Îlot A (Punique)
|
|
IB
|
wall in
(Punic) block B
|
mur de
l’Îlot B (Punique)
|
|
IC
|
wall in
(Punic) block C
|
mur de
l’Îlot C (Punique)
|
|
ID
|
wall in
(Punic) block D
|
mur de
l’Îlot D (Punique)
|
|
IE
|
wall in
(Punic) block E
|
mur de
l’Îlot E (Punique)
|
|
SA
|
amphora
wall
|
mur
d'amphores
|
|
SC
|
substructural wall C
|
mur
substructurel C
|
|
SD
|
substructural wall D
|
mur
substructurel D
|
|
SE
|
substructural wall Es
|
mur
substructurel Es
|
|
SF
|
substructural wall F
|
mur
substructurel F
|
|
SG
|
substructural wall G
|
mur
substructurel G
|
|
SH
|
substructural wall H
|
mur
substructurel H
|
|
SK
|
substructural wall K
|
mur
substructurel K
|
|
SM
|
substructural wall M
|
mur
substructurel M
|
|
SN
|
substructural wall N
|
mur
substructurel N
|
|
SO
|
substructural wall O
|
mur
substructurel O
|
|
SS
|
substructural wall S
|
mur
substructurel S
|
|
SX
|
substructure wall (other)
|
autre
mur substructurel
|
PI
|
B
|
foundation pile in row B
|
pile
en la rangée B
|
|
C
|
foundation pile in row C
|
pile
en la rangée C
|
|
E
|
foundation pile in row E
|
pile
en la rangée E
|
|
X
|
foundation pile (other)
|
autre
pile
|
RU
|
-
|
rudus
|
rudus
|
Table 2.3: Type and subtype codes
axes, I reference the ID for that axis in the
feature trace table in Appendix
C. A table and accompanying map of
these axes is also included in
Appendix
C.
2.3 Feature Location System
The excavators of the French
Mission created a customized grid system
to allow themselves to specify feature locations in an imprecise but concise fashion. This system divides the
entire site into 2020 m major grid cells (
through
) that are identified by column (A through Q) and row
(I through XX). The major grid cells are then subdivided into
a 44 grid
of 55 m minor grid cells (1 through 16).
A feature's location is then specified by combining the ID of a major grid cell with the number of one of the
interior minor grid cells (e.g.,
).
This system is the key to georeferencing most of the maps and profiles
in the
Byrsa volumes. Unfortunately, much of the system was not published, and I had to reconstruct it
from the pieces that were. My reconstruction of the grid system will be presented in Chapter
4.
This feature location system works well for concisely (albeit
imprecisely) locating figures on a sitemap, and I have chosen to use it in this thesis in order to ensure
compatibility and comparability with previous scholarship. It must be noted that a drawback of this system is
its opacity to readers who are not already familiar with the site. For example, designating a wall's location as
“
” would mean nothing to a reader who did not already
know that major grid cell
is in
the southwest corner of the complex. To compromise between these competing demands for compatibility and
accessibility, I have elected to use the system sparingly in my discussion of various features, but to embed it
deeply in the feature metadata that is presented in Appendix
C and
included in my supplementary files,
Chapter 3 An Abridged History of
Excavations on the Byrsa
“C'est de cette idée de l’interdépendance, non seulement technique, mais
monumentale, de l'ensemble des vestiges qu’il convient de partir pour reprendre l'étude de cette colline
dont le malheur paradoxal est d’avoir été trop explorée.”
“It is from this idea of the not only technical, but
also monumental
interdependence of all the remains that we should start to resume the study of this hill, whose
paradoxical fate is to have been explored too much.” (Gros in
Byrsa III,
25)
The history of excavations on the Byrsa Hill spans 160 years and
more than a dozen different project directors. For the first century or so, basically all of the project
directors operated independently, with almost no coordination. They ranged widely over the hillside, largely
avoiding the areas excavated by their predecessors. Their open-air excavations removed huge quantities of
earth and materials, as they searched for features of interest (primarily Punic tombs and inscriptions).
When they documented other features at all, they described them briefly and vaguely. Those features very
rarely survived the destructive combination of natural erosion and spoliation that followed from excavation,
so their descriptions, however cursory they may be, often remain indispensable. Consequently, any
large-scale investigation of the Byrsa Hill must give an account of the site’s excavation history.
That history is too long and convoluted for a full account to be
included here, but a very abridged account should still prove helpful. For the sake of clarity and brevity, I will not discuss every researcher in this chapter, only those
whose findings are pertinent to my datasets. I will also not discuss those findings in detail; such details
will be provided, when necessary, in Chapter
5.
3.1 Charles-Ernest Beulé (1859)
While the Byrsa Hill was included in a number of loose surveys in
the 1700s and early 1800s (e.g.,
Shaw
1738; Humbert 1821;
de Chateaubriand 1859), Beulé was the first western researcher to excavate on the site. A French archaeologist and politician
with a thorough education in classical literature and history, Beulé had first made a name for himself by
excavating on the Athenian Acropolis, where he used a large amount of explosives to uncover a Roman
staircase and a Byzantine postern gate (
Campbell 2007). During his
single, self-funded excavation season (1859), Beulé made a massive informal ground survey of the hill and
its immediate surroundings, and his team of excavators (mostly local workers) conducted at least 11
different excavations. Beulé published a very inaccurate map of the survey and excavations, along with a
description of their results in
Fouilles À Carthage (
1861), a rather rather rambling and confused, albeit enthusiastic book,
replete
with quotes from and references to ancient authors. The excavations that will be relevant for my dataset are “Fouilles G” (
1861,
46-65), which uncovered some apses along the south side of the Roman Byrsa
complex; “Fouilles F” (
1861,
42), which provided an approximate height for the Roman complex in its
southeast corner; “Fouilles K” (
1861,
39), which revealed remains of what would later be recognized as a wall
of interlocking amphorae, but which the researcher mistook for a cellar; and “Fouilles I” (
1861,
66-74), which uncovered another alignment of apses along the complex’s east
side.
3.2 Alfred-Louis Delattre
(1880-1897)
Almost thirty years after Beulé’s expedition, Delattre began
conducting excavations in many locations on and around the hill. These excavations were conducted under the
authority of the
Pères Blancs, an ecclesiastical order that was tied first to the Saint-Louis
Chapel and later also to the Cathedral, and of which Delattre was a member. Delattre had a penchant for bite-sized publication, resulting in a mess of small articles and reports
that are often vague, repetitive, and confusing. For my datasets, his most important excavations are those in the complex’s southwest corner, where he
uncovered part of the substructural walls of a temple (
Delattre 1893a; note that the excavator mistook these foundations for the walls
of a bastion); the south perimeter, where he uncovered an alignment of apses that originally were continuous
with those found in Beulé’s “Fouilles G”
(
Delattre 1893a); and the southeast perimeter, where he
found more apses that were
backed by a wall of interlocking amphorae (
Delattre 1893b;
Delattre 1894).
3.3 Charles Saumagne (1923-1926)
In 1923, Saumagne began directing a new archaeological project
focused on the east side of the complex under the auspices of the
Direction des Antiquités et Arts de
Tunisie (
Saumagne
1924b,
177;
Byrsa
I,
35). The excavations and surveys from this project produced the first map to cover the entire site (
Saumagne 1924b,
181
plan II), which included very rough elevation measurements. Saumagne continued the project in
1925 and 1926, but he never published the results of these later campaigns (
Byrsa I,
35 n. 65); they were finally
taken up and brought to publication over 50
years later in
Byrsa I.
Saumagne (
1924a) also investigated urban layout of Roman Carthage and its relationship
with the surrounding rural cadastration, but these findings are less relevant for this thesis.
3.4 Gabriel Guillaume Lapeyre
(1930-1938)
Four years after Saumagne’s investigations had concluded, Lapeyre,
another member of the
Pères Blancs, began a new project focused on the southern side of the
complex. Over the next eight years, Lapeyre conducted a series of excavations that uncovered numerous
Punic
tombs and Roman substructures, one of which he enthusiastically mistook for part of a Punic enclosure (
Lapeyre 1934). The quantity and locations of these excavations are difficult to pin down, because their results were
published very incompletely and imprecisely, when they were published at all (
Byrsa I,
25). Lapeyre recorded almost no stratigraphic information, and his
excavations destroyed the vast majority of the Roman strata for the south side of the complex.
3.5 Colette Picard (1947)
Intrigued by some features found by Lapeyre under a large building
in the southern part of the complex, Picard, who was then the curator of the site of Carthage, conducted a limited investigation of the
area (
Ladjimi-Sebaï
2005,
43;
Byrsa I,
31-32). She determined them to be non-funerary walls dating to the late 3rd
or early 2nd century BC, near the end of the Punic period (
Picard 1951).
3.6 Jean Ferron and Maurice
Pinard (1950-1958)
Several years after Picard’s investigation, Ferron (another member
of the
Pères Blancs) and Pinard (an architect) began directing a new project which resumed Picard’s
excavations and extended them to the south (
Ladjimi-Sebaï 2005,
44;
Byrsa
I,
33). Underneath
the
Roman embankment, they found
the remains of some Punic buildings along an orientation that was different from the Roman layout. The
results of these excavations, while rudimentary, were published rather promptly and completely (
Ferron and Pinard 1955). Afterwards, Ferron and Pinard extended their excavations eastwards, where they found remains of more
Punic buildings grouped into city blocks. The results of these later excavations were published in similar
fashion to the earlier ones (
Ferron
and Pinard 1960).
3.7 Serge Lancel et al.
– The French Mission (1972-present)
By the early 1970s, decades of real estate prospecting and urban
expansion had caused ancient Carthage to be almost completely subsumed under modern constructions. In 1972, at the request of the newly independent Tunisian government, UNESCO launched an
international campaign to excavate remaining parts of the ancient city, to keep it from being completely
destroyed. The Byrsa Hill was re-entrusted to French institutions, and the
Académie des Inscriptions et
Belles-lettres created a new project, the
Mission Archéologique de Carthage-Byrsa to lead
the new excavations, with archaeologist Serge Lancel as the overall project director (
Morel 2011b). This project, which I will
hereafter
call “the French Mission,” began excavating in 1974, and has continued to excavate more or less continuously ever since (
Morel 2011b). The project was divided into
several teams: the first team (responsible for “sector A”) was lead by Serge Lancel with the assistance of
Jean-Paul Thuillier, the second team (responsible for “sector B”) was lead by Jean-Michel Carrié and Nicole
Sanviti (succeeded in 1978 by Jean-Paul Morel), and the third team (responsible for the summit and parts of
the southern slope) was lead by Pierre Gros with the assistance of Jean Deneauve, Marie-France Giacobbi and
Françoise Villedieu (
Morel 2011b). A handful of architects have
contributes to the project, in particular Gérard Robine, as well as the technical artist Philippe de
Carbonnières. Jean-Paul Morel became the director of the project in 1983, a position he still occupies today
(
Morel 2011b).
The primary publications to come out of this project are
Byrsa
I,
II, and
III. Primary excavation results can also be found in several other
articles (e.g.,
Gros and
Deneauve 1980;
Deneauve 1983;
Morel 2011a). While there have been several
indications that
Byrsa IV and
V are in the works, there has been no other major long-form
publications from the project since 1985, when
Byrsa III was published.
Chapter 4 Collating the Cartographic
Data
To date, no large-scale map has been
published that indicates
features' dimensions, orientations, dating, and construction for the entire Byrsa Hill complex.
Ideally, this map should also show elevation data for the upper and lower extents of the features, or at
least show the extents of other figures in which elevation data are encoded (such as profile drawings—see
Chapter
6). Instead, a multitude of smaller maps have been
published (mostly in the
Byrsa volumes), which are drawn in different styles, emphasize or omit
different features, and conform to varying standards of accuracy and precision. In this Chapter, I will show how
I have integrated these smaller maps into a single cartographic dataset, which I will call my “initial
dataset.” In the next chapter, I will show how this integration revealed many ambiguities and
inconsistencies in prior maps, and how I resolved or mitigated them to produce a final dataset that is as
internally consistent as possible.
The first step to producing a unified sitemap is to
“georeference” each map in the initial dataset—that is, to determine the extents that it represents
within a Coordinate Reference System (CRS). Visually, this causes the maps' features to overlap, making it easy
to compare features between multiple
maps and create traces of their outlines. As far as I can tell, it is not possible to directly georeference any
of these maps: none of them display their original datums (reference points within the CRS), and none of their
parent publications provide other definitions of their extents, such as coordinates or gridlines in their CRS.
Consequently, each of these maps must be georeferenced indirectly, with their contents visually aligned with the
contents of other maps either in the initial dataset or some external dataset.
4.1 Basemap
The best candidates for basemap were
and
.
Both maps displayed large sections of the reference grid, covering most, if not all, of the Byrsa hill,
and both maps also displayed two modern buildings (the Saint-Louis Cathedral and the Carthage Museum), enabling
them to be georeferenced relative to features in modern maps.
was chosen over
for three
reasons. First,
covers a larger area (over
125,000 m
2 more than
), so its reference grid should be more
representative of both the hill and its surroundings. Second,
is printed in a larger scale
(1:1000, while
is approximately 1:1500), so it
should be more precise and less susceptible to printing-induced error. Third,
is drawn in a more
exact-looking style, with
thinner lines and less stylized features,
suggesting that it is intended to be less schematic than
. One notable drawback to
is that it displays significantly fewer major grid cells (81 compared
to
's 120), but these are spread out over a
larger area. As I will show in Section
4.2, the missing
sections of the reference grid in
can be reconstructed from the existing ones.
Before the reference grid could be reconstructed, the basemap had to
be georeferenced relative to an external dataset, so that the derived grid would be georeferenced as well.
Conventionally, digital georeferencing is carried out using algorithms that determine the “best fit”
for a map, given some reference coordinates—the algorithm scales and warps the image, and translates it to its
georeferenced location. It is important to give the algorithm as many reference coordinates as possible and to
make sure that they are spread out over the whole map, otherwise the algorithm will determine the best fit only
for part of the map. In
, modern buildings
were only shown in a small part of the map, near the summit,
so georeferencing the map relative to these buildings would not produce a good fit for most of the site. Because
would be used to derive the reference grid,
it was essential that the grid cells on the georeferenced
map have the correct dimensions. Consequently,
was georeferenced twice. First, it was algorithmically
georeferenced relative to an idealized 2020 m grid to ensure that the map's grid was properly scaled. Then, it was manually translated and rotated so that the footprints of the modern buildings in the map
overlapped with the corresponding footprints in an external dataset. The external dataset used for this purpose was from OpenStreetMap (OSM), because its building footprint fit the
's building footprint most closely (data from Google Maps
was also evaluated—see Figure
4.1).
4.2 Reconstructing the Reference Grid
As was mentioned in
Section
4.1, the
reference grid in
is incomplete. Major grid
cells have only been drawn in two areas of the map,
leaving large swaths of the site uncovered. Moreover, the minor grid cells have not been plotted at all—in fact,
this is
the case for all large maps of the site. Both lacunae can be
resolved from the existing data:Apses the
missing major grid cells can be reconstructed by extending the lines of the existing grid, and the missing minor
grid cells can be re-created by mathematically defining a 44 grid for each major grid cell.
The reconstruction of the major grid cells proceeded as follows.
"Horizontals" and "verticals" are the lines of the grid, and are referenced by the cells that they run between
and around (Figure
4.2). Consequently, "the horizontals from
–
" denotes the 4 East-West lines that run between and
around cells
–
. When horizontals or
verticals are referenced for more than one row or column, they are constructed from the outermost vertices of
those cells (the inner vertices are ignored).
The first cells to be
reconstructed were those whose boundaries either
were directly plotted on the basemap, or could be determined by extending existing horizontals and
verticals
(Figure
4.3). Cells
–
and
–
were
traced directly
from the basemap. Cells
–
were drawn by intersecting the horizontals from
–
with the
verticals from
–
. Cells
–
were drawn by intersecting the horizontals from
–
with the
verticals from
–
.
At this point, two blocks of cells
had been reconstructed, leaving a
gap corresponding to cells
–
(Figure
4.4). The
boundaries of
cells
–
were determined by first drawing horizontals between the eastern vertices of
–
and
the
western vertices of
–
, and then intersecting those horizontals with verticals drawn along
their
quadrants. Cells
–
were drawn by intersecting the horizontals of
–
with the verticals from
–
. Cells
–
were drawn by intersecting the horizontals from
–
with the verticals
from
–
.
To ensure that no part of the site
fell outside the bounds of the
reconstructed reference grid, two additional rows of major grid cells (
–
) were created to the
north, and one additional row (
–
) was created to the south (Figure
4.5). Cells
–
were drawn by first constructing two new
horizontals which intersected with the western vertical from
–
and the eastern vertical
from
–
at a distance
of 20 m and 40 m from
and
. These new horizontals
were then intersected with the
verticals from
–
,
–
, and
–
, and the new cells were drawn accordingly. Cells
–
were drawn by first constructing a new horizontal which intersected with the western
vertical from
–
and the eastern vertical from
–
at a distance of 20 m. This new horizontal was
then intersected with the verticals from
–
,
–
, and
–
, and the new cells were
drawn
accordingly.
Because the minor grid cells are not plotted on the basemap, they had
to be entirely reconstructed from their description in the
Byrsa volumes: measuring 55 m, they were
created by subdividing each major grid cell into a 44 grid (illustrated in
,
,
; textual
description in
Byrsa III,
5 n. 1). Notably, the reconstructed major grid cells do not measure exactly
2020 m, nor are they exactly square; this is expected, because they were traced and reconstructed from a map
that was hand-drawn, printed, and then scanned, each of which introduces error. Consequently, it is not possible
to divide them evenly into 55 m minor grid cells. Instead, I divided each one into 16 quadrilaterals by drawing
lines between the quadrants of opposite sides (Figure
4.6). This
produced minor grid cells which were not precisely square, but were very close, and it spread out the error in
the major grid cell among its constituent minor grid cells.
4.3 Other Maps
Every map of the site (that was useful for my purposes) was
georeferenced relative to the reconstructed minor and major grid cells, except for (georeferenced
relative to foundation piles in ),
(georeferenced relative to the outlines
of
cisterns and walls in ), (georeferenced relative to the outlines of stones in
),
(georeferenced relative to outlines of stones
in ), (georeferenced relative to
features in and ), (georeferenced relative to features in , , , ,
and ), (georeferenced relative to features in ), (georeferenced relative to
features in ), and (georeferenced relative to features in
).
In total, these maps, which
comprise my initial dataset, cover an
overall area of 25608
m
2, including
21248 m
2 (or about 60%) of the hypothetical extents of the Roman Byrsa's
monumental complex. The extents of these maps are plotted in Figures
4.7,
4.8, and
4.9.
Chapter
5 Digitizing the Features
“on ne dira jamais assez combien l'absence d'archives a été préjudiciable à un
développement rationnel de la recherche sur le sommet de Byrsa”
“we can never say enough how detrimental the absence
of archives has been to the
rational development of research on the summit of the Byrsa” (Gros in
Byrsa III,
25)
“A large part of our failure to publish what we 'know' may result from the fact
that we aren't sure what we do know or how we know it.” (
Dever 1996,
42)
Digitizing features from the initial dataset required the resolution
of four significant problems. First was the problem of scale: the dataset covers thousands of Roman and Punic
features, and digitally tracing features on this scale is a major logistical challenge. Second is the problem of
variability: many features are depicted on different maps in slightly different positions and orientations,
requiring the evaluation of the different depictions and the citation of the map chosen. Third is the problem of
ambiguous nomenclature: many features either have no (published) identifier, an ambiguous identifier (e.g.,
there is a “mur a” in both Punic block
C and Punic block
D), or several identifiers (e.g., “mur D”
is sometimes called “mur Lapeyre”). Fourth is the problem of ambiguous ontology: on many maps, features found
in situ are depicted alongside features that are conjectured
(“reconstructed”) by the excavators. For
some features, particularly the Roman substructural walls, there is often no visual distinction between the two,
dissolving the line between evidence and interpretation.
I have attempted to resolve these problems in two ways: first, by
limiting myself to digitizing only large structural features (walls, cisterns, etc) and mostly omitting
architectural fragments; second, by creating a new organizational framework in which each feature is given a
unique alphanumeric ID that encodes its ontological category. The details of this framework are explained in
Section
2.2, but a very brief review may be helpful. The Feature ID codes
are composed of type (wall, cistern, etc.), subtype (substructural wall D, façade wall, etc.), number (0001,
0002, etc.), and ontological codes (E - extant; R - reconstructed; H - hypothesized), which are combined into a
Feature ID code of the form [type]-[subtype][####][Ontology], so that, for example,
refers to an
extant apse semicircular wall (or piece of a wall), and
refers to a reconstructed cistern (or piece of
a cistern).
A brief discussion about the accuracy and precision of my traces is
warranted. Because I cannot ground-truth my results, I cannot build a reference dataset to compare them to, so I
cannot definitively judge their accuracy. A rough comparison to satellite data from Google Earth (Figure
5.1) indicates that features are within about 2 m of their counterparts
in the satellite images, which is very likely within the error bounds for the satellite imagery.
More useful is to consider the precision of my traces. In the interest
of brevity, my assessment must be qualitative, rather than quantitative. The precision of my results can be
evaluated from the internal consistency of my initial dataset, i.e., to what extent the boundaries of features
shift between maps. Much of my initial dataset is consistent to
within 10 cm, most of it is consistent to within
20 cm, and all of it is consistent to within 30 cm. This is perhaps reflective of limitations inherent in my
reconstruction of the reference grid (see Section
4.2),
since
the lines of the grid shown in the basemap were approximately 20-30 cm at scale. In summary, my feature traces
are reasonably accurate and precise.
5.1 The Roman Features
The extant and reconstructable Roman architectural features on the
Byrsa Hill mostly fall into two categories: substructures and perimeter structures. The first category includes
substructural walls and foundation piles that supported above-ground structures and helped to contain the
massive embankment created during the complex's initial construction. The second category includes structures
that lined the complex's perimeter, such as the apses
which supported the
outermost retaining walls, and the
stairs that provided access to the platform from the streets below. In the sections that follow, I will examine
those features which are most relevant to this thesis, either because they date to the Augustan foundation, or
because they replaced other such features. Because the foundation piles and substructural walls generally have
previous IDs that are relatively unambiguous, (e.g.,
C17), I will use those IDs in my initial discussion
and then introduce my new IDs at the end of each section.
It is often difficult to assign dates of construction to the Roman
features, since most of the time they have already been excavated, then backfilled. Where stratigraphic context
is no longer accessible, dating must proceed based on analyses of materials, construction, and the structural
requirements of the complex, which can only give a general idea of the complex's development.
Features of interest in this thesis can usually be assigned to one of
two phases. Features from Phase 1 were generally built during the initial construction program that began with
the Augustan foundation and lasted for at least a decade or more. From the very beginning of the program,
substructural and structural features were needed to direct, resist, and constrain the pressure exerted by the
Augustan embankment, which generally towered 10-20 m over the level of the streets below. Structures from this
phase were often constructed of rubble stones bound together with clay or earth, rubble stones that were
reshaped and arranged in
opus reticulatum, or large sandstone blocks taken from earlier Punic
structures and arranged in
opus quadratum or
opus africanum. Features from Phase 2 were
generally built during a large renovation and reconstruction program that took place in the second half of the
2nd century AD under the Antonine emperors. Under this program, the layout of the Byrsa was subtly reorganized
to accommodate new buildings, including a temple in the SW corner and a large judicial basilica in the NE
corner. The substructural features that were built or refurbished in this period are almost always in
opus
caementicium (
Deneauve
1990,
143-145, retained in
Ladjimi-Sebaï 2005,
68), and the structural features
often contain stones which were clearly quarried by the Romans from sources not used during the Augustan
foundation (e.g., El Haouaria and Hamilcar sandstone, Djebel Jelloud limestone).
