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The ROSAT All-Sky Survey Bright Source Catalogue [ CATS home ] [ Back to CATS list ] [ ftp ]


1999A&A...349..389Voges+

Ses ALSO ReadMe.CDS about identifications with NED and NVSS.

The ROSAT All-Sky Survey Bright Source Catalogue (1RXS)

W. Voges, B. Aschenbach, Th. Boller, H. Bruuninger, U. Briel, W. Burkert, K. Dennerl, J. Englhauser, R. Gruber, F. Haberl, G. Hartner, G. Hasinger, M. Karster, E. Pfeffermann, W. Pietsch, P. Predehl, C. Rosso, J.H.M.M. Schmitt, J. Trumper, and H.-U. Zimmermann
Max-Planck-Institut fur extraterrestrische Physik, 85740 Garching, Germany

To be published in Astronomy and Astrophysics, 1996. The catalogue can be used for scientific purposes as long as the above publication is referenced.

Abstract

We present the ROSAT All-Sky Survey Bright Source Catalogue (RASS-BSC, revision 1RXS) derived from the all-sky survey performed during the first half year of the ROSAT mission in 1990/91. 18,811 sources are catalogued, with a limiting ROSAT PSPC countrate of 0.05 cts/s in the 0.1-2.4 keV energy band. The sources have a detection likelihood of at least 15 and contain at least 15 source photons. At a brightness limit of 0.1 cts/s (8,547 sources) the catalogue represents a sky coverage of 92%. The typical positional accuracy is 30 arcsec.

For each source the ROSAT name, the position in equatorial co-ordinates, the positional error, the source countrate and error, the background countrate, exposure time, hardness-ratios HR1 and HR2 and errors, extent and likelihood of extent, and likelihood of detection are provided. For 94% of the sources visual inspection confirmed the results of the standard processing with respect to existence and position. The remaining 6% have been analyzed using interactive methods; these sources have been flagged. Broad band images are available for a subset of the flagged sources.

A list containing correlations with other catalogues and identifications will follow soon.

Questions or comments may be directed to survey@rosat.mpe-garching.mpg.de. In particular we would be grateful if any errors or inconsistencies found in the data would be reported to this e-mail address.


Browsing the catalogue via WWW Subsets of the catalogue sources - selected by certain properties - may be retrieved via the ROSAT Source Browser (also available in a simplified version). In certain cases, the list provided contains also links to source images. ---------------------------------------------------------------------------- Retrieving the full catalogue The ROSAT All-Sky Survey Bright Source Catalogue can be retrieved via your WWW browser: 1. Select the 'Load to local disk' option of your WWW browser. 2. Open URL http://www.rosat.mpe-garching.mpg.de/survey/rass-bsc/rass-bsc-1rxs.cat.gz 3. Be patient - transmission can take a while (catalogue size is 1 MB). 4. Specify a name for the catalogue file in your local computer environment (recommended: rass-bsc-1rxs.cat.gz). Alternatively, the catalogue is accessible via anonymous ftp: ftp ftp.rosat.mpe-garching.mpg.de user anonymous, as password cd archive/survey/rass-bsc binary get README get rass-bsc-1rxs.cat.gz get quit After transmission, the local catalogue file has to be uncompressed by 'gunzip '. A description of the catalogue format is available. ---------------------------------------------------------------------------- Correlation with other Catalogues An extended version of the ROSAT All-Sky Survey Bright Source Catalogue is in preparation. This catalogue will contain possible source identifications obtained by cross-correlating the ROSAT All-Sky Survey Bright Source Catalogue with many other catalogues, and source identifications obtained by optical follow-up observations. Call for identifications: We plan to include further identifications of X-ray sources into the identification catalogue. Please contact survey@rosat.mpe-garching.mpg.de, if you are interested to contribute your identifcations to this catalogue. ---------------------------------------------------------------------------- Feedback to: survey@rosat.mpe-garching.mpg.de (jer / 14-Jun-96)