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ROSATCAT
ROSAT_WGA
CATS contains two version of ROSAT catalog:
ROSATCAT and
ROSAT_WGA
THE FIRST ROSAT SOURCE CATALOG
During the ROSAT workshop at MPE on October 26, 1994 Wolfgang Voges
announced on behalf of the ROSAT Consortium (MPE-Garching, GSFC/SAO-US,
and WFC-Consortium-UK) the public release of "THE FIRST ROSAT SOURCE
CATALOGUE OF POINTED OBSERVATIONS WITH THE PSPC". This catalogue
contains 50,408 sources from 2876 pointed observations. For each source
the following properties are provided: the observation number, the
ROSAT name, the position in equatorial and in galactic co-ordinates,
four positional errors (intrinsic, systematic, boresight, and total),
the source count-rate and its error, the background countrate,
exposure time, hardness-ratios HR1 and HR2 and their errors, extent
and likelihood of extent, likelihoods of the map-detect algorithm and
of the maximum-likelihood detection algorithm, flags to indicate in
which energy band and by what algorithm the source was detected, the
detection cell size, the off-axis radius, the distances to the nearest
rib and source (before and after removal of ambiguous sources), and a
source confusion flag (set if another source is within 2.1*FWHM of the
point-spread function).
small_wgacat.txt
a small dump of the catalog with ra,dec,lii,bii,
qflag,name,id,exposure,count_rate,count_rate_error,
offset,snr,probability.
Abstract
We have taken all the data contained in the ROSAT public archive and generated
a catalog of 45,000 point sources. This catalog has been made public through
the "http://heasarc.gsfc.nasa.gov/0" HEASARC and
"http://www.esrin.esa.it/htdocs/esis/esis.html" ESIS
online services. The detection technique uses a sliding
box and has been optimized for point source detection. A K-S test for
variability has been made and a number of variable sources identified. A
hardness and softness ratio is also used to identify unusually soft or hard
sources. Cross-correlations against the major optical, radio, x-ray and ir
catalogs are presented.