5.1.1 The Walls
In the paragraphs below, the construction and dimensions of the
substructural walls are discussed. In the interest of clarity, walls are presented in order from south to north.
In the interest of brevity, only walls which belong to Phase 1, or replaced those walls, or are relevant for the
reconstruction of those walls are presented.
5.1.1.1 Wall D (Figure 5.2)
Wall
D (see Figure
5.2)
was first investigated in the early 1930s by Lapeyre, who, under the impression that it was some sort of Punic
fortification, apparently excavated along it for a length of over 80 m (
1934,
341-343). When the wall was re-examined
by the excavators of the French Mission
(Carrié and Sanviti in
Byrsa I,
106-113; Lancel in
Byrsa II,
45-46), they found that
Lapeyre had deliberately misrepresented its construction and
its dimensions in his description and his maps to
better suit his interpretation.
Wall
D is of bipartite
construction. The lower section, which
in some places was set in a shallow foundation trench, was constructed using essentially the same materials and methods as the
E piles: rubble stones
from the Punic destruction layer bound together with clay.
, The bottom of this section basically conformed to the topography of the layers
immediately below the
Punic destruction layer,
but the way the wall conformed was variable: in some places the bottom course was arranged in a spiked
formation, in others a stepped one (
Byrsa
I,
112). The upper section, which was generally thinner
than the lower section (suggesting that it was not molded in a trench), was built heterogeneously, with segments
of large sandstone blocks alternating with segments of rubble joined with clay (
Byrsa I,
112-113). The interface between the upper and lower sections varies in
elevation between 52.29 m and 51.11 m for a western segment (
), tracking with the elevation of the
bottom of the wall (
Byrsa I,
113). The variance is not reported for the eastern segments.
Based on the stratigraphy, composition, and construction of wall
D
, Carrié and Sanviti
concluded that the wall closely predated the Augustan
embankment (
Byrsa I,
113). However, their study only accounted for the westernmost extant segments;
two eastern segments were investigated by Lancel (in
Byrsa II,
45-46), and these
complicate the picture. Profile
seems to show
that wall
D’s foundation trench cuts not just the
Punic destruction layer, but also the Augustan embankment above it, indicating that the wall was constructed
after the embankment and causing Lancel to reject Carrié and Sanviti’s earlier conclusions.
While Lancel’s analysis is convincing for the eastern segments, I do
not think it is necessarily applicable to the western segments, the closest of which is located over 20 m away.
The western segments clearly conform very closely to the level of the pre-Punic destruction layers, and the
interface between lower and upper sections roughly conforms to it, too. If the entire wall was built after the
embankment, why would the builders have contoured the bottom of their trench to the Punic pavement and
sub-pavement layers, and then tailored the level of the interface to match that contouring? The contouring and variable construction of the wall’s bottom is more consistent with a modular approach
to the wall’s construction, in which different teams of workers under different supervision laid segments of the
lower section in different places along a pre-determined centerline. A key advantage of this bipartite approach
is its logistical flexibility: segments of the lower section could be scheduled for construction strategically,
to meet the distribution of available building materials and the local structural demands of the embankment’s
construction.
The wall’s upper section may have been constructed separately;
certainly some segments of the wall were
built in two stages at different points in the construction of the embankment, as the two layers of the
construction trench in profile
indicate.
Construction of the upper section might also have been
piecewise, since the arrangement of the large stone blocks varies between segments. In summary, the wall was probably constructed in individual segments, more or less in concert with the
embankment, with the specific timing, order, and methods varying between different segments.
The width of wall
D varied, but how is not exactly clear.
Lapeyre (
1934,
342) reports that it is on average 1 m, but
he then reports that the blocks are generally 0.66 x 0.70 x 0.60 m, with some as large as 1.10 x 1.01 x 0.50 m
or even 2 m (whether he means 2 m in length, width, or height is unclear) at the southeastern end—these
dimensions clearly do not reflect an overall wall width of 1 m. Carrié and Sanviti do not report an average
width, but one of their profiles (
) indicates a
width of about 1.2 m for western segment
(consistent with map
). Farther east, Lancel’s
profile
seems to indicate a width of about 1.8
m for the east side of
. Unfortunately, Lancel’s cursory description of
(about 1.0 m wide, located
even farther east)
does not indicate whether the extant feature preserves the wall’s full width. I will assume that it does.
5.1.1.2 Wall G (Figure 5.3)
Wall
G (see Figure
5.3)
is very poorly published: I am not aware of any previous publication which provides even a cursory discussion of
its construction and dimensions, with the exception of
Deneauve (
1990,
144), who briefly notes that is is made from the same materials, and using the
same methods, as wall
D and the
E piles. On at least one large map
of the site,
, wall
G is depicted as completely contiguous, but
as maps
and
show, this is incorrect. Three small extant sections can be traced
based on
,
, and
. As with wall
D, the intervening segments can be reconstructed
based on
assumptions of continuity, and the extents can be hypothesized based on the extents of the eastern and western
Phase 1 apses, as in Deneauve's (
1990,
151) proposed reconstruction. All of these sections are shown in Figure
5.3.
5.1.1.3 Wall H and an
Associated Wall (Figure 5.4)
Wall
H (see Figure
5.4) is mentioned only cursorily in the
Byrsa volumes, and
subsequent publications have added little to the picture.
Deneauve (
1990,
149) describes its construction as irregular stones (presumably rubble) joined
with earth, which is clearly similar to the construction of wall
D, and consequently he dates it to the
Augustan foundation. It had a foundation pit nearly 1 m deep (
Byrsa I,
94). There are only two
extant segments of
H in my initial dataset (
and
), but Deneauve, on the basis of
(unpublished) excavations conducted to the north of those sections, argues that there were identical
substructures 26 m north of them which mirrored the extant sections (
1990,
150-151). I retain these
reconstructions. The extant and reconstructed sections of this wall are shown in Figure
5.4.
The inner westward spurs of wall
H are interrupted by a set of
very large sandstone blocks (up to 2.5 m long, almost 1 m wide, almost 1 m high), which are linked together in
courses (three are extant) by dovetail seals resting on bare earth (Gros in
Byrsa I,
273-280;
Deneauve 1990,
157). Two isolated pairs of similar
blocks to the west of these courses indicate a westward continuation. Judging from map
, this
continuation extended at least 24 m west of the westernmost pair, as an excavation trench there revealed the
foundation trench of the same wall. Based on the construction and dimensions of this wall, Deneauve suggests it
served as the stylobate of a temple which is known to have existed in this area. Assuming symmetry about a
central axis, Deneauve infers that this wall circled around behind the temple to meet up with the northern spurs
of wall
H. It is not clear how Deneauve determines the western boundary of this wall, but judging from
, he sets it about 3.8 m to the east of
the large Roman cistern. I retain his
reconstructions. The
extant and reconstructed sections of this wall are shown in Figure
5.4.
5.1.1.4 Wall K (Figure 5.5)
On the other side of the stylobate wall, wall
K (see Figure
5.5) perfectly resumed the track of the northern
westward spur of
, but in
opus caementicium,
rather than earth-bound rubble (
Deneauve 1990,
149). Deneauve interprets this dimensional
continuity as evidence that
wall
K represents a Phase 2
alteration or reconstruction of previous Phase 1 foundations. Following the same assumptions of symmetry as he used for the stylobate wall above, Deneauve posits an
identical wall that mirrors wall
K about the temple's central axis. I retain this reconstruction. The extant and reconstructed sections of this wall are shown in and Figure
5.5.
5.1.1.5 Wall M and Three
Associated Walls (Figure 5.6)
Wall
M (see Figure
5.6) was a substructural wall in
opus caementicium running
basically parallel to the
cardo maximus about 28 m from the western side of the complex. Extant segments of this wall can be seen e.g., in maps
,
,
and
. At wall M’s
southern end, a second wall, also in
opus caementicium (
Deneauve 1983,
95), continued perpendicularly to meet the edge of the
cardo maximus.
Extant segments of this second wall are visible in
and
.
Additional excavations found
segments of a third wall (to the west) and a fourth wall (to the north), which joined the previous two walls
into a rectangular enclosure adjacent to the
cardo maximus. Unfortunately, the extant segments of the third and fourth walls do not appear to have been published in
a reasonably georeferenceable fashion. They are shown on several low-quality
georeferenceable maps (of which the
best is ),
but these maps are invariably printed at a very small scale,
and they diverge from the rest of my initial
dataset by at least 1-2 m. I do take the western extent of the third wall from , since this is a critical constraint that
no other map can provide, but every other aspect of these walls must be reconstructed.
I reconstructed wall
M as follows. I assume that the northern
side was flush with the line of the southern façade of the eastern basilica in
(see Section
5.1.3.4), and that it was 4.0 m wide (following
Deneauve 1983,
105 fig. 8). I reconstruct the intervening segment between
and
based on an assumption of
continuity. I assume that the southern extent of the wall is given by
, and that the northern extent is
flush with the line from the south façade of the basilica..
I reconstructed the second (southern) wall as follows. I assume that
the west side was colinear with the west side of the third wall, and that the wall maintained a constant width
of about 2.1 m, based on the width of the west side of
.
I reconstructed the third (western) wall as follows. I assumed that
its south side abutted the north face of the second wall, and that its north side abutted the south face of the
fourth wall. I assume the west side followed the line shown in
. I assume the wall had a constant width of 4.4 m, following
Deneauve (
1983,
95).
I reconstructed the fourth (northern) wall as follows. I assumed that
the north side was flush with the line of the south façade of the basilica in
. I assumed that the east side had a width of 2.1 m as shown in
Deneauve (
1983,
105 fig. 8). I assumed that the west side was colinear with the west side of
the third wall, and that its width was equal to that of the east side.
5.1.1.6 Walls D', F', and
G' (Figure 5.8)
Deneauve conducted excavations in a
handful of locations on the north
side of the central square (very near the side walls of the modern museum), which uncovered the remains of
substructural walls that paralleled walls
D,
F, and
G, which he termed walls
D’,
F’, and
G’ (see Figures
5.7 and
5.8). The results of these excavations were only published in one
cursory article (
Deneauve 1983), which provides very little information about the walls’ locations, dimensions, and construction. The
schematic site plan included in this article (
Deneauve 1983,
105 fig. 8) is drawn to scale (specifically 1/200), but it is discontinuous and
it has no reference grid or other feature which could be used to georeference it.
The excavators uncovered the
remains of five segments of wall
D’. Of these, the westernmost abutted the north wall of the large enclosure adjacent to the
cardo
maximus (
, see Section
5.1.1.5) and the
easternmost seems to have been aligned (and perhaps continuous) with the southern façade wall of the basilica
(
Deneauve 1983,
105 fig. 8). The width of wall
D’, judging from the plan, varies between 1.0 and
1.2 m; in my reconstruction, I
assumed a width of 1.1 m. No information is given about the construction of this wall, but Deneauve dates it to
Phase 1 (
1983,
96).
The excavators uncovered the remains of two segments of walls
F’ and
G’, which ran parallel to each other (
F’ abutting the north side of
G’) to
the south of and parallel to wall
D’. For the western segment (which according to the plan was located 9.0 m east of wall
M), judging
from the plan, the interior distance between
D’ and
F’ was about 9.5 m,
F’ was about 1.5 m
wide, and
G’ was about 1.7 m wide (
Deneauve 1983,
105 fig. 8). For the eastern segment (which according to the plan was located
10.0 m east of the line
of the Basilica’s western façade), judging from the
plan (
Deneauve 1983,
105 fig. 8), the interior distance
between
D’ and
F’ was about 9.8 m,
F’ was about 1.3 m wide, and
G’ was about 1.7 m
wide. The interior distance is almost identical to that separating wall
D from wall
F (
Deneauve 1983,
96). No information is given about
the construction of these walls, but Deneauve dates
G’ to Phase 1 and
F’ to Phase 2 (
1983,
96). I consider these walls to be reconstructed within the bounds of the two
segments. I hypothesized their original eastward and westward extents based on assumptions of symmetry with
their southern counterparts (this is consistent with Deneauve's reconstructions in
,
).
5.1.1.7 Other Walls
On the north side of wall
D’, the
excavators found
opus
signinum paving (
Deneauve
1983,
97). On the eastern side of wall
D’, the excavators found that this paving was delimited by a foundation pit (Figure
5.9), which
Deneauve (
1983,
97) notes is aligned with similar remains found 60 m to the west during repair
work to the museum. Judging from the plan, the interior distance between this pit and wall
D’ was about 10.1 m and the
width of the pit was about 2.3 m (
Deneauve 1983,
105 fig. 8). Deneauve hypothesizes that the enclosed area constituted a portico
opening onto the forum (
1983,
97). No information is given about the construction of this wall.
Deneauve (
1983,
98) does not directly suggest a function,
but implies that the wall may have served as a stylobate. To the west of Deneauve’s excavation, more remains
(probably) belonging to this substructure were found in
during renovation work in the modern museum (
Byrsa III,
140).
Consequently, I consider this wall to be reconstructed from this point
east (), and hypothesized from this
point west ().
The remains of a parallel
substructure, which probably served as the
stylobate for another portico, were found adjacent to the northwest side of the basilica (
Deneauve 1983,
98;
Byrsa III,
140). No map of these remains has been published. The width of this
substructure is given as 1.75 m (
Deneauve 1983,
98), which yields an interior distance of 58.94 m between it and the stylobate
of the southern portico. To the west of Deneauve’s excavation, more remains (probably) belonging to this substructure were found
in
-13 during renovation work in the modern museum (
Byrsa III,
140). Consequently, I
consider this wall to be reconstructed from this point east (
), and hypothesized from this point west
(
).
A little over 10 m past the eastern ends of this northern portico, in
excavators uncovered a segment of a
perpendicular substructural wall which supported the
basilica’s western alignment of columns ( see Figure
5.10;
Byrsa III,
52). The width of the remains was 2.40-2.45 m, and the wall appears to have
continued under the entire alignment of columns (
Byrsa III,
52). Neither the extant
segment nor the reconstructed segments of this wall are labeled on the maps of
Byrsa III, and the
former is visually very similar to
adjacent later constructions. I assume that the
north and south ends of this
wall originally abutted the north and south façade walls of the basilica (see Section
5.1.3.4). As far as I am aware, there is no published description of
the wall’s mode or date of construction; I will assume that the wall dates to Phase 2 and that it was constructed similarly to those another
substructural wall which was found about 21 m farther east. This eastern wall is structurally related to the
apses of the eastern perimeter, so it will be discussed in Section
5.1.3.4.
There are several additional sets of substructural walls that deserve
mention. According to Deneauve’s reconstructions (
,
), on the east side of the Byrsa, three
north-south substructural walls are shown adjacent to (or under) two staircases which provided access to the
cardo IV east below (see Figure
5.11). Two walls are adjacent to the southern staircase (
), and one wall is adjacent to the northern
staircase (
). As of this writing, I have
not been able to find any published description of these walls.
The southern pair is also shown in
, but it is
unclear if it is directly attested or just
reconstructed. Based on
and
, it appears that the eastern wall of the southern
pair abuts wall
G and belongs to Phase 1, while the western wall abuts wall
F and belongs to Phase 2. The northern
wall is shown in no other maps. Some of its remains may have been encountered during Deneauve’s (
1983,
96)
excavation in the southwest corner of the basilica (which his
reconstruction calls for it to abut), but his
publication does not mention them. In Deneauve’s Phase 1 reconstruction (
), the wall seems to abut wall
G’, and in the
Phase 2 reconstruction (
), it seems to
abut wall
F’. I will assume that
F’ was built
around this wall, so that its dimensions did not change in Phase 2. I will call the southern pair reconstructed,
and the northern wall hypothesized. The relationship between these walls and the adjacent substructural walls
will be further discussed in Section
5.1.3.4.
More certain than those pairs of walls are the substructures which
appear to have
supported a Phase 2 temple in the southwestern corner of the
complex (see Figure
5.12). These walls were constructed in
opus caementicium, with an
opus quadratum crosswall
(which the excavators call
Es) giving them the shape of an H (
Byrsa I,
168-172). The
UNESCO-backed excavations in this area divided the structure into 5 walls:
O (west),
N (north),
S (south),
S1 (smaller wall to the south abutting
O), and
N1 (smaller wall to the
north abutting
O). Based on maps
and
, it appears that
N,
S,
and
O may actually be continuous with one another (i.e., part of a single unified construction), but this is
not mentioned in the excavation report, so I will assume that they are separate.
Finally, there was a retaining wall that was braced by the apses along
the south side of the complex. Since this wall is in close structural relation with these apses and other south
perimeter structures, it will be discussed in Section
5.1.3.2.
5.1.2 The Foundation Piles
Excavations on the southern slope
of the Byrsa have uncovered three
rows of Roman foundation piles (B, C, and E) running parallel to the axis of the
decumanus maximus and
spaced 11-12 m apart.
Each row is composed of up to a few dozen piles, spaced 4-5 m apart, thrust into (or through) the
Augustan embankment. These piles served two primary purposes: they assisted in retaining the massive weight of
the Augustan embankment (which would otherwise have overwhelmed the support structures lining the
decumanus
I south), and they served as substructures for walls and other constructions on the surface of
the
embankment.
These piles stretch almost the entire length of the southern slope of
the hill, and given that almost no above-ground Roman structures remained when archaeological excavations began,
the piles were likely some of the first Roman features to be discovered. It is unfortunate, then, that no comparative study of the individual piles has ever been published.
Instead, brief descriptions are scattered across the excavation reports of Lapeyre, Ferron and Pinard, and the
authors of the Byrsa volumes. In the following paragraphs, I draw from the general observations given
in these reports to summarize the existing data for the piles’ location, composition, and chronology.
5.1.2.1 The E Piles
(Figure 5.13)
The northernmost row contains six clearly
extant piles (
E1
through
E6) and physical traces of three others (
Eh,
El,
Ee), and a very likely
location for one more (
Ea).
These piles are roughly constructed from irregular chunks of Ariana limestone and other stones from the
Punic destruction layer that are joined together with clay. Piles
E1,
E2, and
E3
Feature ID
|
Previous name
|
|
pile
E1
|
|
pile
E2
|
|
pile
E3
|
|
pile
E4
|
|
pile
E5
|
|
pile
E6
|
|
pile
El
|
|
pile
Eh
|
|
pile
Ee
|
|
|
|
|
|
|
|
|
|
pile
El
|
|
|
|
|
|
pile
Eh
|
|
|
|
pile
Ee
|
|
|
|
|
|
pile
Ea
|
|
pile
E3
|
|
pile
E5
|
Table 5.1: Feature IDs and
previous
names for the E piles.
display a bipartite morphology in which their lower sections
appear roughly constructed but relatively straight, while their upper sections appear more exactly constructed
but lean towards the east (
Byrsa I,
132-133). This suggests that the
E piles were constructed by digging
foundation pits into (and in the case of
Eh, through) the Punic destruction layers, filling the pits with
irregular chunks of Ariana limestone and other stones from the Punic remains, intermixed with dirt or clay, and
then placing stones in more regular patterns on top of the filled pits. The rough mode of construction, which
closely resembles that of wall
D, prompted Carrié and Sanviti to conclude that the
E piles are
contemporary with wall
D and shortly predate the Augustan embankment (
Byrsa I,
132-133).
In modeling the Augustan Byrsa, it is necessary to reconstruct some
additional piles and sections of piles in this row and to hypothesize several more. The extant, reconstructed,
and hypothetical features in row E are summarized in Table
5.1 and Figure
5.13. Several of the extant
E piles are clearly fragmentary, so I
have correspondingly reconstructed some sections: these are
,
,
,
,
, and
. Based on the spacing of the
E piles and
their proximity to wall
D, it
seems likely that the
E piles served as supports for a colonnade (
Byrsa I,
135). As such, it is
reasonable to reconstruct additional piles in the gaps between the extant ones: these are
,
,
,
,
, and
(pile
Ea). Given the extensions of the colonnade proposed
by
Deneauve (
1990),
we can hypothesize 4 additional piles to the west of
El (
): these are
,
,
, and .
5.1.2.2 The C Piles
(Figure 5.14)
The central row contains 21 extant piles
(
C1 through
C21), which are constructed of
opus caementicium with small re-used rubble stones whose dressing
resembles that of
opus reticulatum facing.
This composition is consistent with a date after the initial Augustan
Feature ID
|
Previous name
|
|
pile
C2
|
|
pile
C2
|
|
pile
C3
|
|
pile
C4
|
|
pile
C5
|
|
pile
C6
|
|
pile
C7
|
|
pile
C8
|
|
pile
C9
|
|
pile
C10
|
|
pile
C11
|
|
pile
C12
|
|
pile
C13
|
|
pile
C14
|
|
pile
C15
|
|
pile
C16
|
|
pile
C17
|
|
pile
C18
|
|
pile
C19
|
|
pile
C20
|
|
pile
C21
|
|
pile
C8
|
|
pile
C16
|
|
|
|
|
|
|
|
|
|
|
Table 5.2: Feature IDs and
previous
names for the C piles.
construction of the Byrsa complex
(
Byrsa I,
74;
Deneauve 1990,
144). The stratigraphy and morphology of the piles support this hypothesis by
helping to post-date the piles relative to the Augustan embankment. Studies of the stratigraphy around the piles
show no evidence of foundation pits distinct from the piles themselves, and the piles tend to widen slightly
toward the top (
Byrsa I,
74). Both of these observations suggest that the piles were constructed by digging deep shafts through the
Augustan embankment and pouring a mix of concrete and stone inclusions into the shafts.
The
C piles were (originally?) joined together with additional
stonework to form substructural wall
C. The piles are contiguous with the H-shaped foundations on the SW corner of the hill, which also post-date
the Augustan embankment and likely belong to Phase 2. It is possible that the southwest foundations and the
C piles are contemporary;
Carrié and Sanviti
seem to imply that the date of the southwest foundations informs the date of the piles, and refer the reader to the following chapter (a report on the excavations on the SW corner) for further
discussion (
Byrsa I,
132). Unfortunately, while that report acknowledges that the
C piles are
contiguous with the SW foundations (
Byrsa
I,
170), it does not discuss their relationship.
It seems likely that the C piles originally extended farther
eastward, since the last extant one, C21, is over 40 m away from the east side of the complex. I
hypothesize that there were an additional five C piles to the east of C21, sized about 1.8 1.8 m, spaced
about 4.4 m apart, and following the same alignment.
The extant, reconstructed, and hypothesized
C piles are
presented in Table
5.2 and Figure
5.14.
5.1.2.3 The B Piles
(Figure 5.15)
Table 5.3: Feature
IDs and previous names for the B piles.
Feature ID
|
Previous name
|
|
pile
B1
|
|
pile
B2
|
|
pile
B3
|
|
pile
B4
|
|
pile
B5
|
|
pile
B6
|
|
pile
B7
|
|
pile
B8
|
|
pile
B9
|
|
pile
B10
|
|
pile
B11
|
|
pile
B12
|
|
pile
B13
|
|
pile
B14
|
|
pile
B15
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
pile
B1
|
|
|
|
pile
B15
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
The southernmost row contains at least 15
extant piles (
B1
through
B15), with two other possible piles to the east of
B15. These were constructed differently from the piles in the other two rows, with small pieces of rubble
(including some stones that seem to come from destroyed Punic buildings) surrounded by white-grey mortar (
Byrsa I,
133). Their morphology is also quite different, flaring widely at the base (see photos
,
).
