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A&A 424, 1097-1100 (2004)
DOI: 10.1051/0004-6361:20034029
Introducing BAX: A database for X-ray clusters and groups of galaxies
R. Sadat1, A. Blanchard1, J.-P. Kneib1, 2, G. Mathez1, B. Madore3 and J. M. Mazzarella31 Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées, 14 avenue E. Belin, 31400 Toulouse, France
e-mail: rsadat@ast.obs-mip.fr
2 Astronomy Department, California Institute of Technology, Pasadena, CA 91125, USA
3 California Institute of Technology, Jet Propulsion Laboratory, MS 100-22, Pasadena, CA 91125, USA
(Received 1 July 2003 / Accepted 19 April 2004)
Abstract
We present BAX, Base de Données Amas de Galaxies X
(http://bax.ast.obs-mip.fr), a multi-wavelength database dedicated to
X-ray clusters and groups of galaxies allowing detailed information retrieval.
BAX is designed to support astronomical research by providing
access
to published measurements of the main physical quantities
and to the related bibliographic references:
basic data stored in the database are cluster/group identifiers, equatorial
coordinates, redshift, flux, X-ray luminosity (in the ROSAT band) and
temperature, and links to additional linked parameters
(in X-rays, such as spatial profile
parameters, as well as SZ parameters of the hot gas, lensing measurements,
and data at other
wavelengths, such as optical and radio).
The clusters and groups
in BAX can be queried by the basic parameters as well as the
linked parameters or combinations of these.
We expect BAX to become an important tool for
the astronomical community. BAX
will optimize various aspects of the scientific analysis of X-ray clusters
and groups of galaxies,
from proposal planning to data collection, interpretation and publication,
from both ground based
facilities like MEGACAM (CFHT), VIRMOS (VLT) and space missions like
XMM-Newton,
Chandra and Planck.
Key words: galaxies: clusters: general -- X-rays: galaxies -- astronomical databases: miscellaneous
SIMBAD Objects
Tables at the CDS
© ESO 2004
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