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Laura Peperoni1 and Marina Zuccoli
Astronomy Department, University of Bologna, Bologna, Italy,
e-mail:
archivio@astbo3.bo.astro.it
1Librarian, Economics Department, University of Bologna, Bologna, Italy
The archives of the Department of Astronomy of the University of Bologna date back to the XVII century, collecting scientific and administrative papers, letters and drawings.
The astronomical institute of Bologna - first public observatory in Italy - was founded in 1711. The archives collect its preliminary documents, the first observations made in the astronomical tower, then following its history until 1957.
The papers can be divided into three main archival categories: meteorological observations, astronomical observations and 65 miscellaneous boxes.
The archives had been organized by Prof. Guido Horn d'Arturo (1879-1967), director of the Observatory from 1921 to 1954. He followed a twofold method, both chronological and by subject. Therefore the boxes bear a title and are grouped according to their subject, such as ``calendar'', ``ephemerides'' or ``letters''. Within the subject, the papers are placed in chronological order.
We decided to keep this organization, thinking that informatics could cope
with some oddities in the classification. In order to select a program, at
first
we considered some Italian databases for historical archives and we eventually
focussed on the program used at Brera Observatory, in
Milan
(http://albinoni.brera.unimi.it/CAELUM/BIBLIO/biblioteca.html).
Our choice was a Web interface, putting the archives on the Web server of the Astronomical Observatory of Bologna . The Web interface appeared suitable not only for aesthetical reasons, but also for its hypertextual structure and added values, such as e-mail, network-based information retrieval, and document saving. The home page opens with general information about the archives and an interactive form for microfilm requests. A brief history of the Observatory is linked to a list of its directors. An English version of the historical introduction and of the main information services is provided.
The main part of the site is the archives' inventory. The database, written in HTML, is made of files, all with uniform structure. Each file contains a description of the documents (or set of documents) collected in a box, or the list of notebooks of observations.
Our choice of the HTML language is based upon two reasons. The first is that, HTML being a standard format for description of document structure, Web browsers can view the files directly. Secondly, the wide-spread diffusion of the Internet and of the Web interface ensures future maintenance and updating of the involved protocols and tools.
The database can be accessed in sequence and searched by strings.
The sequential approach is available through the hypertextual guide and its frame structure. The Web page is thus divided in two sections: a static section on the left side, bearing the list of the archival series, and a larger one on the right, showing the item selected from the list.
Since taking care of the historical archives is not the only duty, and maybe not the first one for the astronomical library, the work goes on slowly. The Web interface allows to present the archives even if work is still in progress. In fact, a first look at the archives is possible through the summary in the frame. As soon as an item in the list (e.g., a new box) is examined and decribed, a new file is linked to the summary. In the end, all items in the summary will have an analytical description on the right of the screen. Abstracts of each letter will be a further step in document description. Anyway, letters are available at present with their date, place and names of sender and addressee; only a few of them are already abstracted.
Search by string has been developed trying to meet the users' needs, as they had been expressed during the last years. The archives are generally visited by university researchers (astronomers, historians of science and of meteorology) and by students attending the course of history of astronomy. Our historical archives deal mainly with astronomy, but some mathematics, physics, meteorology and other disciplines are touched by its documents. The life of the observatory itself is of paramount importance for historians of science. In fact it started its activity under the Pope's government, was closed by Napoleon and, in the XXth century, it bore the consequences of having a Hebrew director during Fascism. This makes the archives interesting for a wide range of users, whose information needs are not entirely predictable. Therefore, search by string should be available on a very analytical database, even if archival theory suggests to stop description at series level.
Information retrieval is possible through WWWWAIS.C (2.5), an ANSI.C program downloadable from the Net . It works as a gateway between other programs creating indexed file catalogs, such as freeWAIS or SWISH, and a forms-capable Web browser. Search by string should follow the instructions supplied, using boolean operators AND and OR, and the asterisk as a wildcard.
The page ends with a ``Work in progress'' section, comprehending three projects: the directors' gallery, the published observations and the authority file.
Our present task is to complete the description of the boxes still missing to put them on the Web, supplying the astronomical community with an important tool for historical research.
The authors wish to thank Marco Lolli for his help.
Further Reading
Hensen, S. L. 1983, Archives, personal papers and manuscripts, Washington: Manuscript Division, Library of Congress
Next: The Revision of UDC 52 and of the Astronomy Thesaurus
Up: Posters presented in Absentia
Previous: Publication Costs of Astronomical Research
Table of Contents -- Index -- PS reprint -- PDF reprint