These piles are much shallower than the
E and
C piles; some do not even make contact with
the Punic destruction layers, indicating that the piles post-date the Augustan embankment. Carrié and Sanviti
infer that the Punic inclusions were used in other Roman structures before the
B piles, prompting them to
conclude that the
B piles were constructed from the remains of decommissioned Roman structures after the
complex's initial construction (
Byrsa I,
133). More precise dates for the piles have been proposed, but these are
controversial.
While the
C piles likely
replaced earlier Augustan foundations,
the case is not so clear for the
B piles. As Deneauve and Villedieu point out (in
Byrsa
I,
171), supports would have been necessary from the
beginning of the complex to hold back the tremendous mass of the embankment—not just in the southwest corner,
but also all the way along the southern slope. Out of all of the foundation piles, the
B piles had to
make up the greatest difference in elevation, which ranged from 13 to 20 m over the eastern third of the south
slope. The idea of constructing piles, from unworked rubble stones, on a footprint of about 1.8 1.8 m, to a
height of 13-20 m before surrounding them with an embankment seems rather impractical. I think it is reasonable
to suggest that the
B piles were built during or immediately after the construction of the Augustan
embankment, in order to minimize the risk of structural failure. The fact that some of them do not touch the
Punic destruction layers has no bearing on their dating, nor does their morphology. In the absence of more
information about the pile's inclusions and the strata located below them, I think an Augustan dating is
possible, and perhaps probable.
The extant, reconstructed, and hypothesized
B piles are
presented in Table
5.3 and Figure
5.15.
If we date the
B piles to Phase 1, then it is reasonable to
assume that they would have originally extended to some point close to the extrados of the southwestern apses,
since
some sort of substructure was necessary to help retain the
embankment (
Byrsa I,
171) and the substructural walls in
opus caementicium had not yet been
built. This westward extent of the
B piles can be indirectly hypothesized based on the layout and
construction of these later walls, despite significant gaps in their published data (see Figure
5.16).
It seems clear that the
opus quadratum wall
Es was
constructed before the other
opus caementicium walls
N,
S, and
O, and that its
north and south ends, which were ultimately encased in walls
N and
S, originally spanned both of
their widths. While it is likely that wall
Es served an active substructural role in the final building above
it, its first purpose might very well have been as a temporary retaining wall. The pouring of walls
N and
S could not proceed without the destruction of vaults, façade walls, rectilinear walls, and semicircular
walls in the first and fourth apses of the southwestern alignment (
Byrsa I,
169), which would have destabilized the second and third apses, compromising the integrity of the entire Phase 1 support system in an area where the embankment rose 5 –
6 m above the level of apse floors. The installation of
Es would have alleviated that problem. Walls
N1 (
) and
S1 (
) appear to have been
constructed after walls
N,
S, and
O, and they
braced the semicircular walls of the second and third apses against wall
O, which kept the semicircular
walls upright after their vaults,
rectilinear walls, and façade walls were
dismantled.
Based on the published data, It seems that walls N and S
may each have been constructed in two sections: on map , Es's cut into S appears to
end just 20 cm short of the outer edge of S (which is within the range of precision of my initial
dataset), and the western extant piece of S () ends immediately after that. Moreover, the
northwest corner of abruptly ends in
a 90-degree angle cut toward Es. This suggests that both
N and S may have been poured in two segments, with the first segment stretching between O
and Es, and the second segment extending east from Es. Groundtruthing could help confirm or
disprove this hypothesis, since it could show whether the matrix of was continuous with the matrix of
.
Why was wall
Es placed where it was, about 2.5 m back from the
extrados of the southwestern apses? The simplest answer would be that it was placed according to the initial
plans of the 2nd-century architect who designed the temple, but this answer seems unlikely. The architect must
have been aware that there were substructures embedded under the Augustan platform, but they likely did not know
their precise locations and dimensions. These would have needed to be determined before they could begin laying
the foundations. I hypothesize that the
B piles originally extended to a point abutting the east side of
Es, whose location was chosen to mark the end of that extension. The architect could then have been
confident that
Es would function as a temporary replacement for the
southwestern support system, allowing
the workers to safely decommission the first four apses in the southwest alignment. It is possible that the same would be true for the Phase 1 substructure that was replaced by the
C
piles.
Notably, this hypothesis would align the westernmost B pile
(and perhaps Phase 1 C pile) with the westernmost E pile. While this certainly does not prove the
hypothesis, it does make it more attractive, from an engineering standpoint. Thus, I follow this hypothesis and
hypothesize an additional seven piles in row B, each about 1.8 1.8 m and spaced about 3.9 m apart
(consistent with the extant piles near them), following the same alignment.
It seems likely that the B piles originally extended farther
eastward, since the last extant one, ,
is over 40 m away from the east side of the complex. I
hypothesize that there were an additional six C piles to the east of C21, sized about 1.8 1.8 m,
spaced about 4.8 m apart, and following the same general alignment as the rest of the row.
5.1.2.4 Other Piles
During the excavation of the northern portico of the central square
(see Section
5.1.1.6),
Deneauve (
1983,
96) found the remains of a column sub-base about midway between walls
G'
and
D', leading him to suggest that the northern portico had a central row of
columns similar to the southern portico (see Figure
5.17). This sub-base is not reliably
geolocatable. It is somewhat unclear if Deneauve thought there was a row of foundation piles in the northern
portico—he makes no such hypothesis in his text, but his plan (
1983,
105 fig. 8) specifically labels
this sub-base as part of a hypothetical row of
E' piles. This hypothesis seems to be retained in
Deneauve's Phase 1 reconstruction of the site (
), which has a row of 19 squares in the southern
portico and an almost identical row in the northern portico. Consequently, I will assume that Deneauve hypothesized a row of foundation piles in the northern portico,
whose dimensions and spacing were very similar to the
E piles. I retain Deneauve's hypothesis, and I
further hypothesize that these piles were basically square, about 1.8 1.8 m, stretched between the eastern and
western limits given in
(slightly
adjusted north or south to be midway between walls
G' and
D'), with a spacing of about 5.3 m. These piles are given the subtype 'X'.
5.1.3 The Perimeter
Structures
No Roman features have been more enduringly popular in the minds of
western archaeologists than the structures which lined the perimeter of the Byrsa complex. This has created
several notable conditions. Temporally, the perimeter structures have the greatest depth of scholarship, ranging
from Beulé's foray in 1859 to the first—and, so far as I can tell,
only—systematic study of their architecture,
conducted by the excavators of the French Mission in the 1970s and 80s. Physically, they are the worst
preserved, with the vast majority of the apses and façade walls completely destroyed by prior excavations, early
modern and modern constructions, and spoliation. Ontologically, they are very opaque, with large sections of the
perimeter so poorly documented that the distinctions between
extant,
reconstructed, and
hypothesized become very difficult to see. The combination of these conditions means that the dataset
is paradoxically both sprawling and sparse, and very difficult to untangle. It is necessary to make use (with a
critical eye) of some very old measurements and analyses. Sometimes, it is possible to supplement or amend these
with the results of modern systematic surveys, but as we shall see below, the results published by these surveys
are often (though not always) no more complete than the earlier reports, and sometimes require a similarly
critical approach.
This task is very difficult to do at all, let alone concisely. In
the
interest of clarity, this section will be organized spatially. After a brief overview of the sorts of structures
that will be considered, I will discuss the apses on the south side of the western slope, then the apses of the
west side of the south slope, continuing in a counterclockwise fashion until the apses of the northeastern
corner. The perimeter structures of the northern slope and the western slope are mostly unexcavated and have
never been published, so they are omitted. For each section of the perimeter, I will summarize the existing data
for the dimensions, construction, and dating of the structures therein.
The perimeter of the Byrsa
complex was essentially comprised of façade
walls, staircases, rectangular rooms, and apses that lined the complex's edges along the
cardo IV east,
decumanus I south, and
cardo maximus. A brief overview of the apses is warranted.
These were
rectangular rooms that were separated by rectilinear walls, and that each had an opening onto the street and,
opposite that opening, a semicircular recess topped with a semi-dome (
cul-de-four).
While these apses may have performed various functions during their lifetime,
this thesis is concerned only with their structural purpose. They served as the support system of the
outermost retaining wall for the Augustan embankment, a role that was essential from the very beginning of the
complex’s construction.
5.1.3.1 The Southwest
Perimeter
The Roman features of the
southwestern section of the perimeter are
primarily described in the 1974-1975 site report of Deneauve and Villedieu (
Byrsa I,
143-182), and some
subsequent findings are published in
Gros and Deneauve (
1980). These
researchers identified a series of five apses (hereafter “Series 1”) along the southern part of the
western side, of which remains of three are extant. The other apses were either destroyed by prior excavations
or incorporated into a later set of substructures (walls
N,
S, and
O; see section
5.1.1). The extant, reconstructed, and hypothesized figures in Series 1 are summarized in Figure
5.18.
The rectilinear walls rested on a
foundation composed of two courses
of rectangular stones (
Byrsa I,
168). The types (sandstone or limestone, or a combination thereof) and dimensions of these stones have not been
published, but rough measurements taken from map
suggest lengths around 1.5 m and widths around 1.0 m.
The semicircular walls rested on the tufa bedrock of the hill (
Byrsa I,
168).
The rectilinear walls themselves have survived just barely, if at all,
but judging from Beulé and Delattre's descriptions of the southern apses (apparently confirmed by Deneauve's
excavations—see
Gros and
Deneauve 1980,
322), they
would have been constructed in large-block
opus quadratum. The semicircular walls were composed of small pieces of stone rubble bound together with lime and lined
with
opus reticulatum (
Byrsa I,
167). As with the foundations, the types and dimensions of these stones have
not been published, but map
suggests a rubble
layer thickness around 0.9 – 1.0 m and a
reticulatum layer thickness of about 0.15-0.20 m.
The ceilings of these apses have not survived—they were very likely
destroyed during the construction of substructural walls
O,
N, and
S. Deneauve and
Villedieu report a large fragment of a vault in
opus caementicium inside the southernmost apse, but it
is unclear if this came from the apse itself or from some other structure (
Byrsa I,
168).
These apses likely had a façade wall, as indicated by the shape of the
surviving rectilinear wall foundations, but none of this wall appears to have survived (
Byrsa I,
168). Its
construction may have been
identical to that of the rectilinear wall
that abutted the north side of the northernmost apse, perhaps comprising the façade from that point northward
(
Byrsa I,
168).
As Gros and Deneauve reconstruct them (), the apses had
very similar dimensions. Interior diameter varied between 3.7 m and 3.9 m. Interior length varied between 6.4
and 6.3 m, Rectilinear walls were about 0.6-0.7 m thick. Semicircular walls were about 1.1 m thick. The façade
walls fronting each rectilinear wall were assumed to all be the same size, based on the only extant one
(): 0.97 m wide and 1.52 m long. On
the basis of construction, Deneauve and Villedieu date the apses
of Series 1 to Phase 1.
To the south of Series 1, Deneauve and Villedieu found the remains of
a rectangular corner room constructed of façade walls is
opus quadratum and
opus reticulatum
(
Byrsa I,
164-167). The room measures approximately 8.9 m in length, and its width is
about 5.8 m at its west side and 5.5 m at its east side). Based on its construction, this room likely dates to
Phase 1, although later alterations (including the installation of some cisterns) have made its original
function unclear. This room is also shown in Figure
5.18.
To the east of that corner room, researchers identified a series of at
least six apses (of which remains of three are extant) along the western part of the southern side (hereafter
“Series 2”). The extant, reconstructed, and hypothesized features from Series 2 are summarized in Figure
5.19. In construction, these apses mostly mimic the previous
alignment: the semicircular walls were lined with
opus
reticulatum (which presumably served as facing for a matrix
of rubble joined with lime), the rectilinear walls were build in
opus quadratum with stones from the
Punic destruction layer, and there was a façade wall (
opus quadratum or perhaps
opus
reticulatum) (
Gros and
Deneauve 1980,
322). Gros and Deneauve reconstruct façade walls between 0.70 and 0.75 m thick, rectilinear walls about 0.60 m
thick, and semicircular walls about 1.0 m thick (
). Contrary to the previous alignment, the apses’
rectilinear walls rested on
rudus foundations, their interior diameters varied between 3.30 and 3.70 m,
and their interior lengths varied between 5.9 and 6.2 m (
Gros and Deneauve 1980,
322). On the basis of construction, Gros and Deneauve date the apses of Series
2 to Phase 1.
Gros and Deneauve's map (
) reconstructs an additional two
apses to the east Series 2, which basically keep Series 2's dimensions and construction. After those two apses
there is about 10 m of no recorded remains before the alignment of apses resumes with the next series. The area
containing the two reconstructed apses, the gap, the next series, and several more apses to the east was
excavated in the early 1890s by Delattre. While his measurements and map (
1893a,
pl. XI; also called
) are not precise or accurate enough to be
trusted, I will briefly summarize his descriptions. Delattre claimed to have identified eight extant apses. By the time of his excavation,
the rectilinear walls of these apses
were entirely gone—perhaps taken as
spolia by people living nearby, who would have noticed the apses that Beulé uncovered previously (see Section
5.1.3.2)—leaving behind only the semicircular recesses, which
Delattre says were constructed of some sort of stone masonry (
1893a,
102-103). At least one of the apses was lined along its interior with
opus reticulatum (
Delattre 1893a,
102).
Delattre’s (
1893a,
102) measurements of these apses
suggests an apse width (interior diamter + widths of the side walls) of 3.20 m, which is rather less than that
of Series 2. This figure is very imprecise because it is an average of Delattre's hypothesized original number
of apses over the approximate length of Delattre's excavations (
Byrsa I,
48 n. 48). I retain the
reconstruction of the two apses from
,
and then hypothesize three other apses whose dimensions match
those of the westernmost apse in Series 3.
5.1.3.2 The South
Perimeter
Such variability grew more
pronounced about 8 m farther east, where
the UNESCO-backed excavations uncovered a series of about five apses (hereafter “Series 3”) that
were originally continuous with those of Series 2.
The extant, reconstructed, and
hypothesized features from Series 3 are summarized in Figure
5.20. They are likely the apses that were left buried by Delattre's
excavations, but which are still shown in dotted lines on his map (
1893a,
pl.
XI). As far as I am aware, the only published descriptions of these apses are from Lancel (in
Byrsa I,
48), who notes very briefly that they are constructed from small pieces of
rubble (I assume joined with lime) inset with large stone pillars in
opus quadratum, and
Morel (
2011a,
352),
who mentions (also very briefly) that the semicircular walls are in
opus caementicium with numerous
ceramic and stone inclusions that appear to be Roman in origin, suggesting a later construction date. Because I have not found any confirmation of Morel's
cursory assessment, I retain the late 1st-century BC
construction date accepted by Lancel, Gros, Deneauve, and Ladjimi-Sebaï. The semicircular walls can be seen on
map
, along with a few remaining sections of
rectilinear walls in
opus quadratum that were set
deep into the rubble-lime matrix, all other stone blocks having been removed by previous excavators or local
people.
Among the four apses whose recesses were completely preserved,
interior diameter was between 2.2 and 3.5 m. If we assume that the outer and inner edges of the façade were
colinear with those of Series 2 (meaning that the façade walls for Series 3 were 0.75 m thick), then interior
length varied between 5.3 and 5.9 m. The rectilinear wall
thickness
varied between 1.0 and 1.5 m, and the
semicircular walls are preserved to a thickness ranging from 1.6 to 2.2 m, with stone pillars 1.0-1.2 m wide and
0.9-1.7 m long. I hypothesize that for each apse, the façade wall segments had lengths that provided an opening
proportional to that reconstructed for the apses of Series 2.
The mode of
construction for Series 3 was markedly different from that
of Series 2. The rectilinear walls were much thicker and set deeply into the rubble-lime matrix of the
semicircular walls. These semicircular walls were also much thicker and were reinforced by thick stone insets,
and they tended to be “flatter,” that is, the central angle of the arc of their intrados is smaller.
The transition between these two modes of construction can be observed in the westernmost apse of Series 3,
whose semicircular wall does not have a stone inset, and whose eastern rectilinear wall does not appear to be
set into the rubble.
The extrados of the Series 3 apses appear to be contiguous with a
thick Roman retaining wall (
),
partially destroyed by prior excavations and spoliation, whose northern
extent was found by the UNESCO-backed excavations to the south and southwest of Punic block
B (
Byrsa II,
143). While this wall is mentioned several times in the
Byrsa volumes,
I am not aware of a previously published description of this wall’s construction or dimensions, and its extents
are not directly geolocatable. Lancel suggests that the wall was destroyed only within the limits of
Beulé’s “Fouilles G,”
meaning that the extant
limits of the former allow the limits of the
latter to be precisely identified (
Byrsa
I,
14). Unfortunately, Lancel did not plot the extant limits of the former on any of his maps. I will assume that the limits of the extant section of the wall
are even with the limits of Series 3. To
the east and west of these apses, the limits of the rest of the retaining wall thus be hypothesized. I
hypothesize that the eastward limit was dictated by the wall of amphorae found by
Beulé (
1861,
39) and
Delattre (
1894,
89-91), and that the western limit was
imposed by the extrados of Series 1. This is consistent with the hypothetical(?) extents shown on maps
and
.
Based on my above assumption, Beulé's “Fouilles G” began
at the western limits of Series 3. These excavations stretched for about 40 m to the east and unearthed another series of (likely) six apses
(hereafter “Series 4”). The extant, reconstructed, and hypothesized features in
Series 4 are summarized in Figure
5.21. Beulé describes their
construction thus: the apses had an
interior diameter of 3.30 m, an internal length (from the apex of the recess to the inside of the fronting wall)
of 4.20 m, a rectilinear wall
thickness of 1.10 m, and a fronting wall thickness of 1.00 m.
Five apses were
constructed (both rectilinear and semicircular walls) from large stone blocks measuring as big as 1.50 x 1.25 x
1.00 m (
Beulé 1861,
60). For the rectilinear walls,
these appear to have been laid in the regular, interlocking courses of
opus quadratum (
Beulé 1861,
60). For some courses, perhaps specifically those of the semicircular walls and/or the foundations, the blocks
were not regularly shaped, but still fit very closely together (
Beulé 1861,
61 and pl. II fig. 2). Mortar was found in some external joints and on some uppermost courses, but
nowhere else (
Beulé 1861,
63). The sixth apse was constructed
mostly in
opus reticulatum (Beulé notes this is one of several, the rest being presumably unexcavated),
and at the time of excavation it still stood 8 m high (
Beulé 1861,
63). Six meters above the floor, the walls of the recess were pierced with square holes which
Beulé (
1861,
64) surmised once held cross-beams. Beulé does not say whether the other apses
also had these holes, but he does note that none of them survived to a height greater than 5 m (
1861,
64).
Some aspects of Beulé's description warrant further scrutiny. Judging
from the variability observed in the dimensions of the Series 3 apses, Beulé very likely homogenized
his
measurements to make the apses all appear the same size. Nevertheless, his measurements are the only ones we have from this point onward, until the apses of the
eastern basilica: all of the apses in Series 4, all of the apses between Series 4 and the southeast corner of
the complex, and all of the apses between that corner and the basilica have been destroyed or incorporated into
modern constructions, and no measurements or maps of them were ever published. Consequently, I retain Beulé's
measurements for Series 4, and I will assume that they are applicable to all of the apses after Series 4 as
well. All of these apses will be considered hypothesized.
The dimensions and construction that Beulé reports for Series 4 are
noticeably different from those of Series 3 (Figure
5.21). Aside from a
slight widening in the rectilinear and façade walls, Beulé's apses are significantly shorter, with an interior
length of just 4.2 compared to the 5.7-6.0 m of the eastern apses of Series 3. This means that their extrados
would (just barely) not touch the intrados of the nearest apses of Series 3. Moreover, Beulé makes no mention of
the south slope retaining wall that was observed to be contiguous to the extrados of Series 3, even though he
had to have encountered it, since its presence in this area is attested in the negative (
Byrsa II,
85 n.
2). I propose that these discrepancies may be caused by two simple problems: first, that the two easternmost
apses of Series 3 were originally lined with semicircular
opus quadratum walls that have
long since
disappeared due to spoliation; second, that Beulé's description of his
apses' semicircular walls may reflect the
dimensions of similar interior stone walls which lined larger,
approximately flat (though perhaps very mildly
curved) walls constructed of rubble joined with lime. These
semicircular walls would then have been contiguous
with the retaining wall. Framed this way, Beulé's odd dimensions and
his omission of the retaining wall fit
together with his obvious shortcomings. His preconceptions, nurtured
by his classical training, inclined him to fixate on the most
immediately impressive features of what he thought were the Punic
ramparts, and to utterly destroy anything less impressive that proved
to be an obstruction. Contrary to what appears on his map, it is certain that he did not clear all six apses down to the level
of their bases; by his own admission (
1861,
59), temporal and financial constraints forced him to simply follow the walls
with discrete trenches. This strongly suggests that he would have disregarded adjacent walls of much rougher
rubble-and-mortar construction, since the features that captivated him were almost entirely constructed in
large-block
opus quadratum.
Consequently, I hypothesize that the apses excavated by Beulé were
actually constructed with a 2.0-1.5 m thick rubble-and-mortar wall lined with a 1 m semicircular fronting wall
of
opus quadratum, and with rectilinear walls extending past the intrados of the fronting wall to meet
the southern edge of the rubble and mortar wall. I retain this hypothesis for all of Series 4 and the rest of
the apses between it and the start of the amphorae wall.
5.1.3.3 The Southeast
Perimeter
Several decades after Beulé,
Delattre (
1893b;
1894) excavated an unspecified number of apses to the east of Series 4,
whose contiguity therewith is unknown. These features are summarized in Figure
5.22. He notes that
one of these apses had interior facing in
opus reticulatum (
1894,
89-90); the rest presumably were
lined with large-block stonemasonry, as was the case for Series 4. Leaning against the extrados of these apses, Delattre found a very large wall of stacked amphorae
(
), which had been filled with the
earth
of the Augustan embankment and then arranged in an
interlocking pattern that was about 4.40 m thick and 6.00 m high (
1894,
89-91). This wall stretched for 50
m around the bend of the southeast corner of the complex, with its western end located close to the eastern end
of Series 4 (
1894,
89). While Delattre provides no map of this area, the extents of this amphora
wall can still be reconstructed with some degree of certainty, provided that we make some assumptions about the
layout of this sector.
At the southeastern corner of the complex, the perimeter turned approximately 90 degrees to the north. There were probably apses along the perimeter
here—this is strongly implied by Delattre's (
1894) description and it is retained in
—and I assume that they
were of dimensions identical to those of Series 4. About 34 m north of the corner, Deneauve's Phase 1
reconstruction (
) has a gap in the
perimeter to allow for a large staircase (
; approximately
30.2 m long and 10.4 m wide) that connected the top of the platform to the
cardo IV east below. His Phase 1 reconstruction has the eastern end of this staircase flanked
by two pairs of apses (which
terminate their segments of the perimeter), and the western end of the staircase founded on a short
substructural wall.
Deneauve's reconstruction calls for the dimensions of
the staircase to change between Phase 1, and Phase
2, but due to a lack of evidence and some key inconsistencies,
I do not
retain this.
At each corner formed by the 90 degree turns in this section of the
perimeter, Deneauve (, ) assumes there was a corner room
analogous to the rooms that definitely
existed in the southwest and northeast corners of the complex. I retain this assumption, and in hypothesizing
the layout of these rooms I assume that their outer walls were colinear with the façade walls of the neighboring
apses, and their inner walls were simply the rectilinear walls of the neighboring apses. I further assume that
their widths and lengths were not less than the interior lengths of the neighboring apses, i.e., 4.2 m.
