Ray
Norris,
The
management of astronomical data has become an increasingly significant issue in
recent years, because of large surveys now routinely producing Terabytes of
data, and because of the growing importance of www-based data centres, remote
observing, data archiving, etc. There have been two dominant issues since the
last GA: the Virtual Observatory, and the protection of freedom of access to
large databases. The Virtual Observatory work will be describe in detail by the
VO working group, but some implications have been handled by the WGAD, which
will be described here. A major issue for the IAU is the proposed database
protection legislation which is opposed by CODATA on behalf of the ICSU.
CODATA
is the committee on data in science and technology of the ICSU (International
Council for Science), and it serves the role of coordinating data-related
activities between the various scientific unions such as IAU and URSI. Given
the increasing significance of data in astronomy and the threats to our freedom
to use it, IAU involvement in CODATA is very important.
Ray
Norris represented the IAU at the October 2000 meeting in
There
is a worldwide shift towards increased protection for intellectual property. In
particular, the World Intellectual Property Organisation (WIPO) has proposed
legislation with the very reasonable aim of protecting commercial databases,
but with unwanted side-effects which will cause problems for open access to
scientific data (see http://www.codata.org/data_access/summary.html
for a summary of issues). Various groups, particularly in the
The growth
of databases from large surveys, and the advent of the virtual observatory, has
raised a number of issues around astronomical data. One of these is the need to
ensure future freedom of access to astronomical archive data from major
observatories, and a resolution to this effect will be tabled at the next
Until about 20 years ago
astronomy was split into a number of sub-disciplines corresponding to the
different wavelengths at which observations were made (optical astronomy, radio
astronomy, etc). Each of these tended to use its own data formats, as a result
of which it was awkward to combine data from different wavelengths. In 1981 the
FITS (Flexible Interchange Transport System) format was proposed (http://fits.gsfc.nasa.gov/documents.html),
and adopted enthusiastically by all sub-disciplines of astronomy. This
permitted easy interchange of data between the sub-disciplines, and was largely
responsible for breaking down cultural barriers between these sub-disciplines.
As a result, many astrophysicists today take their data at whichever wavelength
is needed to solve the astrophysical problem being addressed. This is probably
partly responsible for the current healthy state of astronomy and astrophysics
internationally, with new discoveries about the origin and evolution of the
Universe being made at a breathtaking rate.
While FITS has been
enormously and demonstrably successful, astronomical data are now seen by some
as outgrowing the 1980s technology on which FITS was based. The
An even more
sophisticated approach has been taken by organisations in US and