19th International CODATA Conference
Category: Open Communication
Information networking and integration: collaboration between data centres and academic journals
F.
Genova (CDS) (genova@astro.u-strasbg.fr ),
C. Bertout
(Astronomy & Astrophysics), F. Ochsenbein
(CDS), and S. Lesteven (CDS)
Observatoire astronomique, France
Astronomy is at the forefront for data conservation and distribution, and also
for information networking, thanks to early definition of de facto disciplinary
standards, on-line availability of observatory archives, and collaboration between
archive providers, data centres and peer-reviewed journals. The current astronomy
information network already allows scientists to surf from observations to results
published in journals, and includes value-added information services.
Collaboration between data centres (CDS and NED) led to an early definition of a disciplinary standard to describe bibliographic information, long before the Web age. This standard is widely used and maintained by the Astrophysics Data System (the reference bibliographic service for astronomy) and the data centres. Astronomy services have now to implement a smooth transition from their disciplinary standard to the general standard DOI, defined since then by publishers.
The implementation of journals
on the Web has also opened new possibilities for the scientific usage of published
results, and also new types of content validation, complementary to the referee's
one, and to the layout performed by publishers. For instance, the European journal
"Astronomy & Astrophysics" decided as early as 1993 to publish
'long' tables in electronic form at CDS, included in a catalogue service together
with reference astronomy catalogues. The standard description of tables is now
shared by other journals, in particular by the journals of the American Astronomical
Society (
In addition, authors publishing in "Astronomy & Astrophysics"
are able since several years to tag the names of astronomical objects in their
papers. A link controlled and maintained by CDS is then built to the data about
the object contained in the SIMBAD database. This can be a complex procedure,
due to the extreme diversity of nomenclature in astronomy, and tools are offered
to authors to check the validity of object names in their papers. The
One key question for the Virtual Observatory, is to find a proper way of describing the semantic content of information. One important knowledge base in that respect is built from the journal keywords. Other knowledge bases (thesaurus, Uniform Content Descriptors, ...) also exist and a preliminary action is under way to compare some of them with the possible goal to build one or several astronomy ontologies (Project Massive Data in Astronomy).