Finally, I assume that the flanking apses terminated the substructural
walls ( to the south, to the north) that abutted them. This is
contrary to Deneauve's
reconstructions (, ), but I do not see any reason to
accept his suggestion that walls D and
G cut off the openings of the flanking apses here.
Given these assumptions and hypotheses, and based on the dimensions
reported by Delattre, the extents of the amphora wall can be posited with a reasonable degree of confidence.
This is shown in Figure
5.22, where I have extended the amphora wall
to an interior length of 50 m. It is notable that the amphora wall seems to replace both the retaining wall and
the rubble-and-mortar wall reconstructed and hypothesized for Series 4. Delattre clearly says that the amphorae
leaned against the extrados of the apses, and
based on my interpretation
of Beulé's description, I can only
assume that Delattre means the inner semicircular walls that by this point were likely constructed almost
exclusively in large-block stonemasonry. Why (and how) could the thick substructural walls for Series 3 and 4
have been replaced with a wall of amphorae in this area, which constituted by far the steepest section of the
perimeter? I propose that these substructural walls were not necessary in
this sector because the descent of the
staircase lessened the pressure from the embankment, allowing the
south façade of the staircase and the southernmost apses in the eastern
perimeter to take some of the load. Indeed, the western edge of the
amphora wall is almost completely even with
the western end of the staircase—this does not confirm my hypothesis,
but it is consistent with it.
One last topic must be discussed before I leave behind the apses of
the southern perimeter: dating. It is almost universally agreed that the apses along the southwest, south, and
probably southeast slopes date to the Augustan foundation. This dating is based primarily on their construction
and partially on their context. The use of
opus reticulatum and
opus quadratum composed of
stones taken from previous Punic structures is commonly found in other Roman structures which date to the
colony’s first few decades. Along the southeastern slope, the wall of amphorae could be narrowly dated to
between 43 and 15 BC on the basis of stamps (
Delattre 1894,
91). While this logic may not seem watertight—comparative architectural dating is rather imprecise, and the
amphora wall did not stretch across the entire south slope—the destruction of the southern apses and the lack of
documentation for their stratigraphic context ensures that no other material evidence will be forthcoming.
Nevertheless, to these factors might be added one more, namely, that the prospect of modifying sections of this
massive southern support, which for most of its length had to withstand the outward pressure from the embankment
over a height greater than 10 m, was very probably unattractive. It seems likely that in this sector of the
complex, more than any other, structural modification of the retaining wall risked shifting the soil of the
embankment and destabilizing the structures above.
5.1.3.4 The East
Perimeter
The extant, reconstructed, and
hypothesized features of the east
perimeter are summarized in Figure
5.23. Based on Deneauve's
reconstructions (
,
) the pair of flanking apses north
of staircase
and an adjacent corner
room resumed the complex's perimeter, which stretched another 50 m to the north before turning westward again to
accommodate a second staircase (
), which
again was flanked with two pairs of apses. Since the topography of this stretch of the perimeter would probably have been comparable to that around
Series 4, it is reasonable to hypothesize that these apses had roughly the same dimensions as Series 4, and were
similarly backed by a rubble-and-mortar wall followed by a secondary retaining wall. Following Deneauve's
reconstruction, I assume that there was a corner room at this northern turn, and for both rooms' dimensions I
follow the same assumptions that I made for the southeast perimeter. This section
of the east perimeter was in Beulé's time
occupied by an old French cemetery and now is completely buried under
modern constructions, so it
has never been formally excavated.
On the north side of this
staircase lie the remains of the last
documented section of the complex's perimeter, where Beulé (
1861,
67-74) found an alignment of five
apses (of which he excavated two) on the eastern slope of the hill, beginning a little over 100 m north of the
complex’s southeast corner to avoid the old French cemetery. His sparse description of their construction is
superseded by the modern survey conducted by Pierre Gros as part of the UNESCO-backed excavations. The extant, reconstructed, and hypothesized features of the northeast perimeter
are summarized in Figure
5.23
Gros identified nine apses in Beulé’s alignment (four on either side
of a central apse that was on the axis of the
decumanus maximus), and two additional pairs of apses
oriented perpendicularly, bordering the alignment to the north and south. Originally, according to Gros, the apses appear to have been basically homogenous in construction,
although they were decorated differently and some were modified in later periods. Focusing most of his attention on the central apse, due to its superior preservation, he described their
construction as follows.
The rectilinear walls
rested on earthen berm (“banquette”)
foundations—presumably cut into the elevation of the hill as it climbed to the north—while the paved interior of
the rectangular rooms had more complex foundations composed of a layer of pebble-cement on top of a layer of
rubble.
The foundation of the semicircular walls does not seem to have been directly investigated, probably to
minimize the risk of collapse, but it is reasonable to assume that it was identical to that of the rectilinear
walls.
The walls themselves were of bipartite construction. The bottom
section was El Haouaria and Hamilcar sandstone in
opus quadratum, with block width usually 0.40-0.50 m,
height 0.50-0.90 m (shorter for higher courses), and length around 0.50-1.2 m. The blocks had 2.5-5 cm thick joints of beige mortar, and they all bore marks from lifting clamps (
Byrsa III,
7). There were five courses for the rectilinear walls and six courses for the
semicircular walls. On top of the
opus quadratum there were three courses of stones shaped to look like
bricks (specifically
bipedales), some of limestone and others of sandstone, which
were also used in the
facing of a bench-like feature in the central apse (
Byrsa III,
34). They were
presumably joined with the same mortar as was used in the
opus quadratum. Gros did not report their
dimensions, but Beulé puts the combined thickness of the three courses at 0.40 m (
1861,
69).
It is not immediately clear if the brick-like stones extended over the
rectilinear walls, but Gros (
Byrsa III,
7) seems to imply that they do. The impost was pierced with a series of
rectangular holes that Gros suggests held scaffolding used during the construction of the
cul-de-four
over the recess (
Byrsa III,
8).
The layer of brick-like stones served as an impost for the vaulted
ceiling of each apse, which was constructed in
opus caementicium (
Byrsa III,
7-8). Over the semicircular
recess, this was a
cul-de-four, and over
the rectangular room it was a barrel vault. The first northern apse may have had a different ceiling system, but
it is not clear if Gros accepts this (
Byrsa
III,
10-11).
The apses were partially enclosed by a fronting wall composed of
stonework, presumably in
opus quadratum like the rectilinear walls. It was joined to them with the same
mortar, had a width of around 1 m, and may have extended for about 1.6 m on either side of each rectilinear
wall, creating openings of about 2.75 m for each apse (
Byrsa III,
33).
Behind the apses, and operating in conjunction with them, was a
massive substructural wall. This wall served to support the basilica’s eastern alignment of columns, and its
eastern face appears to have braced the extrados of the apses (
Byrsa III,
19) and the eastern
rectilinear wall of the first northern apse (
Byrsa
III,
10). The wall was constructed from blocks of
sandstone from El Haouaria, presumably in
opus quadratum (
Byrsa III,
19). The excavators of
the French Mission do not directly report any dimensions for this wall, and like its western counterpart it is
shown unlabeled on their maps. Judging from map
, its width was about 2.0 m. No extant sections of this
wall are published on a map, even though they certainly have been found, so it must be entirely reconstructed.
The excavators also do not suggest a date of construction.
Gros pointed out that the stonework used in the apse walls closely
resembled that of other structures dating to the Antonine period, prompting him to assign a date of construction
in the second half of the second century AD. He suggested that these Antonine-era supports replaced analogous Augustan-era structures, whose
dimensions and construction would have been identical to the apses on the southern (
Byrsa III,
27,
34) and southwestern (
Byrsa III,
34) slopes.
Gros' dating warrants further scrutiny. It is almost universally
agreed that the extant apses along the northeastern slope date to the second half of the 2nd century AD. This
dating is based entirely on their construction (particularly the distinctive type of opus quadratum and the use
of stones to imitate brick-work) since the UNESCO-backed team of excavators did not find any intact stratigraphy
that predated them. Consequently, the
support system that predated these
apses is not materially attested, and
while some reconstructions have been proposed, they seem to be entirely speculative. As far as I can tell, the
only reconstruction of the eastern Augustan apses to have been published is that of Gros and Deneauve, which
appears without explanation or comment in a plan in
. The corresponding plan for the Antonine era
(
) is presumably the plan followed by Gros
and Deneauve in the construction of their scale model of
the Byrsa complex in the 2nd century AD. This model was featured on the cover of
CEDAC 15 and is
still housed in the Carthage Museum (
Gros 1997,
347 n. 3), but aside from a brief
article in a popular news magazine (
Gros and Deneauve 1996), it remains
unpublished.
and
are really just sketches—the apses are
outlined roughly in dotted lines and the level of detail is quite low—but it is clear enough that in the
Augustan-era sketch, all of the apses have the same dimensions: an interior diameter of about 3.5 m, and an
interior length of about 6.5 m. In other words, it is assumed that all of the eastern apses had the same
dimensions as the south and southwestern apses, but with the same façade as the Antonine apses. Hence, Gros and
Deneauve assumed that the construction of the 2nd century basilica involved the removal, not just of the
Augustan supports, but also of the 7 m-high embankment over an additional 4 to 5 m behind the those supports.
They further assumed that the new supports followed a completely different plan
from the old ones. I think both
of these assumptions have problems.
Problems with these assumptions can be seen in comparison with a
similar building project that took place on a much smaller scale in the southwest corner of the complex. The
construction of the southwest temple took place with an elevation level difference (platform level – street
level) ranging from about 5 to 7 m, along a relatively limited façade (~16 m), in a corner of the platform that
probably was not previously occupied by a large structure. The construction proceeded by encasing the existing
supports with new foundations and filling the voids with more soil, allowing the embankment front to advance
forward. In contrast, the construction of the basilica took place over an elevation difference of at least 7 m,
over a façade more than 80 m wide (almost half of the eastern side of the platform), in a part of the complex
that was very likely occupied by a major, albeit smaller, structure with another structure immediately west of
it. It seems unlikely that the construction of the Antonine basilica would have pushed the embankment
backward, since, if the ground shifted or settled, it would potentially compromise the structural integrity of
other foundations nearby.
Moreover, it seems unlikely that the Antonine apses would have
followed a different plan from the Augustan ones, since during the construction of the southwest temple they
were incorporated into the new foundations, where they continued to play an important structural role. By
extension, if the Antonine apses of the eastern slope were replaced by new apses following a different plan, we
would expect to see some trace of them in the new foundation structures. We should not assume that all of the
Augustan apses were
constructed along roughly the same basic plan: the
retaining wall of the complex was a
massive construction project that required years—potentially well over a decade—of labor. If anything, we should
assume a heterogeneous plan that accounted for local variations in topography and availability of building
material. It is not unlikely that there were multiple construction workshops operating in tandem on different
sections of the retaining wall. The construction methods used along the south slope were clearly not
homogeneous, and there probably was not much aesthetic difference, if all of the apses were originally stuccoed.
Accordingly, I hypothesize that the Augustan apses followed the same
footprint of their Antonine successors. I further assume that the substructural wall abutting the extrados of the eastern apses dates to Phase 1.
These hypotheses are summarized in Figure
5.25.
5.2 The Punic Features
During the initial construction of the Byrsa complex, existing Punic
features were either cleared during the leveling of the summit, destroyed to make way for new Roman
substructures, or else simply buried under the growing embankment. The architectural features that are most
relevant to this thesis are the walls of the five Punic city blocks (A, B, C, D, and
E) on the southern slope, since they occupied the most volume and therefore held the most influence over
the energetic cost of the reconstruction.
The original goal of this section was to document the digitization of
all of the Punic walls, cisterns, tombs, and other features on the Byrsa Hill. Unfortunately, time and size
constraints have made made complete digitization impossible
within the scope of this project. As a preliminary
effort, I have digitized the walls of the five Punic city blocks on the southern slope, as well as a few
cisterns and tombs. The digitized features are summarized in figures
5.26,
5.27,
5.28, and
5.29.
My digitization of these features must be regarded as preliminary. For
the walls, I have not recorded the construction methods, as I did with most of the Roman features, and the
boundaries of my feature traces only reflect contiguity and source map, not actual context—in other words, the
traces of walls are only divided when the map from which they were traced indicates a gap, or when I switch to a
new map for tracing. This means that the boundaries between walls—and their Feature IDs—could change in the future, as they
are refined to better reflect their discrete archaeological contexts. For cisterns and tombs, I have only traced
those features that are included in profiles published within the
Byrsa volumes (see Chapter
6).
The locations and dimensions of these features are given in maps and
tables in Appendix
C, but some additional observations are worth
noting. For block
A, all features have been traced from map
. Even though this map is more
schematic and much less well aligned than most others, it is the only one to show block
A, whose walls,
almost completely buried under the foundations of a later structure, are shown only on
. For block
B, all features have been traced from map
. While the coverage of this block is not as limited
as that of
A—it is also shown on maps
,
,
,
,
, and
—all of these either
are poorly aligned (
), lack
detail (
,
),
or else offer only very partial coverage
(
,
,
). Block
C was mostly covered by maps
,
, and
, but these
maps were in many places poorly aligned with one another. The alignment was particularly off for
,
reaching close to 30 cm in some places, which was surprising because this map at first appeared much more
precise than both of the other maps. Block
D was only covered by maps
and
,
both of
which were poorly aligned with the larger maps.
was taken at the end of the excavations in this block
and thus better showed the extents of the walls; as a result, all features for this block were traced from it.
Chapter 6 Digitizing the Topographic
Data
In the last chapter, I
showed how I digitized all of the Roman
features and some of the Punic ones, and I gave a full synthesis of the existing data for features relevant
to the site’s first phase. This information can offer some insight into the site’s layout, but it does not
reveal anything about the site’s topography, which is essential for understanding the site’s planning,
development, and function, particularly in the Augustan era. As I mentioned in Chapter
1, the Augustan construction of the Byrsa complex required the complete
reshaping of the entire hill: the summit was ground down to sterile soil, and the slopes were buried under
thick layers of soil and debris. Consequently, the design and construction of many of the complex’s
substructures and perimeter structures were largely governed by the initial topography of the hillside.
An archaeological site’s topography can now be reliably recorded
in great detail using remote sensing techniques (e.g., photogrammetry, LIDAR), but these have never been
applied on the Byrsa Hill. Consequently, the hill’s topography can currently only be reconstructed from
published elevation measurements. Such measurements can be found in older publications, such as
Delattre (
1893a,
pl.
XI) and
Lapeyre
(
1934,
pl. 1, 2), but their low accuracy
and poor geolocatability renders them basically useless for my purposes.
Thus, I am limited to measurements published in the
Byrsa volumes.
Elevation measurements in the Byrsa volumes are given
primarily in maps and profiles, although some can be found in the text. While measurements in maps are very
easy to digitize, provided that the map can be georeferenced, it is often difficult to determine what layers
or features they are describing, and how the elevation of that layer changes over space. Hence, profiles are
more useful for my purposes, because they record elevations that change continuously over space and link
them to distinct stratigraphic contexts. In this chapter, I will use the term “profile” to indicate any
illustration which has a vertical axis, even if it is a reconstructive or composite illustration, rather
than a drawing of a trench wall.
The original goal of this chapter was to digitize all of the
elevation measurements that were encoded in profiles in the
Byrsa volumes, and to supplement them
where necessary with measurements from maps. Due to time constraints, I was only able to digitize the
extents of most of the profiles, but these should still prove useful to other scholars who wish to better
reconstruct the Byrsa hill’s topography in the future. Moreover, the process of digitizing the extents
revealed numerous errors and omissions in the profiles and maps, which seem to have gone essentially
unremarked and uncorrected in the 40 years since their publication. While some of these mistakes are minor
and can be corrected without much trouble, others can render profiles very difficult or impossible to use.
A full explanation of how I corrected each profile would be
prohibitively dense and is outside the scope of this chapter. On the other hand, readers who want to use my
digitized profile extents may need to see those explanations, in order to evaluate my results for
themselves. Consequently, while I take a mostly synthetic approach in this chapter, I have put full
explanations of my corrections for the most important profiles in Appendix
D. In the sections below, I will present an overview of the most
common types of mistakes, and then discuss two example profiles in detail. In the next chapter, I will argue
that these mistakes are reflective of deeper problems in the systems by which archaeological data is
published.
6.1 The Main Problems with the
Profiles
There are 99 distinct profiles
in the
Byrsa volumes, of
which I was able to georeference around 60 (see Figures
6.1,
6.2, and
6.3).
The other profiles were left out for a variety of reasons, but mostly because their reference
elevation could not be determined, because they could not be georeferenced, or because they did not seem
relevant for my period of focus, the Augustan era. The profiles that I did georeference are summarized in
Tables
6.1 (
Byrsa I),
6.2
(
Byrsa II), and
6.3 (
Byrsa III).
The problems with the published profiles may be divided into three
main categories: problems with reference elevation, problems with mapped extents, and problems with
symbology.
Table 6.1:
Summary Information for Byrsa I profiles. Reference elevations in
parentheses are adjacent to the profile. Map IDs in parentheses indicate that the
profile is located on the map, but its extents are not plotted or labeled.
Profile
|
Drawn On map
|
Labeled on map
|
Map
|
Ref. Elev.
|
Notes
|
|
|
|
|
51.92
|
|
|
|
|
|
(51.92)
|
Reference elevation given in
(adjacent)
|
|
|
|
|
51.83
|
|
|
x
|
x
|
|
49.13
|
|
|
x
|
x
|
|
50.00
|
|
|
x
|
x
|
|
50.00
|
Map
extent markers are imprecise
|
|
|
|
()
|
(50.00)
|
Reference elevation can be determined from
(colinear)
|
|
|
|
()
|
(49.10)
|
Reference elevation can be determined from
|
|
x
|
x
|
|
51.72
|
|
|
x
|
x
|
|
51.61
|
Profile is split into two pieces that have some
overlap
|
|
x
|
x
|
|
50.33
|
|
|
x
|
x
|
|
49.85
|
|
|
x
|
x
|
|
50.70
|
Extents also shown incorrectly in
(width
4.13 m)
|
|
x
|
x
|
|
53.40
|
|
|
|
|
|
50.00
|
|
|
x
|
x
|
|
|
|
|
x
|
x
|
|
|
|
|
x
|
x
|
|
|
|
|
x
|
x
|
|
|
|
|
x
|
x
|
|
|
|
|
x
|
x
|
|
|
|
|
x
|
|
|
|
|
|
x
|
x
|
|
56.00
|
|
|
x
|
x
|
|
56.00
|
|
|
x
|
x
|
|
48.53
|
Multiple other reference elevations are given; width
in georeferenced map has only one discontinuity (following the map symbology,
which is incorrect - there should be two discontinuities)
|
|
x
|
x
|
|
44.95
|
|
|
x
|
x
|
|
(48.75)
|
Reference elevation given in
|
|
|
|
()
|
47.47
|
|
Table 6.2:
Summary Information for Byrsa II profiles. Reference elevations in
parentheses are adjacent to the profile. Map IDs in parentheses indicate that the
profile is located on the map, but its extents are not plotted or labeled.
Profile
|
Drawn On map
|
Labeled on map
|
Map
|
Ref. Elev.
|
Notes
|
|
|
|
()
|
51.90
|
|
|
|
|
|
46.35
|
Multiple other reference elevations are given, but
they are illegible
|
|
|
|
()
|
48.53
|
Another reference elevation is given
|
|
|
|
()
|
(49.70)
|
Reference elevation is given in
|
|
x
|
x
|
|
46.80
|
Multiple other reference elevations are given
|
|
|
|
()
|
45.05
|
Another reference elevation is given
|
|
x
|
x
|
|
52.73
|
|
|
x
|
x
|
|
52.66
|
|
|
x
|
|
|
(48.30)
|
Reference elevation can be determined from
|
|
x
|
|
|
(49.98)
|
Reference elevation can be determined from
|
|
x
|
x
|
|
(50.50)
|
Extents in are very schematic;
reference
elevation can be determined from
(or from )
|
|
x
|
x
|
|
50.40
|
Extents in are very schematic;
multiple
other reference elevations are given
|
|
x
|
x
|
|
49.30
|
Extents in are very schematic and
partially
incorrect; multiple other reference elevations are given
|
|
x
|
x
|
|
49.11
|
Extents in are very schematic;
multiple
other reference elevations are given
|
|
x
|
x
|
|
49.26
|
|
|
x
|
x
|
|
49.26
|
|
|
x
|
x
|
|
49.13
|
|
|
x
|
|
|
49.18
|
|
|
x
|
|
|
49.18
|
|
|
x
|
|
|
49.43
|
Multiple other reference elevations are given
|
|
|
|
()
|
48.93
|
|
|
|
|
()
|
49.02
|
|
|
x
|
|
|
55.98
|
|
|
x
|
|
|
55.98
|
|
6.1.1 Problems with
Reference Elevation
If a published profile does not explicitly tie some locus to a
reference elevation, it can be very difficult, if not impossible, to obtain the elevation data encoded in
the original profile. Sometimes, it is possible to get a replacement reference elevation from another
profile that is adjacent (e.g.,
gets 51.92
m from
) or colinear (
gets 50.00 m from
), or from a map that covers the profile
(e.g.,
Profile
|
Drawn On map
|
Labeled on map
|
Map
|
Ref. Elev.
|
Notes
|
|
x
|
x
|
|
49.14
|
|
|
x
|
|
|
(48.67)
|
Reference elevation can be determined from
(adjacent)
|
|
x
|
|
|
48.67
|
|
|
x
|
|
|
(50.55)
|
Multiple other reference elevations are given
|
|
x
|
|
|
(54.56)
|
Reference elevation given in
(given also in
)
|
|
x
|
|
|
(55.61)
|
Reference elevation given in
(given also in
)
|
|
|
|
()
|
(54.90)
|
Reference elevations are given in
|
|
|
|
()
|
(54.90)
|
Reference elevations are given in
|
|
|
|
|
49.14
|
Multiple other reference elevations are given
|
|
x
|
|
|
(56.06)
|
Reference elevation can be determined from
|
Table 6.3: Summary Information
for Byrsa III profiles. Reference elevations in parentheses are adjacent to the profile.
Map IDs in parentheses indicate that the profile is located on the map, but its extents are not
plotted or labeled.
gets 49.70 m from ). But
other times, no replacement can be found. This can happen even when there is a covering map, if the elevations
are
printed illegibly (as is the case e.g., for ), or not at all (as is the case e.g., for and ). This latter case is particularly
noteworthy—not a single one of the profiles published for the southwest corner of the Byrsa complex has a
reference elevation. It may be possible to determine approximate replacements from profiles and
168a-3, but these are purely reconstructive and were not at all intended for this purpose. As of this
writing, I have not been able to identify any elevation measurements in other published descriptions of this
area that could be used as replacements for the missing reference elevations. This is a major
problem. Without a corrective or supplementary publication from the original excavators of this
area, the elevation data encoded in those profiles could be permanently lost.
6.1.2 Problems with Mapped
Extents
Many profiles do not
have their extents clearly plotted on a map.
Generally, their extents can still be determined from a map, e.g., in the boundary of a trench (as with
profiles
and
on map
), or in the outline of a feature (as with profiles
and
382-1 on map
). For many profiles, the heart
of the problem is in labeling: a profile’s extents are
plotted on a map, but the profile itself has no label (e.g.,
), or the profile’s label is incorrect
(e.g.,
,
,
, and
),
or the extents on
the map have no label (e.g.,
,
,
,
,
,
, and
). For other profiles,
the heart of the problem is in plotting: a profile’s extents are plotted on a
map, but the extents are very imprecise (e.g.,
,
,
) or wrong (e.g.,
and
;
). Finally, for significant number of profiles, the extents are not
drawn at all (e.g.,
and
239;
).
6.1.3 Problems with Symbology
Sometimes it is difficult
to determine a profile’s extents from a
map because the profile is actually more of a perspective drawing, i.e., it is a projection of features from
multiple locations and angles onto a single plane. Such drawings can be completely continuous (e.g.,
), or they can have discontinuities (e.g.,
;
,
and
; and
,
, and
). While discontinuous profiles can
be straightforward when their extents are properly mapped
and labeled (e.g.,
), they can be difficult
or almost impossible to georeference when this is not
the case. This issue can be compounded when the extents are plotted on a map incorrectly (as with
),
or plotted on a map but not labeled (as with
). Sometimes, discontinuities are
not even shown in a profile, even
though they are obvious in a
photograph: this is the case with
, which
according to photograph
should show a gap
between
tombs
A144 and
A154 (these are the Feature IDs from
Byrsa II). Because this gap is
not shown, and because half of the profile is not captured in the photograph, I did not attempt to
georeference it.
6.2 Two Big Examples
To illustrate how the problems
discussed above can significantly
limit the available elevation data, it is helpful to consider the example of two profiles in particular.
B1.P.200 is the third-widest profile in Byrsa
I after B1.P.134 and (compared to which it is
considerably more detailed), and no other profile in any of the volumes stretches closer to the southeast
corner of the complex.
is partially colinear with
, but extends almost 40 m farther northwest,
crossing
through a large area (Punic block A) that has no other profiles, making it one of the widest and
potentially most important profiles in all of the Byrsa volumes.
6.2.1
The extents of profile
are clearly plotted and labeled in
map
(see Figures
6.4 and
6.5), but
several problems make the profile very difficult to
georeference. First, mapped extents have a width of 23.91 m on the georeferenced map, while the
printed width of the profile is 22.91 m. Second, the symbology of the mapped extents
indicates a discontinuity about 8.25 m northwest of the south endpoint, but the profile only shows a
discontinuity 18.75 m northwest of the south endpoint. Third, the grid cell labels given in the profile do
not match the grid cells that the mapped extents pass through on the georeferenced map. I found that the
most direct way to resolve these three problems was to focus on the third problem, so that is the approach
that I will take in this section.
The mismatch in grid cell labels can only be caused by one of
three things: a) the grid cells in map are
incorrectly labeled, b) the profile extents in map
are incorrectly plotted, or c) the grid
cell labels in profile are incorrect. I
will now
consider each option in turn.
-
The grid cells in map are not actually labeled, but the labels can be determined and applied by comparison with map ; the resulting labeled map is shown in Figure 6.4.
Therefore, the grid cell labels in are
correct.
- The positions of various features along the profile extents plotted in map
can be compared to the positions of corresponding features in profile . In ,
the
distance between the southern side of wall a and the next wall to the south (the ID for this wall
is not immediately clear) is about 8.17 m—this is consistent with the
distance evident in ,
omitting the discontinuity indicated by the map symbology. This observation indicates that the
discontinuity shown in the map was mistakenly omitted from the profile.
In , the distance between the southernmost
wall (ID again unclear) and the left endpoint is
about 4.70 m, which is greater than the distance of about 3.10 m in . This difference would be
eliminated if I assumed that the south end of the extents continues another 1.5 cm under and past the
map’s smudgy grid label, which is not unreasonable.
Finally, in , the distance between the
northern side of wall a and the right endpoint of
the profile is about 7.80m. This is significantly smaller than the distance of 10.31 m in . In the map, if I omit the segment stretching between and 10, which is parallel to the
discontinuity farther south, the distance in the map becomes 6.24 m, which is much closer to the
distance of 7.80 m in the profile. The remaining difference of 1.56 m is eliminated if I assume that the
north end of the extents continues to the middle of the triangle next to the profile extent label A'.
These observations indicate that the discontinuity shown in the profile was mistakenly omitted from the
map.
Based on these observations, the profile extents plotted in are basically consistent with
the
features shown in profile , although some
adjustments must be made to the north and south
endpoints.
- According to the grid cell labels in , the profile bisects cistern
E1 (labeled only in the profile) longitudinally in . Judging from the maps on which this cistern is plotted (e.g., and ; ),
this
situation is impossible: the cistern must be bisected in cell . From this, it is clear that at
least some of the grid cell labels in are
incorrect, rendering the rest of the labels suspect.
Based on the above considerations, it is clear that the profile
extents plotted in
are basically correct,
provided that the northern and southern endpoints are
adjusted, and that the grid cell labels in
are incorrect. The corrected labels are shown in Figure
6.5.
6.2.2
Profile
is presented almost without mention in
Byrsa
II: it is briefly cited only twice, in reference to the steep NW-SE slope along Punic roads II (
Byrsa II,
32) and III (
Byrsa
II,
46). On the surface,
the absence of discussion for this profile seems very strange: at a printed width of 62.76 m, this profile
is one of the three biggest profiles in all of the
Byrsa volumes. On close inspection, it becomes clear that features within the first 22.40 m of the profile
(beginning from the left endpoint) overlap perfectly with features in
. Therefore, the leftmost
22.40 m of
are colinear with
. The profile’s point labels strengthen this
association: for
both
and
, the left endpoint is marked A and the right endpoint is marked A’.
Two main problems make the rest of profile exceptionally
difficult to georeference. First, the extents are not plotted on any map. This problem is unexpected, because the profile
clearly has point labels, and essentially every other profile with point labels in the Byrsa
volumes has its extents plotted on some map. Second, the profile’s symbology does not indicate any
discontinuities over the segment that is colinear with , so it is clear that I need to deduce the
discontinuities in the rest of the profile myself.
To make the georeferencing process easier to follow, I broke the
portion of the profile that was not colinear with
into five segments (Figure
6.6). Segments 1 and 2 traverse Punic block
C, an area
that is covered by many other profiles in the
Byrsa volumes, and upon closer inspection it appears
that the segments are actually composites of these other profiles. Consequently, I have only georeferenced
segments 3, 4, and 5.
6.2.2.1 Segment 5
Segment 5 (Figure
6.7) shows a
transverse cut through a cistern (width 2.24 m), almost immediately adjacent to the base of a wall whose
width (0.95 m) and top elevation (53.60 m) almost perfectly match those of
in map
m. In
this map,
is 0.66 m away from the
remains of a parallel cistern whose transverse width of 2.09 m
is very similar to that shown in the profile. There are no other walls and cisterns in my initial dataset
which match the profile’s features as closely as these, so I must conclude that they are the features shown
in the profile, and I digitize the cistern as the following features:
,
, and
.
Given those assignments, it is to determine the identity of the
remaining feature. About 0.71 m to the left of the cistern, segment 5 shows a longitudinal cut of a tomb
(width 1.92 m). Multiple tombs can be seen around this area in maps and ,
but only one of
them matches the width shown in the profile: tomb A192 in (printed width 1.98 m).
Consequently, I conclude that it is the tomb shown in the profile, and I digitize it as .
The assignment of the tomb reveals several important points.
Firstly, the cut through the tomb is not parallel to the cuts through
and the cistern, so the
profile is clearly a bit of a perspective drawing. Secondly, the north side of
is 3.14 m away from the south side of
,
which is much
larger than the 0.71 m shown in the profile. I conclude that there is a hidden discontinuity in the profile.
Finally, judging from the assignment of features in segment 4, the remaining distance of 1.19 m hides
another
discontinuity.
6.2.2.2 Segment 4
Segment 4 (see Figure
6.8) shows
a wall (width 0.69 m) immediately adjacent to (and left of) a longitudinal cut through a cistern (width 6.62
m), which is almost immediately adjacent to (and right of) a second wall (width 0.66 m). Simply put, this
configuration is almost identical to the configuration of walls (
,
) and cistern shown
in the center of Punic block A in map
.
Consequently, I conclude that those are the walls shown in
the profile and I digitize the cistern as
,
,
, , , and .
Notably, the profile omits the piece of that cuts into
the cistern, and there is a short hidden discontinuity between and .
6.2.2.3 Segment 3
Segment 3 (see Figure
6.9) shows
a transverse cut through two parallel and adjacent tombs (combined width 1.77 m), located about 2.55 m from
wall
of segment 4. This
configuration almost perfectly matches tombs
A183 and
A184
in map
. Since no other tombs seem to fit as
well as these, I conclude that they are the ones shown
in the profile, and I digitize them as
and
.
The profile indicates a discontinuity at the left edge of
, which constitutes the end of
segment 3.
6.3 Deeper Problems
The last two sections have made it clear that the profile drawings
of the Byrsa volumes suffer from numerous problems that make them harder to geolocate and
interpret. These problems can obscure or erase the elevation measurements for critical areas of the site,
e.g., as happened with and all of the
profiles of the southwest corner. The loss of such data
should be of central concern to scholars of the Byrsa Hill. Archaeology is a science in three dimensions,
especially on this site: the Roman Byrsa complex represents a tremendous stratigraphic project, in which the
slopes of the natural hill were blanketed in the detritus of its own destruction, piled in drifts many
meters high and subsequently anchored in place with substructures, foundations, and retaining walls. The
loss of yet more elevation data threatens to permanently occlude our understanding of that project.
How did these problems happen? Why were they not caught upon
publication, or corrected in the 40 years since? I do not believe that I have the final answers to these
questions, but I do have some ideas.
Some fault must lie with the
strategies and decisions that
determined how the
Byrsa volumes' text, maps, and profiles were first composed. When an entire
excavation report is published without any elevation measurements in its maps or profiles (as with the
southwest corner; see Section
6.1.1), or when
an
entire collection of profiles is drawn without
any way to determine
their extents on a map (as with the many
profiles from Byrsa III: 131-133; see n.
169), or when the grid cell labels in a
profile do not match those in the figure captions or text (as with
; see Section
6.1.2
and n.
168), something is wrong with the writeup process itself. The
last of those problems, I think, offers some further insight into the situation: the researcher(s) who wrote
the captions and text were not the same people as those who drew the profiles and maps.
Some fault also must lie with the publisher's editorial decisions,
which determine not just the style and shape, but also (to some extent) the
content of the final
(yet “preliminary”) site publications. The example of
is particularly illustrative in this regard.
Why was one of the biggest profiles of all of the
Byrsa volumes, which for some areas is the sole
source of published elevations data, and which was clearly drawn with point labels and multiple reference
elevations—why was this profile not given mapped extents and printed so small that most of the elevations
are illegible? The simplest (and, I think, most likely) answer is that the prospect of printing two more
large foldout pages, which would have been required to reproduce
at the same scale as
as
well as a map of the extents, was deemed too expensive, since the book already was replete with large
fold-out maps and profiles. From a financial perspective, the omission of the mapped extents and the shrinkage of
make
some sense. It is expensive to print large, detailed figures; put another way, it is expensive to print full
datasets that ensure a publication’s analyses are reasonably reproducible.
Fault aside, why have these problems not provoked prior criticism?
I have been unable to find any publication to date that offers such critique of the Byrsa volumes.
Many of the problems I have pointed out seem obvious, given the data that I have shown. And therein, I
think, lies the answer: it took five to six months of work for me to be able to begin digitizing the profile
extents and collecting those data. Granted, three of those months were spent diagnosing and correcting
distortions in Persée’s digitized copies of Byrsa I and III, but even so, the remaining
two to three months represent around 300-500 hours of work, several weeks of which was spent reconstructing
the reference grid. I think that the main reason no one has previously published such a critique of the
Byrsa volumes is that no one else has had the necessary tools, time, and interest. The data in
these books had to be fundamentally re-structured before problems could really be identified. This is a
major barrier to research on this site.
The existence of this barrier points, I think, to an even deeper
issue with how archaeologists manage and publish their data. This issue is tied to the division of labor
between archaeologists and technical illustrators, and to the publication paradigm that structures the
relationships between archaeologists and their publishing editors. This is the issue that I will discuss in
my next and final chapter.
Chapter 7 Conclusions: Reforming the
Publication of Archaeological Research
“Final publication begins the day the first pick goes into the
ground, indeed,
before that, in our conception of the project” (
Dever 1996,
43)
“L'Afrique carthaginoise est devenue française : c'est nous, à présent, qui sommes
les Romains.”
“Carthaginian Africa has become French: it's us, now, who are the Romans.”
(
Babelon 1896,
116)
My collation, digitization, and re-organization of the archaeological
data on the Byrsa complex have highlighted how recurrent problems in archaeological data management have
significantly limited our understanding of the site, particularly in the Augustan period. These problems are
long-standing, and they are persistent: while the systematic methods and analyses of the French Mission
represent a great improvement over the piecemeal efforts of Beulé, Delattre, Lapeyre, and Ferron and Pinard,
their publications suffer from some of the same fundamental problems as their predecessors. At times, these
problems overshadow the improvements, because they make it difficult—and sometimes impossible—to critique or
confirm old interpretations, or to re-use the data to answer new
questions. By re-structuring the data into a
single internally-consistent dataset, I have made it much easier to do just that. In this chapter, I will
discuss these old problems, new interpretations, and new questions.
Before I begin my critiques, I must acknowledge that much of this work
would not have been possible without some major advancements in the open publication of old archaeological
publications on the Byrsa. Without the digitization and online re-publication of
Beulé (
1861), Delattre (
1893a;
1893b;
1894),
Saumagne (
1924b),
Lapeyre (
1934), and Ferron and
Pinard (
1955;
1960), most of which are out of
print and not commonly held by anglophone universities, my dataset, analyses, and interpretations would have had
very little historical depth and the scope of this project would have been greatly reduced. Links to these
sources are included in my Bibliography.
7.1 Old and Common Problems
Most of the problems with the management and publication of
archaeological data on the Byrsa Hill fall into three categories: problems related to the distance between
archaeologists and technical illustrators, problems related to the distance between different archaeologists,
and problems related to the distance between archaeologists and publishing editors. I will discuss each of these
problems in turn.
7.1.1 Distance Between the
Archaeologist and the Technical Illustrator
The most visible problems that my study has highlighted concern the
collection of published maps and the profiles that make up my initial dataset. Put simply, the geolocatability,
accuracy, and symbology of the published maps and profiles are often compromised, making them harder for other
scholars to understand and re-use. I believe this results from a general disconnect between the (archaeological)
illustrator and the archaeologist (writer). This disconnect prompts the question of what the role of a map
should be in an archaeological publication.
None of the early
maps of the Byrsa Hill follow a coordinate system,
nor do they provide reference datums—perhaps unsurprising, since most of them were produced by architects (e.g.,
Bonnet-Labranche, Thouverey), rather than geographers or cartographers. Consequently, they are not directly
geolocatable.
In contrast, the maps of the French Mission were created within a standard geographical coordinate
reference system and linked together with a single, site-specific coordinate system, but, as I showed in Chapter
4, the second system was not fully published, and the two systems were
never linked in the publications. The biggest improvement in the maps of the French Mission is their
accuracy—while it is difficult to find a reference dataset for comparison, their maps are certainly more
accurate than those of their predecessors. The biggest shortcoming of the maps of the French Mission is their feature symbology, which is often more
ambiguous than their predecessors, making it difficult—and sometimes impossible—to distinguish between extant,
reconstructed, and hypothesized features.
As I explored in Chapter
6, problems with ambiguous symbology can also be found in the
profiles of the
Byrsa volumes, which often “project” (i.e., unfold) features from multiple different
planes onto the plane of the illustration. This process of projection can create discontinuities that are not
always shown in the profile (e.g.,
), or the
mapped extents (e.g.,
, with extents plotted in
), making the profile much more difficult to
interpret. This problem is compounded by another problem,
the tendency to not plot and/or label profile extents on a map at all. This omission can make profiles very
difficult (e.g.,
) or even impossible (e.g.,
profiles from
Byrsa III,
131-133; see n.
169) to georeference. Some profiles that
are georeferenceable are still mostly useless, because their reference elevations have been omitted (e.g.,
profiles for the southwest corner) or made illegible (e.g.,
).
In a project of the magnitude of the
Byrsa volumes, some
inconsistencies and errors are bound to crop up, but the sheer quantity and scale of the problems with the maps
and profiles, combined with the disregard for them in subsequent publications, suggests to me
that there is a
deeper issue at work: those who make the maps and profiles are not the same people as those who write about
them.
The simple fact is that since the beginning of the discipline, many,
if not most, archaeologists of the Mediterranean have been unable (or unwilling) to draw their own maps and
profiles, relying instead on architects, cartographers, or artists for their technical illustrations. While this division of labor tends to produce illustrations that are clean, professional, and often quite
beautiful, it also creates a multitude of problems, not simply logistical (how does the archaeologist coordinate
the illustrators with the excavators?), or ethical (how should the illustrator be credited?), but also, as I have shown through numerous examples in Chapters
5 and
6,
epistemological. In the context of the Byrsa Hill, this division is partly why later scholars of the
site, when reproducing or citing problematic maps and profiles from the French Mission, have tended not to point
out or engage with those problems. More broadly, this division is one of the main reasons why
archaeologists very commonly do their analyses
and write their reports using maps and profiles that are different
from maps they publish. As long as this
practice continues, publications will continue to be produced that do
not actually report the data on which their results are based.
7.1.2 Distance Between
Different Archaeologists
Given that the
Byrsa Hill has been the subject of excavations for over
160 years, it is striking, but not surprising, how disjointed and insular the efforts of various researchers
have been. Delattre, in his published work, largely avoided the places where Beulé had excavated,
and the same is mostly true for Lapeyre. Consequently, as I outlined above in Chapter
3, the excavation history of the Byrsa is a patchwork, with
excavations conducted all over by different researchers with different motivations, frameworks, and approaches.
The prevailing attitude seems to have been that in places where
excavations had already occurred, there could not be any more remains of interest. This attitude is to some
extent understandable. Firstly, each of the major campaigns was separated from the others by 20-30 years, and
during those interludes features which had been uncovered were deteriorated due to a combination of spoliation
and erosion. Secondly, the fixation of all of the excavators on tombs and inscriptions, combined with their
penchant for large, open-air excavation methods, all but ensured that no material of interest to them would
remain in a given area after a single campaign there.
On the other hand, this attitude was also an outgrowth of the colonial
explorer mentality that has characterized most of European and North American archaeological research in North
Africa—and many other places around the world—since the beginning of the discipline. Very often, the “discovery”
and excavation of a feature bestows some sort of
ownership of it, in name if not in deed. This is why scholars still
sometimes refer to the apses of the eastern basilica as “Beulé’s Apses,”
and
to wall
D as “Mur Lapeyre:” the association of a publication with a feature or set of features has long
been sufficient to warrant subsequent attribution within the archaeological community, and as with appellations
coined by other sorts of colonial explorers (Bombay, Mount Rushmore, Lake Victoria, etc.), such names have a
tendency to stick. For Delattre and other subsequent excavators, the prospect of re-examining the site of a
previous excavation was far less attractive than starting a new one, ideally in mostly unexplored area, where
the chances of uncovering new tombs, inscriptions, and impressive architectural features were much higher. This
preference for creating personal scholarly domains is evident, e.g., in the idiosyncratic (or non-existent)
notation systems used in the different campaigns to refer to specific features, and in the tendency of each campaign to omit features found by other excavators in their own maps. The result of this mentality is that, with a few exceptions, for more a century, excavations on the Byrsa largely functioned as isolated scholarly domains.
The excavators of the French Mission of the 1970s and 80s were the
first to attempt to unify these disparate domains into a collection of more-or-less coherent datasets, which
they presented in individually-authored site reports. To some extent, they were successful: this thesis is a
testament to that success, since the overwhelming majority of my data
are
sourced from their excavations. But as
I discussed in Chapters
5 and
6, the process of integrating these datasets reveals numerous
inconsistencies in the overlaps and gaps between them. Some features are described by multiple excavators in
significantly different ways—such was the case with the
B piles (made with cement or mortar?) and the
E piles (bound with dirt or clay?). Other features are basically not described at all, either due to a simple lack of prioritization, as
happened with the south slope retaining wall (see Section
5.1.1.7) and wall
G (see Section
5.1.1.2), or due to a misunderstanding, as with the western
C piles.
These problems are exacerbated by the absence of an inventory, index,
and precise ID system for extant architectural features in the
Byrsa volumes. The investigations of Roman architecture in these volumes are characterized by a search for extant
sections of previously recognized, pre-defined features. Granular identification is eschewed for small,
recognizable names such as “wall
D,” and “pile
C1.”
While this system generally works well for a
small set of features that are obvious and well-defined—a description
which admittedly applies to many of the
Roman remains on site—it has some notable shortcomings. First, it does
not discriminate between sections of a feature, which creates
ambiguities for very large or
partially destroyed features (also applicable to most of the Roman
remains) and makes it difficult to tell
whether a feature under discussion has been actually found, or was
only hypothesized or reconstructed. Second,
their ID system is not
systematically extensible, that is, it does not seem to follow a set of
rules that
could be used to uniquely identify a large number of additional
features. Finally, many important features are
not assigned an ID at all, and given the lack of an index or
inventory, this can make it very difficult to determine where (or even
whether) they are discussed in the
Byrsa volumes.
7.1.3 Distance Between the
Archaeologist and the Editor
Many of the problems in the previous two categories are reinforced
by
constraints imposed by the systems of archaeological publication. A book-length primary site publication cannot
be constructed around a systematically extensible feature ID system if the publisher is not willing to provide
the editing resources required for a large and robust cross-referencing system. Similarly, such a publication cannot include a comprehensive dataset if the publisher is not willing to
print a large number of high-quality maps, profiles, and many pages of find inventories. While these
restrictions are to some degree out of aesthetic or rhetorical concerns, the primary motivation is economic. For
essentially all archaeological publishers, the first concern must be whether a product will be financially
feasible. When a book’s expected sales are numbered in the hundreds, rather than the thousands, publishers are
often unwilling to pay the costs required for overcoming these problems, because their very existence is
dependent on how well their products suit the market.
In addition to the
economic considerations, there are professional
factors at play. For over a century, excavations on the Byrsa Hill were almost exclusively conducted by public
officials and priests who were curious, well-connected, and largely untrained. These were amateurs—in the
original sense of the word—and their goal was not to compose comprehensive writeups of their excavations, but to
communicate their most exciting finds to their wider, and also largely amateur, audience.
After Beulé’s singular, self-funded expedition and monograph chapter (
1861,
1-84),
the next century of publications on the site was dominated by small,
bite-sized communications (e.g., Delattre
1893a;
1893b;
1894;
Saumagne 1924b) with some very uncommon longer articles
(e.g.,
Lapeyre 1934) or thesis sections (e.g., in
Audollent 1901). The systems of
archaeological publciation in these decades
prioritized small, self-contained preliminary reports, discouraging the collation and organization of data into
unified frameworks or archives. Of course, this relationship was complex (excavators had many different priorities
aside from
publishing), and recursive (the publications that excavators read probably somewhat influenced how they wanted
to excavate). Yet, the fact is that no publication longer than Beulé’s monograph chapter was produced until
Ferron and Pinard (
1955), and no wider-ranging, more comprehensive publication was produced until
Byrsa I (published 1979).
It almost goes without saying that the vast majority of the data not
published by Beulé, Delattre, Lapeyre, and other excavators has been lost. The result of this is that for at
least the last 50 years,
researchers on the Byrsa have been forced to
rely on tiny, scattered, data-poor publications to make arguments that those publications were often never
intended to support. As I have shown in the sections above, despite some notable improvements, this problem
continued to persist in the
Byrsa volumes through the omission of critical data in many of the maps and
profiles, and in the absence of a robust feature identification and reference system. This abridgement and lack
of structure in the published data is threatening to become permanent, because many of the original excavators
of the French Mission have passed away and there is still no publicly-identified, centralized archive of their
excavation documents.
7.2 Reforming the Publication of
Archaeological Research
As I discussed in Chapter
1, these
problems of publication are endemic, not just in the archaeology of Carthage, but in Mediterranean archaeology
more generally. Although they have, in some circles, occasionally provoked genuine inquiry (e.g.,
Frere 1975;
Cunliffe 1983;
Carver et al. 1992) and introspection (e.g.,
Richards 2004;
Pollock 2010;
Morgan 2013), the problems have
proven largely intractable, and according to some (e.g.,
Dever 1996;
Shanks 1996b;
Herzog 1996), they have grown
significantly worse. The lack of
concerted research
on this topic (with the exception of the edited volumes
Shanks 1996a and
Shanks and Magness 1999) makes it
difficult to definitively confirm such an assessment at the scale of the entire field, but at the scale of
subfields and specific sites it is often painfully obvious.
I believe that this predicament constitutes an existential threat to
the field, because it threatens our academic integrity, it is incredibly wasteful for researchers of legacy
data, and it harms the mental and financial health of the multitude of archaeologists who have not been trained
to efficiently and sustainably collect, analyze, and publish data at the scale of an entire site. The threat to
our academic integrity has already been pointed out, e.g., by
Herzog (
1996,
103-104), who noted that absent or incomplete publications create inequities in
data accessibility. This makes it very difficult, and sometimes impossible, for other researchers to critique
the excavators' results or propose alternate interpretations of their published data, since the excavators are
privy to meaningful information that has not yet been published. When additional publications are not forthcoming, because the site director has moved on to another
project or (more often) passed away, they often take with them an intimate knowledge of the organization and
contents of their datasets, leaving behind scant documentation of these topics for future researchers and making
the task of consuming, synthesizing, and arranging the remaining data for publication far more expensive than it
already was. Sometimes, the cause for such languishing is not that the site director left or passed away, but
that they simply cannot manage the data themselves. Perhaps the dataset has become too sprawling and variegated
for them to effectively understand (
Dever 1996,
42;
Jacobs 1996,
71); or maybe they have run out of funding, their
grant money having mostly
gone toward excavation (
Mazar 1996,
27;
Dever 1996,
40); or perhaps the prospect of
organizing, tabulating, composing, and typesetting their data and analyses, with no guarantee of a publisher,
for years on end, has simply (and quite understandably) overwhelmed them—as
Shanks (
1996b,
51) puts
it,
“The archaeologists who fail to publish are not, for the most part, bad people. They are
not disinterested or intentionally neglectful or lazy. They fail to publish, for one reason or another,
because they can't. They simply cannot do it. It is a mountain they cannot climb whether for legitimate or
psychological or other reasons. In short, they need help. And it should be the task of the profession to
find some means to give them that help.”
This crisis requires a combination of solutions. First, we must
rethink and redefine what it means to properly publish archaeological research. It has been clear for quite some
time that the monograph is not well suited to the task of publishing data at the scale of a site. It is terribly
tedious and inefficient to typeset thousands of pages of documentation, drawings, and spreadsheets into a
manuscript, and it is terribly expensive to print it. The rise of digital publication technologies has offered
an unprecedented opportunity to rethink the publication norms of our field, enabling researchers to forego the
costs of printing and to use more flexible formats than manuscripts. These formats include self-published online
databases (e.g.,
Bates 2019;
Manière, Crépy, and Redon 2020),
interactive site maps (e.g.
Aksoy and
Bayar 2016;
Townsend et al. 2020), and
linked-data e-books (e.g.,
Opitz,
Mogetta, and Terrenato 2016). Unfortunately, such technologies
remain significantly under-used, in no small part because they tend to be under-represented in Review, Tenure,
and Promotion (RPT) requirements. There needs to be a concerted effort to redefine RPT requirements to encourage
such publications.
Second, there must be a curricular shift toward data management and
digital publication. Far too many archaeologists, particularly in the Mediterranean, never complete coursework
on data management. Instead, they learn the data recording and organizational strategies of their advisor, or
perhaps their colleagues, on the fly. Without formal training, it can be difficult to create a data management
plan that is comprehensive (describing all data collected within the project), easy for other researchers to
understand, flexible enough to accommodate the addition of new types of data, and systematically extensible to a
sufficiently large number of loci. Similarly important (and under-used) is coursework on digital
publication. All of the digital publishing formats mentioned in the previous paragraph require a significant
amount of training to create, and if researchers do not have at least some experience with them, they are
unlikely to seek out such training on their own. Moreover, it is often very difficult for an archaeologist to
effectively use such technologies if she did not factor them into her original data management plan.
Third, we must change the mentality—still all too common in our
profession—that the publication of site reports represents a necessary evil and the “last stage of research”
(
pace Herzog 1996,
88). Complete and open
communication is essential to scientific inquiry and academic community. If it is prohibitively difficult to
communicate one’s data completely and openly, then something has gone wrong. Doing archaeological research
should be predicated on participating in the archaeological community—in other words, excavation should be
predicated on publication, not the other way around. The reticence of many project directors toward full
publication belies the nature of the threat posed by publication delays: the greatest risk of a project director
moving on or passing away is not that their interpretations will be lost. The greatest risk is that their
knowledge and understanding of
the data recording, collection, and
structuring schemes will be lost, that future
researchers will not know where the excavation records are stored, how they can be accessed, or how they are
organized. This is how unpublished excavation records vanish: when the people who created, organized, and used
them have passed away, their unorganized papers and undocumented personal archives are left to colleagues and
relatives to whom they have little or no importance, and who eventually place them in perpetual storage, or
worse, throw them away. Data must be published before they are actually useful, or as
Dever (
1996,
47) puts it, “unpublished data are not data
at all.” Publication represents the first stage of research, not the last.
In this thesis, I have demonstrated that it is possible to restructure
old archaeological data in a sustainable and systematically extensible way. There are undoubtedly flaws and gaps in my work, but I was still able to resolve many of the problems
inherent in prior publications. I have also demonstrated that the restructuring of old data can give rise to new
interpretations and questions about a site, some of which were not possible within the old organizational
framework. In the final section of this chapter, I will discuss some of those interpretations and questions for
the Byrsa Hill.
7.3 What can we do with Restructured
Data?
The restructured dataset has enabled new interpretations about the
design and development of the Byrsa complex, particularly with regards to the substructural walls and perimeter
structures in and along the complex’s southern side. Some of these interpretations require additional proof,
highlighting certain areas of the site and certain questions for further investigation.
7.3.1 New Organization Enables
New Interpretations
The most
significant new interpretation that I have proposed above is
that the Phase 1 substructural systems and perimeter structures and of the Byrsa complex were constructed in a
modular, piecewise fashion. This flexible approach allowed construction crews to adapt more easily to the local
availability of stone rubble from the Punic destruction layer, while still following the original design of the
complex. The approach is evident in wall
D’s variable and somewhat crooked construction, both of which
were obscured by the reductive symbology used to depict it in the maps of the
Byrsa volumes. The
approach is also evident in the vastly different dimensions and construction of the apses lining the
southwestern, southern, and eastern apses. The apses of Series 1 and 2 were significantly wider and had much
thinner walls than the apses of Series 3.
The apses of Series 3 themselves exhibited a remarkable shift in dimensions, growing significantly wider
from west to east, and they seem to have been significantly longer than the apses of Series 4, although I
believe that this last discrepancy may have been at least partially made up for by
a now-missing stone lining.
This interpretation contrasts with previous characterizations (e.g.,
Deneauve 1990) of the Augustan-era
construction project, which have emphasized the unity of the complex's design and execution.
I have also proposed several smaller interpretations that still want
for additional proof. First, I showed that the late dating of the B
piles that was proposed by the original excavators seems
questionable, and I suggested some reasons why a Phase 1 dating may
make more sense. Second, I proposed an order and rationale for the
development of the substructural walls of the Phase 2 southwest
temple, and showed how the interaction between these walls and the B piles and C piles was
probably more complicated than previously acknowledged. Third, I reconstructed the approximate extents of the
amphora wall in the southeast corner of the complex, and showed that it may have functioned in concert with the
southeast staircase nearby. Finally, after pointing out that the previously proposed dimensions of the Phase 1
eastern apses have no basis in material evidence, and in fact contradict the construction strategies used in the
southwest corner of the complex, I hypothesized that the Phase 1 dimensions may have been identical to the Phase
2 ones.
7.3.2 New Interpretations
Prompt New Questions
These preliminary interpretations and hypotheses highlight the
attractiveness of certain areas of the site for further investigation, and prompt new questions about the
complex’s design and development. A fuller excavation (and publication) of the substructural walls of the Phase
2 eastern basilica would probably provide helpful constraints on the dimensions and design of the building’s
Phase 1 predecessor, particularly in the southwest corner, where the building’s substructures met wall
D’
(built in Phase 1). A new field survey
of the substructural walls of
the southwest temple would clarify their
extents and their stratigraphic relationships with one another, which would in turn clarify their order of
construction; an archival survey could supplement the fieldwork with elevation measurements from the primary
excavation documents on this sector. Targeted excavations around the southeastern perimeter would almost
certainly clarify the (very hypothetical) layout of this part of the complex, including the original extents of
the amphora wall and the original dimensions of the apses and/or other retaining walls, but this entire area
appears to be underneath modern homes and businesses, so even limited excavation is unlikely to be possible in
the foreseeable future.
The complex’s design
and development could be greatly clarified by
making a serious investigation of the structural requirements imposed by topography of the Punic destruction
layer and the volumes of earth and debris found above it. In the past, excavators have tended to make vague
statements about the role of the apses, the substructural walls, and the foundation piles in resisting outward
pressure from the Augustan embankment. These statements are very shallow, from an engineering standpoint. What
sorts of pressures did these structures need to resist? How large were they, and in what directions? How did
these pressures change over time, as the soil naturally shifted, compacted, and creeped? How did these changes
influence the decisions which governed the construction of Phase 2 structures? These are necessary questions,
but they cannot be answered without a comprehensive dataset describing the topography of the Punic destruction
layer and the vertical and horizontal extents of all of the Roman and Punic features. As my preliminary work in
Chapter
6 seems to indicate, such a dataset may well be
obtainable at least for the southern part of the complex.
Such a dataset could also reveal how the Phase 1 Roman construction
crews navigated the site’s Punic remains. By integrating the horizontal and vertical extents of both Roman and
Punic features, we could determine how the various Roman substructures cut, abutted, and included Punic walls,
cisterns, tombs, and other features. This would offer insight into what sorts of Punic features the Phase 1
Roman construction crews would have seen during their work, and what they, or their superiors, decided to do
about them. Which Punic walls were removed to make way for Roman ones, and which ones were merely included? How
many tombs did the construction crews encounter, and how many did they fully or partially destroy? How might the
presence or discovery of tombs have influenced the construction decisions that followed—e.g., as in the
southwest temple? These, too, are necessary questions, which cannot be answered without restructuring the
current architectural dataset for the Byrsa complex.
These questions touch on a deeper theme underlying the foundation of
the Roman colony at Carthage, a theme that has been largely neglected by modern scholars of this site: the role
of reconstruction and erasure in shaping public and private narratives about the past and present. Still bearing
the physical and psychological scars of the recent violent upheavals at the end of the Republic, the Romans who
labored on the colony’s foundation literally took apart the remains of their country’s greatest geopolitical
rival—and deeply despised nemesis—stone by stone, and then they re-made the city in Rome’s own ideal image. What
did this project mean to the laborers, surveyors, architects, artisans, and soldiers who undertook it? What did
it mean to their families and children? How did it influence their perception of the new political order? These
are questions that can and should be asked of this site. By collating, digitizing, restructuring, and
re-publishing archaeological
data from the Byrsa Hill, I have begun to
make that asking possible.
References
Aksoy and Bayar
2016Aksoy, Can and Bayar,
Ziyacan, "Archaeological Ethnography of the Battle of Aslıhanlar
(29–30 August 1922): A Case Study of Public Archaeology, Visual Storytelling, and Interactive
Map Design", European Journal of Archaeology
19, 1 (2016),
pp. 68--94.
Alperin et al.
2021Alperin, Juan Pablo,
Schimanski, Lesley A., La, Michelle, Niles, Meredith T., and McKiernan, Erin C., "The Value of Data and Other Non-Traditional Scholarly Outputs in Academic
Review, Promotion, and Tenure in Canada and the United States", in Open Handbook of Linguistic Data Management (Cambridge, MA: MIT Press, 2021).
Altekamp and
Khechen 2013Altekamp, Stefan and
Khechen, Mona, "Third Carthage: Struggles and Contestations Over
Archaeological Space", Archaeologies 9, 3 (2013), pp.
470--505.
Architecture
2018Architecture,
Forensic, "The Destruction Of Yazidi Cultural Heritage",
Forensic Architecture (2018).
Audollent
1901Audollent, Augustus Marie
Henri, Carthage romaine, 146 avant Jésus-Christ-698 après
Jésus-Christ (Paris: L'Université de
Paris, 1901).
Babelon 1896Babelon, Ernest, Carthage (Paris: E. Leroux, 1896).
Bates 2019Bates, J., "The
Published Archaeobotanical Data from the Indus Civilisation, South Asia, c.3200–1500BC",
Journal of Open Archaeology Data 7,
0 (2019), pp. 5.
Benichou-Safar
1976Benichou-Safar,
Hélène, "Carte Des Nécropoles Puniques de Carthage",
Karthago XVII (1976), pp. 5--35.
Bernbeck 2010Bernbeck, Reinhard, "Heritage Politics: Learning from Mullah Omar?", in Controlling the Past, Owning the Future: The Political Uses of
Archaeology in the Middle East (Tucson: University of Arizona Press, 2010),
pp. 27--54.
Bernbeck and
Pollock 2016Bernbeck, Reinhard
and Pollock, Susan, "`Grabe, Wo Du Stehst!' An Archaeology of
Perpetrators", in Archaeology and Capitalism : From Ethics
to Politics 1st edition (New
York: Routledge, 2016), pp. 217--233.
Beulé 1861Beulé, Charles-Ernest, Fouilles à Carthage aux frais et sous la direction de M. Beulé
(Paris: Imprimerie Impériale,
1861).
Boivin 1997Boivin, Nicole, "Insidious or Just Boring? An Examination of Academic Writing in
Archaeology", Archaeological Review from
Cambridge 14, 2
(1997), pp. 105--125.
Callot 1986Callot, Olivier, "La
région nord du palais royal d'Ugarit", Comptes rendus des séances de
l'Académie des Inscriptions et
Belles-Lettres 130, 4 (1986), pp. 735--755.
Campbell 2007Campbell, Gordon, "Beulé, Ernest-Charles-Auguste", in The
Grove Encyclopedia of Classical Art and Architecture (Oxford: Oxford University Press,
2007).
Carver et al.
1992Carver, Martin O. H.,
Chapman, Hugh, Cunliffe, Barry W., Hassall, Tom G., Hebditch, Max, Lawson, Andrew, Longworth,
Ian, Morris, Richard, Phillipson, David, Schofield, John, and Wainwright, Geoffrey,
"Archaeological Publication, Archives and Collections: Towards a National
Policy", British Archaeological News 7 (1992).
Cronin and La Barre
2004Cronin, Blaise and La Barre,
Kathryn, "Mickey Mouse and Milton: Book Publishing in the
Humanities", Learned Publishing 17, 2 (2004), pp.
85--98.
de Chateaubriand
1859de Chateaubriand,
François-René, Itinéraire de Paris à Jérusalem et de Jérusalem
à Paris (Paris: Garnier,
1859).
Cunliffe 1983Cunliffe, Barry W., "The Publication of Archaeological Excavations: Report of a Joint Working Party
of the Council for British Archaeology and the Department of the Environment", Department of the Environment (1983).
Curl 2006Curl, James Stevens, A Dictionary of Architecture and Landscape Architecture Second (Oxford University Press,
2006).
Davin 1930Davin, Paul, "Etude sur
la cadastration de la Colonia Julia Carthago", Revue
Tunisienne 2 (1930), pp. 73--85.
Delattre 1891Delattre, Alfred-Louis, "Tombeaux puniques de Carthage: Nécropole de la colline de Saint-Louis",
Revue Archéologique XVII
(1891), pp. 52--69.
Delattre 1893aDelattre, Alfred-Louis, "Fouilles archéologiques dans le flanc sud-ouest de la colline de Saint-Louis
en 1892", Bulletin archéologique du Comité des travaux
historiques et scientifiques (1893), pp. 94--123.
Delattre
1893bDelattre,
Alfred-Louis, "Un mur à amphores romaines découvert à l'angle sud
de la colline de Byrsa (Carthage)", Comptes rendus des
séances de l'Académie des Inscriptions et Belles-Lettres 37,
3 (1893), pp. 152--155.
Delattre 1894Delattre, Alfred-Louis, "Le mur à amphores de la colline Saint-Louis à Carthage", Bulletin archéologique du Comité des travaux historiques et
scientifiques (1894), pp. 89--119.
Deneauve 1983Deneauve, Jean, "Le
tracé monumental de Byrsa à l'époque romaine: État des recherches",
Cahiers des Études Anciennes 16
(1983), pp. 89--106.
Deneauve 1990Deneauve, Jean, "Le
centre monumental de Carthage: Un ensemble cultuel sur la colline de
Byrsa", in Histoire et Archéologie de l'Áfrique du Nord:
Carthage et son territoire dans l'Antiquité: Actes du IVe colloque international sur
l'histoire et l'archéologie de l'Afrique du nord vol. I,
(Paris: Comité des Travaux Historiques et
Scientifiques, 1990), pp. 143--155.
Dever 1996Dever, William G., "The
Importance of Research Design", in Archaeology's Publication
Problem vol. 1, (Washington,
DC: Biblical Archaeology Society, 1996),
pp. 37--48.
Duval 2005Duval, Noël, "In
memoriam Serge Lancel (1928-2005)", Revue d'Etudes Augustiniennes et
Patristiques 51, 2 (2005), pp. I-V.
Effros 2018Effros, Bonnie, Incidental Archaeologists: French Officers and the Rediscovery of Roman
North Africa (Ithaca, NY: Cornell University Press, 2018).
Ennabli 2020Ennabli, Abdelmagid, Carthage: "Les Travaux et les Jours": Recherches et Découvertes
1831-2016 (Paris: CNRS
Éditions, 2020).
Estabrook and
Warner 2003Estabrook, Leigh and
Warner, Bijan, "The Book as the Gold Standard for Tenure and
Promotion in the Humanistic Disciplines: Report for the Committee on Institutional
Cooperation", Committee on Institutional Cooperation
(2003).
Faniel et al.
2013Faniel, Ixchel, Kansa, Eric,
Kansa, Sarah Whitcher, Barrera-Gomez, Julianna, and Yakel, Elizabeth, "The
Challenges of Digging Data: A Study of Context in Archaeological Data
Reuse", in Proceedings of the 13th ACM/IEEE-CS Joint
Conference on Digital Libraries (New York, NY,
USA: Association for Computing Machinery, 2013), pp. 295--304.
Ferron and Pinard
1955Ferron, Jean and Pinard,
Maurice, "Les Fouilles de Byrsa: 1953-1954", in Cahiers de Byrsa (Paris:
Imprimerie Nationale, 1955), pp.
31-81 and pl. I-LXXVI.
Ferron and Pinard
1960Ferron, Jean and Pinard,
Maurice, "Les Fouilles de Byrsa (Suite)", in Cahiers de Byrsa (Paris:
Imprimerie Nationale, 1960), pp.
77-170 and pl. I-XCV.
Freed 2001Freed, Joann, "Bibliograph of Publications by Alfred-Louis Delattre (1850-1932)",
Centre d'Etudes et de Documentation Archéologique de Carthage
(Carthage) 20 (2001), pp. 3--60.
Freed and Moore
1996Freed, Joann and Moore,
Jennifer, "New Observations on the Earliest Roman Amphoras from
Carthage: Delattre's First Amphora Wall", Centre d'Etudes et
de Documentation Archéologique de Carthage (Carthage) 20
(1996), pp. 19--28.
Frere 1975Frere, Sheppard S., "Principles of Publication in Rescue Archaeology: Report by a Working Party of
the Ancient Monuments Board for England", Committee for
Rescue Archaeology (1975).
Gros 1982Gros, Pierre, "Le forum
de la haute ville dans la Carthage romaine d'après les textes et
l'archéologie", Comptes rendus des séances de l'Académie des
Inscriptions et Belles-Lettres 126, 3 (1982), pp. 636--658.
Gros 1985Gros, Pierre, Byrsa
III: Rapport sur les campagnes de fouilles de 1977 à 1980: la
basilique orientale et ses abords vol. 41, (Rome: École Française de Rome,
1985).
Gros 1990Gros, Pierre, "Le
premier urbanisme de la Colonia Julia Carthago", in L'Afrique dans
l'Occident romain: Ier siècle av. J.-C. - IVe siècle
ap. J.-C.: Actes du colloque de Rome (3-5 décembre 1987) (Rome: École Française de Rome,
1990), pp. 547--573.
Gros 1992Gros, Pierre, "Colline
de Byrsa: Les Vestiges Romains", in Pour sauver Carthage.
Exploration et conservation de la cité punique,
romaine et byzantine (Paris: UNESCO/INAA, 1992), pp. 99--104.
Gros 1997Gros, Pierre, "Les
Bâtiments Administratifs de La Carthage Romaine. Problèmes
d'identification et de Localisation", Mitteilungen des
Deutschen Archäologischen Instituts Römische Abteilung 104
(1997), pp. 341--350.
Gros 2018Gros, Pierre, "In
memoriam : Jean Deneauve (1922-2017)", Antiquités africaines.
L'Afrique du Nord de la protohistoire à la
conquête arabe (2018), pp. 5--7.
Gros and Deneauve
1980Gros, Pierre and Deneauve,
Jean, "Hypothèses sur le centre monumental de la Carthage
romaine, d'après les recherches récentes sur la colline de Byrsa", Comptes rendus des séances de l'Académie des Inscriptions et
Belles-Lettres 124, 2 (1980), pp. 299--332.
Gros and Deneauve
1996Gros, Pierre and Deneauve,
Jean, "La Carthage romaine restituée", Archéologia (1996), pp. 54--61.
Gutron 2010Gutron, Clémentine, L'archéologie en Tunisie (XIXe-XXe siècles): jeux généalogiques sur
l'Antiquité (Paris and Tunis: Karthala and IRMC, 2010).
Herzog 1996Herzog, Ze'ev, "With
Time, We're Getting Worse", in Archaeology's Publication
Problem vol. 1, (Washington,
DC: Biblical Archaeology Society, 1996),
pp. 87--110.
Hodder 1989Hodder, Ian, "Writing
Archaeology: Site Reports in Context", Antiquity 63, 239 (1989),
pp. 268--274.
Hurst 1994Hurst, Henry R., Excavations at Carthage: The British Mission vol. II, 1, (Sheffield: Oxford University Press, 1994).
Isakhan and Meskell
2019Isakhan, Benjamin and
Meskell, Lynn, "UNESCO's Project to `Revive the Spirit of Mosul':
Iraqi and Syrian Opinion on Heritage Reconstruction after the Islamic State", International Journal of Heritage Studies 25, 11 (2019), pp.
1189--1204.
Jacobs 1996Jacobs, Paul F., "The
On-Line Digmaster Database", in Archaeology's Publication
Problem vol. 1, (Washington,
DC: Biblical Archaeology Society, 1996),
pp. 71--78.
Ladjimi-Sebaï
2005Ladjimi-Sebaï,
Leïla, La colline de Byrsa à l'époque romaine: étude
épigraphique et état de la question vol. 26,
(Paris: C.E.A.M., Institut d'Art et
d'Archéologie, 2005).
Lancel 1977Lancel, Serge, "Le
secteur A", Antiquités
africaines 11, 1
(1977), pp. 19--49.
Lancel 1995Lancel, Serge, Carthage: A History (Oxford:
Blackwell, 1995).
Lancel et al. 1979Lancel, Serge, Carrié, Jean-Michel, Deneauve,
Jean, Gros, Pierre, Sanviti, Nicole, Thuillier, Jean-Paul, Villedieu, Françoise, and Saumagne,
Charles, Byrsa I: Rapports préliminaires des fouilles
(1974-1976) vol. 41, (Rome:
École Française de Rome,
1979).
Lancel, Morel, and Thuillier
1982Lancel, Serge, Morel,
Jean-Paul, and Thuillier, Jean-Paul, Byrsa II: Rapports
préliminaires sur les fouilles 1977-1978: Niveaux et vestiges puniques (Rome: École française de Rome,
1982).
Lapeyre 1934Lapeyre, Gabriel Guillaume, "L'Enceinte Punique de Byrsa d'après Les Dernières Fouilles de La Colline
Saint-Louis de Carthage", Revue Africaine 75 (1934), pp. 336--353.
Lin 2003Lin, Shih-Han Samuel, Lading of the Late Bronze Age Ship at Uluburun (College
Station: Texas A&M
University, 2003).
Manière, Crépy, and
Redon 2020Manière, Louis, Crépy,
Maël, and Redon, Bérangère, "Geospatial Data from the ``Building
a Model to Reconstruct the Hellenistic and Roman Road Networks of the Eastern Desert of Egypt, a
Semi-Empirical Approach Based on Modern Travelers' Itineraries'' Paper", Journal of Open Archaeology Data 8, 1 (2020), pp. 7.
Margueron
1995Margueron,
Jean-Claude, "La Palais Royal d'Oufgarit: Premiers Résultats
d'une Analyse Systématique", in Le Pays d'Ougarit Autour
de 1200 Av. J.-C. Histoire et Archéologie: Actes Du Colloque International, Paris, 28
Juin-1e Juillet 1993 (Paris: Éditions Recherche sur les Civilisations, 1995), pp. 183--202.
Matoïan 2008Matoïan, Valérie, "Les
Objets Du Palais Royal d'Ougarit: Un État de La Question", in
Le Mobilier Du Palais Royal d'Ougarit: Maison de l'Orient et de La
Méditerranée (Paris: Éditions
Recherche sur les Civilisations, 2008), pp. 17--71.
Mazar 1996Mazar, Amihai, "Final
Reports: What They Should Include", in Archaeology's Publication
Problem vol. 1, (Washington,
DC: Biblical Archaeology Society, 1996),
pp. 23--36.
Meskell 2018Meskell, Lynn, A
Future in Ruins: UNESCO, World Heritage, and the Dream of
Peace (Oxford, New York: Oxford
University Press, 2018).
Meskell 2020Meskell, Lynn, "Sites
of Violence: Terrorism, Tourism, and Heritage in the Archaeological
Present", in Embedding Ethics 1st edition (London: Routledge, 2020), pp. 123--146.
Morel 2011aMorel, Jean-Paul, "Les
fouilles de Byrsa (secteur B) à Carthage : un bilan", Comptes rendus
des séances de l'Académie des Inscriptions et
Belles-Lettres 155, 1 (2011), pp. 325--363.
Morel 2011bMorel, Jean-Paul, "Mission archéologique de Carthage-Byrsa", Les
nouvelles de l'archéologie (2011), pp. 39--43.
Morgan 2013Morgan, Catherine, "Publishing Archaeological Research: Comparative Perspectives on Common
Concerns", Mélanges de la Casa de Velázquez 43, 43-2 (2013),
pp. 279--288.
Opitz 2018Opitz, Rachel, "Publishing Archaeological Excavations at the Digital Turn", Journal of Field Archaeology 43, sup1 (2018), pp. S68-S82.
Opitz, Mogetta, and
Terrenato 2016Opitz, Rachel,
Mogetta, Marcello, and Terrenato, Nicola, eds., A
Mid-Republican House from Gabii (Ann Arbor, MI:
University of Michigan Press, 2016).
Picard 1951Picard, Colette, "Vestiges d'un Édifice Punique à Carthage", Karthago III (1951), pp. 119--126.
Pollock 2010Pollock, Susan, "Decolonizing Archaeology: Political Economy and Archaeological Practice in the
Middle East", in Controlling the Past, Owning the Future:
The Political Uses of Archaeology in the Middle East (Tucson: University of Arizona
Press, 2010), pp. 196--216.
Pollock 2016Pollock, Susan, "Archaeology and Contemporary Warfare", Annual Review
of Anthropology 45, 1 (2016), pp. 215--231.
Pulak 1998Pulak, Cemal, "The
Uluburun Shipwreck: An Overview", International Journal of Nautical
Archaeology 27, 3 (1998), pp. 188--224.
Rakob 2000Rakob, Friedrich, "The
Making of Augustan Carthage", in Romanization and the City:
Creation, Transformations, and Failures:
Proceedings of a Conference Held at the American Academy in Rome to Celebrate the 50th
Anniversary of the Excavations at Cosa, 14-16 May, 1998 (Portsmouth: Journal of Roman
Archaeology, 2000).
Richards 2004Richards, Julian D., "Online Archives", Internet
Archaeology (2004).
Ronayne 2006Ronayne, Maggie, "Archaeology against Cultural Destruction: The Case of the Ilisu Dam in the
Kurdish Region of Turkey", Public Archaeology
5, 4 (2006),
pp. 223--236.
Ronayne 2016Ronayne, Maggie, "The
Culture of Caring and Its Destruction in the Middle East: Women's Work,
Water, War and Archaeology", in Archaeology and
Capitalism: From Ethics to Politics 1st edition
(New York: Routledge, 2016), pp. 247--265.
Saumagne
1924aSaumagne, Charles,
"Colonia Iulia Karthago", Bulletin
archéologique du Comité des travaux historiques et scientifiques (1924), pp. 131--140.
Saumagne 1924bSaumagne, Charles, "Notes de topographie carthaginoise: La colline de Saint-Louis",
Bulletin archéologique du Comité des travaux historiques et
scientifiques (1924), pp. 177--193.
Schimanski and
Alperin 2018Schimanski, Lesley A.
and Alperin, Juan Pablo, "The Evaluation of Scholarship in
Academic Promotion and Tenure Processes: Past, Present, and Future", F1000Research 7 (2018), pp. 1605.
Shanks 1996aShanks, Hershel, ed., Archaeology's Publication Problem vol. 1,
(Washington, DC: Biblical Archaeology
Society, 1996).
Shanks 1996bShanks, Hershel, "Getting Assistance in Writing Reports", in Archaeology's Publication Problem vol. 1, (Washington, DC: Biblical Archaeology Society, 1996),
pp. 49--54.
Shanks and Magness
1999Shanks, Hershel and Magness,
Jodi, eds., Archaeology's Publication Problem vol.
2, (Washington, DC: Biblical Archaeology Society, 1999).
Shaw 1738Shaw, Thomas, Travels, or Observations Relating to Seveval Parts of Barbary and the
Levant (Oxford, 1738).
Styrenius et al.
1986Styrenius, Carl-Gustaf,
Nilson, Kjell Aage, Olson, Åke, and Johnsson, Björn, "The Swedish
Carthage Excavations: Preliminary Geodetic and Cartographic Studies", Bulletin of the Museum of Mediterranean and Near Eastern
Antiquities 21 (1986), pp.
81--91.
Townsend et al.
2020Townsend, Russell, Sampeck,
Kathryn, Watrall, Ethan, and Griffin, Johi D., "Digital
Archaeology and the Living Cherokee Landscape", International Journal
of Historical Archaeology 24, 4 (2020), pp. 969--988.
Appendix A Correcting Distortion in
Figures from Persée
A.1 Summary of the Problem
One of the most important
repositories of scholarship on ancient
Carthage is Persée, an open-access digital library that contains an enormous selection of books, conference
proceedings, and journal articles spanning over 200 years of French archaeological research. Particularly
useful is Persée’s selection of books and articles on the Byrsa Hill, which include
Byrsa I and
III (curiously, not
Byrsa II), and several key studies in
Comptes Rendus des Séances
de l'Académie des Inscriptions et Belles-Lettres (
CRAIBL) and
Cahiers des Études
Anciennes (
CEA), including
Deneauve (
1983) and
Gros and Deneauve
(
1980). All of these publications have been manually scanned, de-skewed, and
optimized by Persée, and are available for download as OCR-enabled PDFs.
A significant number of figures in these PDFs are visibly
distorted. Three examples of distorted images from the Persée PDFs (
,
,
) are
given in Figure
A.1, with perfect squares shown in red for
comparison. In all three examples, it
is clear that the reference grids are not square.
These images are not distorted in
their original paper
publications. In Figure
A.2 are shown the same images as in
Figure 1, but scanned instead by me (
,
) and a librarian from Koerner Library (
).
As before, perfect squares are shown in red for comparison. In all three examples, the reference grids are
perfectly square. Notably, physically measuring the images in the printed books yields the same result—the
reference grids ought to be square in the Persée PDFs, but they are not.
This image distortion is a major problem, because the distortion
is not slight. As will be shown below in Figures 5-7, features in depicted in the Persée PDFs diverge wildly
from their personally-scanned counterparts. These distortions are present in multiple publications (
Byrsa I,
Byrsa III, and
Gros and Deneauve 1980), across multiple years (1979, 1985, 1980), and in multiple formats
(book and journal article). This suggests that the
distortions present in these PDFs may be found in many
other documents in the Persée system.
In the following sections, I diagnose the cause of the problem and
demonstrate a solution.
A.2 Diagnosing the Cause of the
Distortion
A close examination of the three
examples discussed above suggests
a common cause for the distortion: all of the examples are composed of non-square pixels. Figure
A.3 shows a close-up perspective on each of the three example pages from
Persée, with perfect squares shown in red for comparison. In all three examples, it is clear that the pixels
themselves are not square. Pixel aspect ratio (AR), calculated as the ratio of pixel width (w) to pixel
height (h), is calculated for each page in Figure
A.3. These AR values vary
significantly. In
and
, the pixels are taller than squares (AR
< 1), while in
the pixels are shorter than squares (AR > 1).
Although square pixels are generally the
norm, digital images may
be encoded with different pixel aspect ratios when created in certain contexts and for certain purposes.
Even so, the pixel aspect ratios calculated from Figure
A.3 are very
different from one another, and they do not match any of the standard non-square values used in common image
and video formats. Moreover, a quick survey of other pages in
Gros and Deneauve (
1980),
Byrsa I, and
Byrsa III shows that
every
page is composed of pixels with a different aspect ratio. These factors suggest that the different
aspect ratios may have been produced accidentally, perhaps during the post-processing of the original,
unoptimized scan files.
The next step was to export the three Persée PDF pages as JPEG
image files, so that key features in them could be traced and overlaid onto the pages I personally scanned.
By examining the sizes of the gaps between the two sets of features, it is possible to determine if the
mismatch is due only to a difference in pixel aspect ratio, or if there are additional sources of
distortion.
When the three PDF pages are exported as JPEG files, the
non-square pixel aspect
ratios are retained. The metadata of the resulting files are
presented in Figure
A.4.
Notably, the JPEG files for
and
are encoded
with pixel aspect ratios that are the mathematical inverse of what were calculated from Figure
A.3. This is caused by an unreported bug in my PDF viewing and editing
program, Adobe Acrobat Pro: when a rotated page is exported to an image file, Acrobat exports the rotated
image,
but encodes that image with the non-rotated metadata. Both
and
were
originally oriented 90 degrees counterclockwise to their orientation in the Persée PDFs—when creating their
PDFs, Persée rotated these pages 90 degrees clockwise so that their figure captions would be right-side-up.
This means that exporting these pages from the Persée PDFs yielded images that were rotated, but also
encoded with the non-rotated (i.e., non-inverted) pixel aspect ratios. This problem is solved by rotating
the PDFs of
and
by 90 degrees counterclockwise before
exporting them as JPEG files.
From this point forward, all exported images of these pages were made using this method.
In the resulting JPEGs of
,
, and
, key
features were traced, and the traces were overlaid on corresponding JPEGs generated from my
personally-scanned PDFs. The results are shown in Figures
A.5,
A.6 and
A.7.
In each Figure, the trace was overlaid in such a way that one
point from it overlapped perfectly with its corresponding point in the image below. I then measured the
distances between this shared point of optimal overlap and five features. I calculated the gaps between
these two sets of distances, and plotted them against the distances for my personal scan. In each case, the
resulting plot was completely linear (R² > 0.99), indicating that the mismatch was caused by a different
linear scaling factor. This limits the potential
causes of the mismatch to differences in pixel aspect ratio
and image resizing, and rules out non-linear causes such as excessive page curling. In each case, the slope
of the plot is essentially equal to the difference between the Persée aspect ratio and 1, which shows that
the gaps are caused entirely by a difference in aspect ratio.
A.3 Demonstrating a Solution
Because pixel aspect ratio is
solely to blame for the mismatch,
the solution to the problem is simple: edit the metadata of the Persée JPEGs and set the pixel aspect ratio
to 1. Image metadata is stored in EXIF format, and can be edited in a variety of ways, including via image
editing software (e.g., Adobe Photoshop), EXIF editing software (e.g., EXIF Pilot), and python scripting
(e.g., with the piexif package). Adjusting the image metadata in this way yields an almost perfect overlap,
as shown in Figure
A.8.
Appendix
B Reproduced Figures
This appendix presents additional reproduced figures that did not
fit in the main text of the thesis. These figures are included here for the sake of transparency and
reproducibility, since my results cannot be reproduced if my initial dataset is not clear. All figures in
this appendix are also included as higher-resolution image files in the supplementary files accompanying
this thesis online.
All figures are presented with
either a citation or Figure ID. The
Figure ID system is explained in Section
2.1.
Appendix C
Supplementary Tables
C.1 Feature Metadata
C.1.1 Axes of
Reconstruction
Table C.1:
Metadata for axes of reconstruction.
Axis ID
|
Description
|
|
western façade of the corner room in ,
extended to meet the NW corner of the western enclosure (library?) in
|
|
line
of the reconstructed façade of the first 4 apses in the southern alignment in
|
|
east
façade of the basilica in ,
extended to meet
|
|
north
façade of the basilica in ,
extended to meet
|
|
line
between the NW corner of and the W side of , extended as
shown in
|
|
line
from the W side of to
the extent shown in , along
an angle
parallel to
|
|
line
extending eastward from the NE corner of to meet at a 90
degree angle, as shown in
|
|
line
extending eastward from the SE corner of to meet at a 90
degree angle, as shown in
|
|
line
extending eastward from the NE corner of to meet at a 90
degree angle, as shown in
|
|
line
extending eastward from the NE corner of to meet at a 90
degree angle, as shown in
|
|
line
extending eastward from the SE corner of to meet at a 90
degree angle, as shown in
|
|
line
from SW corner of to
SE corner of
|
|
line
along E side of ,
extended to a length of 26 m (following dimensions
given in Deneauve 1990: 151)
|
|
central axis of (as shown
in )
extended for 20.6 m (the length of the reconstructed cistern in
)
|
|
line
extending 26 m parallel to , located 3.8
m away from E side of CI-001e,
perpendicular to
|
|
line
from the center of to the center of
|
|
line
between the center of
and the W side of the southern colonnade in
, parallel to
|
|
east
façade of in
, extended N and S parallel to
|
|
south
façade of basilica in , extended
to meet
|
|
west
façade of the basilica in
|
|
line of the N side of the south slope
retaining wall, stretching from the easternmost point shown in through
the westernmost point shown in ,
to a westward endpoint on the E side
of
|
C.1.2 Walls (MU)
Table C.2:
Metadata for walls.
Feature ID
|
Period
|
Subperiod
|
Construction
|
Source
|
|
Roman
|
Phase
1, Phase 2
|
opus
quadratum
|
(assumed S side under later
wall is
parallel to N side; assumed E side abutting )
|
|
Roman
|
Phase
1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase
1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase
1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase
1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase
1, Phase 2
|
opus
quadratum
|
(features hidden behind grid
labels traced
from )
|
|
Roman
|
Phase
2
|
opus
quadratum
|
|
|
Roman
|
Phase
2
|
opus
quadratum
|
|
|
Roman
|
Phase
2
|
opus
quadratum
|
|
|
Roman
|
Phase
2
|
opus
quadratum
|
|
|
Roman
|
Phase
2
|
opus
quadratum
|
|
|
Roman
|
Phase
2
|
opus
quadratum
|
|
|
Roman
|
Phase
2
|
opus
quadratum
|
|
|
Roman
|
Phase
1
|
opus
quadratum
|
|
|
Roman
|
Phase
1
|
opus
quadratum
|
|
|
Roman
|
Phase
1
|
opus
quadratum
|
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed S side parallel
to N side and
contiguous with
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assumed thickness 0.6 m)
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed same dimensions as and ;
assumed placement based on same apse dimensions as with and
, following
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed same dimensions as and ;
assumed placement based on same apse dimensions as with and
, following
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed width about 1.5 m; assumed E and W sides
perpendicular to
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed width about 1.3 m; assumed E and W sides
perpendicular to
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed width about 1.1 m; assumed E and W sides
perpendicular to
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed width about 1.0 m; assumed E and W sides
perpendicular to
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed width about 1.1 m; assumed E and W sides
perpendicular to
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60; assumed contiguous with )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed wall width of 1.1
m following
Beulé 1861: 60; asummed contiguous with ; assumed contiguous with
)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed wall width of 1.1
m following
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed wall width of 1.1
m following
Beulé 1861: 60; assumed E side colinear with E side of )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60; assumed E side colinear with E side of )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60; assumed to extend north and east until N side flush with N side of
)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60; assumed S side abutting )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed width of 1.1 m
following Beulé
1861: 60; assumed E side colinear with E side of )
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(feature exists but is hidden
by other
features)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(feature exists but is hidden
by other
features)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
(assumed construction
identical to
southwest apses)
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
(assumed W side separated
from adjacent
feature in map, which appears to be rudus in Gros and Deneauve 1980: 322;
assumed construction identical to )
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
(features hidden behind grid
labels traced
from )
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
opus
quadratum (base); brick-like stonework (impost)
|
(shown more clearly in
)
|
|
Roman
|
Phase 2
|
opus
quadratum (base); brick-like stonework (impost)
|
|
|
Roman
|
Phase 1
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
(assumed thickness 1 m;
assumed
construction identical to )
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
(assumed thickness 1 m;
assumed
construction identical to )
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed dimensions similar to W part of ,
following
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed S side continued the curve of
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed S side continued the curve of
|
|
Roman
|
Phase 1, Phase 2
|
rubble joined with lime, lined with opus
reticulatum
|
assumed curve of was
originally
semicircular
|
|
Roman
|
Phase 1, Phase 2
|
rubble linked with lime
|
assumed curve of was
originally
semicircular
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed S side continued the curve of
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed S side continued the curve of
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60; assumed contiguous with )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same dimensions as
described by
Beulé 1861: 60)
|
|
Roman
|
Phase 2
|
opus
quadratum (base); brick-like stonework (impost)
|
|
|
Roman
|
Phase 2
|
opus
quadratum (base); brick-like stonework (impost)
|
(assumed thickness 0.5 m from
intrados in
map, thinned where needed to make room for adjacent substructure wall)
|
|
Roman
|
Phase 2
|
opus
quadratum (base); brick-like stonework (impost)
|
|
|
Roman
|
Phase 2
|
opus
quadratum (base); brick-like stonework (impost)
|
(exists but is hidden by other
features)
|
|
Roman
|
Phase 1
|
opus
quadratum (base); brick-like stonework (impost)
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum (base); brick-like stonework (impost)
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1, Phase 2
|
opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assume SE corner continues
under later
wall)
|
|
Roman
|
Phase 1, Phase 2
|
opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1
|
opus
quadratum
|
Assume same size and orientation as , but
truncated as in
|
|
Roman
|
Phase 1
|
opus
quadratum
|
Assume same size and orientation as
|
|
Roman
|
Phase 1
|
opus
quadratum
|
Assume same size and orientation as
|
|
Roman
|
Phase 1
|
opus
quadratum
|
Assume same size and orientation as
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
reticulatum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assumed based on
Mu-FA0013r)
|
|
Roman
|
Phase 1, Phase 2
|
opus
reticulatum
|
(assumed continuous with
)
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assumed width 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assumed width 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assumed length 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assumed width 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
(assumed width 1.8 m;
assumed centered
opening of the neighboring apse)
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as ; assumed S side
flush with ; assumed placement based on
same apse dimensions as with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as ; assumed S side
flush with ; assumed placement based on
same apse dimensions as for
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed length such that apse opening was
proportional to that reconstructed in ; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed length such that apse opening was
proportional to that reconstructed in ; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed length such that apse opening was
proportional to that reconstructed in ; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed length such that apse opening was
proportional to that reconstructed in ; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
assumed length such that apse opening was
proportional to that reconstructed in ; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed same dimensions as described by Beulé 1861:
60; assumed opening width of 2.28 m, proportional to openings of southwest
apses; assumed contiguous with façade walls of adjacent corner room; assumed S
side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same width as
façade walls of
adjacent apses); assumed S side flush with ; assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed contiguous with façade wall of adjacent corner room; assumed E side
flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed contiguous with façade wall of adjacent corner room; assumed E side
flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same width as
façade walls of
adjacent apses); assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same width as
;
assumed N side flush with )
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed thickness identical to ; assumed
opening width of 2.28 m, proportional to openings of southwest apses; assumed
continuous with façade of adjacent corner room; assumed N side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed thickness identical to ; assumed
opening width of 2.28 m, proportional to openings of southwest apses; assumed N
side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed thickness identical to ; assumed
opening width of 2.28 m, proportional to openings of southwest apses; assumed N
side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed thickness assumed opening width of 2.28 m, proportional to openings of
southwest apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed thickness assumed opening width of 2.28 m, proportional to openings of
southwest apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed thickness assumed opening width of 2.28 m, proportional to openings of
southwest apses; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same width as
façade walls of
adjacent apses); assumed E side flush with ; assumed S side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed contiguous with façade wall of adjacent corner room; assumed E side
flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed contiguous with façade wall of adjacent corner room; assumed E side
flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed same width as
façade walls of
adjacent apses); assumed E side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest apses;
assumed contiguous with façade wall of adjacent corner room
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest
apses
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed wall width of 1.0 m following Beulé 1861: 60;
assumed opening width of 2.28 m, proportional to openings of southwest
apses
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 2.6 m,
proportional to
coverage for northeastern apses)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 3.6 m,
proportional to
coverage for northeastern apses)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 2.3 m,
proportional to
coverage for northeastern apses)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 2.6 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 4.2 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 4.2 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 4.2 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed southward extent
symmetrical to
northward extent shown in map)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed southward extent
symmetrical to
northward extent shown in map)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 4.2 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 4.2 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 4.2 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 2.6 m)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 2.3,
proportional to
coverage for northeastern apses)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 3.6 m,
proportional to
coverage for northeastern apses)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed length 2.3 m,
proportional to
coverage for northeastern apses)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
opus
quadratum
|
(assumed same dimensions as
Phase 2
counterpart)
|
|
Roman
|
Phase 1
|
|
(assumed E side abutting
;
assumed width identical to ; assumed W side abutting ;
assumed N side flush with )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed E side abutting
;
assumed W side flush with ; assumed N
and S sides perpendicular to ;
assumed width identical to )
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
(assumed feature continues
under later
wall)
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
(assumed that wall
continued under
)
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
(assumed feature continues under
as shown in )
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
(assumed feature continues unfer
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
,
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
(southward spur on the east
side),
(everything else)
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed dimensions and shape described in Delattre
(1894: 89-90)
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
assumed to extend to
based on Lapeyre 1934:
pl. 2
|
|
Roman
|
Phase 2
|
|
assumed to extend to
based on
(reproduction of Lapeyre 1934: pl. II)
|
|
Roman
|
Phase 2
|
|
assumed to extend east until
|
|
Roman
|
Phase 1, Phase 2
|
|
(for subtype, see and Deneauve
1983: 95)
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed separate from other
adjacent walls
based on )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed separate from other
adjacent walls
based on )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed separate from other
adjacent walls
based on )
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
; (assumed W side flush with
and perpendicular to , which is not
quite as depicted in but
does match ; assumed W side
width same as E side)
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed originally
continuous with
; assumed N side
colinear with N side of
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed wall continues under
later
wall)
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed originally
continuous with
as shown in
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed smooth façade
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed smooth façade
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed S side flush with ; assumed N
side
flush with ; assumed E side abutting
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(wall in this figure is
unrealistically
wide)
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
(this feature is also shown in
,
where it is poorly aligned with in , with which this feature
is assumed to be contiguous)
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
, (assumed S side flush with
)
|
|
Roman
|
Phase 2
|
|
and
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
(assumed N side flush with
; assumed
S side flush with ; assumed E side
abutting as shown in
and )
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed to be part of a wall
based on
dotted lines on map)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed to be more trustworthy
than
, which seems to be more poorly
aligned with other maps of this
area)
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
, (assumed W side location
following ; assumed N side
flush with ; assumed S side flush
with
|
|
Roman
|
Phase 1, Phase 2
|
|
, (assumed W side abutting
, following ; assumed N side flush with AX-005; assumed S
side flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed N side flush with
; assumed
S side flush with ; assumed E side
abutting and
Mu-AR0062h)
|
|
Roman
|
Phase 1, Phase 2
|
rubble linked with earth
|
(W side), (E side)
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble linked with earth
|
|
|
Roman
|
Phase 1, Phase 2
|
rubble linked with earth
|
(assumed symmetrical about
)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
(assumed W side abutting
)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
(assumed E side flush with
;
assumed N side flush with ; assumed N
side width of 4.0 m as shown in
Deneauve 1983: 105 fig. 8)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 1, Phase 2
|
|
, , (assumed N side flush
with , assumed S side flush with
; assumed E and W sides
even
with limits of )
|
|
Roman
|
Phase 1, Phase 2
|
|
, (assumed N side flush with
, assumed S side abutting , , , and
; assumed W side
abutting )
|
|
Roman
|
Phase 1, Phase 2
|
|
, , (assumed N side flush
with , assumed constant width of 1.65 m;
assumed E side abutting
)
|
|
Roman
|
Phase 1, Phase 2
|
rubble linked with mortar
|
assumed to exist based on analogy with adjacent
; assumed N side
abutting ; assumed E
side abutting
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
large blocks (El Haouaria) linked with dovetail
seals
|
(for construction see Deneauve
1990:
157)
|
|
Roman
|
Phase 1, Phase 2
|
large blocks (El Haouaria) linked with dovetail
seals
|
(for construction see Deneauve
1990:
157)
|
|
Roman
|
Phase 1, Phase 2
|
large blocks (El Haouaria) linked with dovetail
seals
|
(for construction see Deneauve
1990:
157)
|
|
Roman
|
Phase 1, Phase 2
|
large blocks (El Haouaria) linked with dovetail
seals
|
(assumed W side flush with
,
following ; assumed
symmetrical about , following ;
assumed W side width of 3.28 m; for construction see Deneauve 1990: 157)
|
|
Roman
|
Phase 1, Phase 2
|
large blocks (El Haouaria) linked with dovetail
seals
|
(assumed that the foundation
trench found
here was once contained wall continuous with and )
|
|
Roman
|
Phase 1, Phase 2
|
large blocks (El Haouaria) linked with dovetail
seals
|
|
|
Roman
|
Phase 1
|
rubble linked with earth
|
(assumed analagous to through
, but with identical
construction to )
|
|
Roman
|
Phase 1
|
rubble linked with earth
|
assumed analagous to ,
symmetrical about
, as shown in ; assumed W side abutting
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed analagous to
through ,
symmetrical about , as shown in
; assumed W side abutting
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed analagous to ;
assumed constant
width of 1.66 m based on W side of
|
|
Roman
|
Phase 1, Phase 2
|
rubble linked with mortar
|
assumed analagous to ;
assumed constant
width of 1.98 m similar to W side of
|
|
Roman
|
Phase 1, Phase 2
|
|
and (for dimensions see
Deneauve 1983: 105 fig. 8; assumptions are too numerous to include here - see
section in my thesis on tracing the walls mirroring D, F, and G)
|
|
Roman
|
Phase 1, Phase 2
|
|
and (for dimensions see
Deneauve 1983: 105 fig. 8; assumptions are too numerous to include here - see
section in my thesis on tracing the walls mirroring D, F, and G)
|
|
Roman
|
Phase 1, Phase 2
|
|
and (for dimensions see
Deneauve 1983: 105 fig. 8; assumed E side abutting and Mu-AR0076h;
other assumptions are too numerous to include here - see section in my thesis on
tracing the walls mirroring D, F, and G)
|
|
Roman
|
Phase 2
|
|
and (for dimensions see
Deneauve 1983: 105 fig. 8; assumptions are too numerous to include here - see
section in my thesis on tracing the walls mirroring D, F, and G)
|
|
Roman
|
Phase 2
|
|
and (for dimensions see
Deneauve 1983: 105 fig. 8; assumptions are too numerous to include here - see
section in my thesis on tracing the walls mirroring D, F, and G)
|
|
Roman
|
Phase 2
|
|
and (for dimensions see
Deneauve 1983: 105 fig. 8; assumed E side abutting , as with
; other assumptions are
too numerous to include here - see section in
my thesis on tracing the walls mirroring D, F, and G)
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
and (assumed S side flush
with ; assumed W and E side widths of
1.1 m)
|
|
Roman
|
Phase 1
|
|
assumed E side abutting
|
|
Roman
|
Phase 1, Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
(for construction, see Byrsa
III:
55)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(for construction, see Byrsa
III:
50-51)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
(assumed N side flush with
)
|
|
Roman
|
Phase 2
|
opus
quadratum
|
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed constant width of 1.75 m, following Deneauve
1983: 105 fig. 8; assumed N and S sides perpendicular to ; assumed W side
flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed 58.94 m away from and constant
width of 1.75 m (Deneauve 1983: 98, 105 fig. 8); assumed N and S sides
perpendicular to ; assumed W side at
limits of , (see Byrsa III:
140)
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed constant width of 2.3 m, following Deneauve
1983: 105 fig. 8; assumed N and S sides perpendicular to ; assumed W side
flush with
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed 10.1 m away from and constant
width of 2.3 m (see Deneauve 1983: 105 fig. 8); assumed N and S sides
perpendicular to ; assumed W side at
limits of (see Byrsa III:
140)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
(for construction, see Deneauve
1983:
95)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
(for construction, see Deneauve
1983:
95)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
and (assumed W side flush
with and perpendicular to ; assumed W
side width same as E side)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
and (assumed W side flush
with ; assumed N and S side widths of
4.40 m following Deneauve 1983:
95)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
and (assumed E side width of
2.1 m as shown in Deneauve 1983: 105 fig. 8; assumed W side width same as E
side; assumed N side flush with )
|
|
Roman
|
Phase 1
|
|
(assumed W side continuous
with
; assumed identical
width and orientation to ; assumed E
side abutting )
|
|
Roman
|
Phase 1
|
|
(assumed W side continuous
with
; assumed identical
width and orientation to ; assumed E
side abutting )
|
|
Roman
|
Phase 1
|
|
(assumed E side flush with
line between
NE corner of and SE
corner of ; assumed W
side flush with
line between NW corner of and SW corner of
|
C.1.3 Piles (PI)
Table C.3:
Metadata for foundation piles.
Feature ID
|
Period
|
Subperiod
|
Construction
|
Source
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed location halfway between and
; assumed original length
and width about 1.8 m
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
|
|
Roman
|
Phase 1
|
|
assumed location along the sevenths between
and
|
|
Roman
|
Phase 1
|
|
assumed location along the sevenths between
and
|
|
Roman
|
Phase 1
|
|
assumed location along the sevenths between
and
|
|
Roman
|
Phase 1
|
|
assumed location along the sevenths between
and
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed location along the sevenths between
and
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed location along the sevenths between
and
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed location along the sevenths between
and
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed original length and width of were
about 1.8 m
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed original length and width of was
about 1.8 m
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed original length and width of were
about 1.8 m
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed original length and width of were
about 1.8 m
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed original length and width of were
about 1.8 m
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
assumed length and width of 1.8 m; assumed spacing of
4.8 m; assumed alignment from and
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
assumed length and width of 1.8 m; assumed spacing of
4.8 m; assumed alignment from and
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
assumed length and width of 1.8 m; assumed spacing of
4.8 m; assumed alignment from and
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
assumed length and width of 1.8 m; assumed spacing of
4.8 m; assumed alignment from and
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
assumed length and width of 1.8 m; assumed spacing of
4.8 m; assumed alignment from and
|
|
Roman
|
Phase 1, Phase 2
|
stone rubble and mortar
|
assumed length and width of 1.8 m; assumed spacing of
4.8 m; assumed alignment from and
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
(pile continues under
neighboring
walls)
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed original width about 1.8 m as shown in
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed original width and length about 1.8 m as
shown in
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed length and width of 1.8 m; assumed spacing of
4.4 m; assumed alignment from and
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed length and width of 1.8 m; assumed spacing of
4.4 m; assumed alignment from and
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed length and width of 1.8 m; assumed spacing of
4.4 m; assumed alignment from and
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed length and width of 1.8 m; assumed spacing of
4.4 m; assumed alignment from and
|
|
Roman
|
Phase 2
|
opus
caementicium
|
assumed length and width of 1.8 m; assumed spacing of
4.4 m; assumed alignment from and
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed location on W end
of ;
assumed length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed location on the
quarters between
and ; assumed length and width about
1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed location on the
quarters between
and ; assumed length and width about
1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed location on the
quarters between
and ; assumed length and width about
1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
assumed original width and height about 1.65 m
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed to be located two
thirds of the
way between and
; assumed length and
width about 1.8
m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed to be located one
third of the
way between and
; assumed length and
width about 1.8
m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
assumed original width about 1.7 m
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed to be located
halfway between
and ; assumed length and width about
1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed original extent based
on detritus
shown on map and discussion in Byrsa I: 129-130)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed to be located two
thirds of the
way between and
; assumed length and
width about 1.8
m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed to be located one
third of the
way between and
; assumed length and
width about 1.8
m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(assumed location halfway
between
and ; assumed width and
length of approximately 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
|
|
Roman
|
Phase 1, Phase 2
|
stones bound with clay
|
(unclear if this part of the
pile is
extant, since it is not traced on any map except ; assumed to be
reconstructed)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed location from
figure; assumed
length and width about 1.8 m)
|
C.1.4 Cisterns (CI)
Table C.4:
Metadata for cisterns.
Feature ID
|
Period
|
Subperiod
|
Construction
|
Source
|
|
Roman
|
Phase 1, Phase 2
|
|
|
|
Roman
|
Phase 1, Phase 2
|
|
assumed central axis along ; assumed
length
20.6 m following
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
(assumed feature continued
under later
walls)
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
C.1.5 Staircases (ES)
Table C.5:
Metadata for staircases.
Feature ID
|
Period
|
Subperiod
|
Construction
|
Source
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed length 30.2 m)
|
|
Roman
|
Phase 1, Phase 2
|
|
(assumed length 30.2 m)
|
C.1.6 Tombs (TO)
Table C.6:
Metadata for tombs.
Feature ID
|
Period
|
Subperiod
|
Construction
|
Source
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
|
Punic
|
|
|
|
C.1.7 Rudus (RU)
Table C.7:
Metadata for rudi.
Feature ID
|
Period
|
Subperiod
|
Construction
|
Source
|
|
Roman
|
Phase 1, Phase 2
|
|
(type is implied in
description)
|
|
Roman
|
Phase 1, Phase 2
|
|
(type is implied in
description)
|
C.2 Feature Locations
C.2.1 Walls (MU)
Table C.8:
Locations of walls.
Feature ID
|
Location
|
|
,,
|
|
,
|
|
|
|
|
|
|
|
,; ,
|
|
,; ,
|
|
|
|
,,,
|
|
,,
|
|
,,
|
|
,;
|
|
,; ,,
|
|
; ,
|
|
,
|
|
,
|
|
;
|
|
,
|
|
,,
|
|
,
|
|
|
|
; ; ;
|
|
,; ,
|
|
,
|
|
,
|
|
,,
|
|
,;
|
|
,
|
|
,,,
|
|
,,
|
|
|
|
,; ,
|
|
; ; ;
|
|
,
|
|
,
|
|
,,
|
|
,,
|
|
,;
|
|
,
|
|
,
|
|
,; ,
|
|
,;
|
|
,;
|
|
,
|
|
,,,
|
|
,,,
|
|
,,
|
|
,
|
|
; ,
|
|
,; ,
|
|
,; ,
|
|
,
|
|
,,; ,
|
|
; ; ;
|
|
; ,
|
|
,
|
|
,,
|
|
,,
|
|
;
|
|
;
|
|
,; ,
|
|
; ,
|
|
,
|
|
,,
|
|
; ,
|
|
,;
|
|
,,
|
|
,,
|
|
,,
|
|
,,
|
|
,;
|
|
,
|
|
; ,
|
|
,;
|
|
,,
|
|
,,
|
|
,,; ,
|
|
,;
|
|
,,
|
|
,,,
|
|
,;
|
|
,; ,
|
|
,,
|
|
|
|
,
|
|
,,
|
|
,,;
|
|
; ;
|
|
,
|
|
,; ,;
|
|
,;
|
|
; ,,
|
|
,,; ,
|
|
,;
|
|
,,
|
|
,,,
|
|
,;
|
|
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C.2.2 Piles (PI)
Table C.9:
Locations of foundation piles.
Feature ID
|
Location
|
|
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|
|
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|
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C.2.3 Cisterns (CI)
Table C.10:
Locations of cisterns.
Feature ID
|
Location
|
|
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|
|
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|
|
|
|
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|
|
|
|
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|
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C.2.4 Staircases (ES)
Table C.11:
Locations of staircases.
Feature ID
|
Location
|
|
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|
|
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C.2.5 Tombs (TO)
Table C.12:
Locations of tombs.
C.2.6 Rudus (RU)
Table C.13:
Locations of rudi.
Feature ID
|
Location
|
|
,
|
|
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|
Appendix
D Corrective Notes for
Previously Published Profiles and Maps
While determining the extents of the profiles, some
inconsistencies and ambiguities became evident. These are identified below, along with the solutions I used
to resolve them. In this appendix, I always use the term “trench” to refer to a unit of
excavation, unless otherwise specified. This is equivalent to the term “sondage” in the original
French.
D.1
Byrsa I
D.1.1 The extents of
profiles and are missing
The extents of
and
(both 4.00 m wide) are not
labeled on any map, though their figure captions give their orientations (west and south) and assign them to
. A trench is shown in this location in maps
,
, and
, but it does not have a south
wall with the correct dimensions and it does not have a west wall at all. Based on photo
, the
extents are located a fraction of a meter (I assumed 50 cm) inward from the western and southern boundaries
of
.
D.1.2 The extents of
profile are missing
The extents of (4.00 m wide) are not labeled on any map,
though the figure caption gives its orientation (west) and assigns it to . A trench is shown in this
location in maps , , and , but it does not have a west wall.
Based on photo , the
extents are located a fraction of a meter (I assumed 50 cm) inward from the western boundary of .
D.1.3 The extents of
profile in the given maps are incorrect
In profile , the rightmost limit, denoted C, is
2.80 m away from B, which marks a bend in the profile wall. This does not match the extents of the
profile as they are plotted in maps and
, where C is shown almost 6 m away
from
B (and immediately adjacent to “coupe 20”). In contrast, in the distance between
B and the leftmost limit, A, is 6.20 m, which is identical to the distance shown in
and .
The contexts and features in
appear to be completely
continuous, so
C in
must really be
3.80 m away from
B. I conclude that the profile
extents plotted in
and
are incorrect, and I resolve this problem by
following the extent
in
only to 3.80 m north of
B.
D.1.4 The extents of
profile are not clearly identified
There is no label for profile that can be used to link
it to extents plotted in maps and
, and no grid cell labels appear in the
corresponding
text, either. Two observations are sufficient to link to the m-n profile in : their
widths are equivalent (just under 8.00 m), and the placement of features in the former is identical to the
latter.
D.1.5 The scale given for
profile is incorrect
The figure caption for profile gives a scale of 1:100.
No scale bar is given, but the scale can still be checked against the dimension labels at the bottom of the
profile. As it is printed, 520 cm (horizontal) in the profile measures 4.55 cm on the page: the correct
scale is about 1:114.3. This distortion appears to be identical in the vertical direction. It seems likely
that this distortion arose during the printing process: perhaps the publisher shrank the profile so that it
would fit better within the required margins.
D.1.6 The scale given for
map is incorrect
The figure caption for map
gives the scale as 1:50, but
as it is printed, 5.00 m on the map (the side length of one grid cell) measures 5.00 cm on the page.
Therefore, the scale is actually 1:100.
D.2 Byrsa II
D.2.1 The extents of
profile are not clearly identified
The extents of profile are not plotted on any map, but
its width (4.38 m from the edge of pile C16) is consistent with a line between the southeast corner
of pile C16 and the southeast edge of the excavations shown on map (staying within the
bounds of ). This assignment is also consistent
with photographs and .
D.2.2 The extents of
profile are not clearly identified
The extents of profile are not labeled on any map, but
its width of 7.40 m almost perfectly matches the length of the southwest limit of the excavations in
. Photographs of the profile wall
( and ) are consistent with this assignment.
D.2.3 The extents of
profile are not clearly identified
The extents of profile are not plotted on any map, but
its width (2.61 m) and features are consistent with a stretch of the northeast limits of Punic block
C excavations shown in . Photographs
, , and are consistent with this
assignment.
D.2.4 The extents of
profile are missing
The extents of profile
are not plotted on any map. Its
width is 3.97 m, the distance from its south limit to the south side of the wall is 1.62 m, the distance
from the north side
of the wall to the profile's north limit is 1.84
m. There are no gaps or bends in the
profile. Based on these factors and photographs
,
, and
, it appears that the profile is
located on the east side of courtyard
E in Punic block
E.
D.2.5 The extents of
profile are not clearly identified
The extents of are not labeled on any map, but its
figure caption and width of 4.28 m are consistent with the easternmost limit of the easternmost trench in
—note that this means the profile stretches
about 30 cm into , even though its label only
specifies .
D.2.6 The extents of
profile are not clearly identified
As with , the extents of profile are not labeled
on any map. The profile's width of 9.95 m is consistent with the westernmost limit of the easternmost trench
in map , provided that the profile stops 40
cm south of the northwest limit. (This is consistent
with 's label (“ - ”), since that extra 40 cm extends into .)
D.2.7 The extents of
profiles , , and in the given map are incorrect
The extents of profiles
,
, and
are plotted on map
, but only in schematic fashion: their
widths do not match the widths of the profiles. I transferred
these extents in
over to
and adjusted them so that they match their
respective profiles'
widths and features.
D.2.8 The grid cell label
for profile is incorrect
The grid cell label of profile is inconsistent with the
extents plotted on map . On the map, the
extents stretch into , even though the profile is
only labeled .
D.2.9 The extents of
profile in the given map are incorrect
The extents of profile are plotted on map , but
in exceedingly schematic fashion. I adjusted the extents to better reflect the width and features
illustrated in the profile.
D.2.10 The grid cell label
for profile is incorrect
The grid cell label for profile is inconsistent with the
extents plotted on map . On the map, the
extents stretch into , , and and , while
the profile's label only specifies , , and
. Note that has some discontinuities: it
displays part of wall C, an arch between piles C6 and C7 located in .
which is disconnected from the other features.
D.2.11 The extents of
profile in the given map are incorrect
The width of profile
(1.68 m) does not match the width
of the extents plotted in map
1.93 m). This
is strange, considering that the width of neighboring
profile
(4.19 m) almost exactly matches the width of the extents plotted in
(4.20 m).
It might seem that the scale bar for profile is
incorrect, because the width of the grave in is 1.32 m, which is very different from the width of
the grave in map (0.72 m). This is not the
case, because in the profile the trench measures 4.25 m
deep, and this measurement is confirmed in the discussion on p. 266. The grave at the bottom of is
drawn such that both of its ends are depicted in dotted lines.
The contradiction over extents can be resolved thus: in map
, the profile should begin at the southeast
edge of the trench extents (dotted line), and continue
on a line toward x' until it reaches the closest point to the southwest corner of grave A325.
That yields a width of1.72 m, which is almost identical to the width of profile (1.68 m, as noted
above).
D.2.12 The extents of
profile are missing
The extents of profile are not plotted on a map, but the
profile's width (1.79 m) and features are consistent with the east wall of trench 2 in , if it is
extended about 60 cm to the south.
D.2.13 The extents of
profiles cannot be georeferenced from
the given map
The extents of
are plotted on
, but this map
is not reliably georeferenceable. They must be transferred over to the corresponding location on map
,
which is georeferenceable.
D.2.14 The grid cell
labels for profiles and are incorrect
The grid cell labels for profiles and say that
they are located in and , but the profiles are
actually located only in .
D.3 Byrsa III
D.3.1 The extents of
profile are not clearly identified
The extents of profile (width 7.39 m) are not labeled
on any map, but they correspond almost exactly to the east wall of a trench at the mouth of the first apse
north of the central apse on . The grid
cell labels for are consistent with
this
assignment.
D.3.2 The extents of
profile are not clearly identified
The extents of profile
(width 3.43 m) are not labeled
on any map, but they correspond almost exactly to the south wall of a trench at the mouth of the first apse
north of the central apse on
. The grid
cell labels for
are consistent with
this
assignment.
D.3.3 The extents of
profile are not clearly identified
The extents of profile are not labeled on any map.
According to the profile's figure caption, the profile follows the wall of the modern staircase in the
second northern apse. By counting the stairs visible in the profile and comparing them to the stairs visible
on map , I can constrain the extents to
about 10 stairs (2.79 m) at the mouth of the apse. This is
consistent with the profile's width of 2.92 m. Note that this means that the profile's extents stretch 40 cm
into , even though this grid cell is not included
in the profile's grid label.
D.3.4 The extents of
profile are missing
The extents of profile are not plotted on any map. The
profile stretches 7.87 m from the outer edge of the basilica's east facade into cardo IV east, and
21.26 m from the building's western facade into the paved area behind it. I assume that the profile follows
the axis of the decumanus maximus. The profile's extents can be reconstructed on the basis of these
observations.