MPE/xray/wave
Max-Planck-Institut für extraterrestrische Physik

8.4 Data Output of the All-Sky Survey
 

Verweis Deutsche Version .  MPE . HEG  . X-Ray Astronomy . Wave . ROSAT
X-Ray Astronomy
Wave
ROSAT
The X-ray Satellite ROSAT
Highlights
Gallery
Publications
Workshops
Calibration
Timeline
Processing
News
ROSAT Results Archive
Catalogues
ROSAT Link & Surf
XMM-Newton
Chandra
Other Projects
Data Center
Exsas

Search
Impressum
Contact

Valid HTML 4.01!

next up previous contents index
Next: Standard Products of the Up: Standard Analysis Software System Previous: 8.3 Data Set of

8.4 Data Output of the All-Sky Survey

 

The main objectives of the first all-sky survey in soft X-rays have been the creation of a catalogue with X-ray sources and their properties [Voges et al.1995, Voges et al.1996, Voges et al.1997, Voges1997, Gruber et al.1997] and the generation of a sky map of the diffuse X-ray background [Snowden et al.1995a]. SASS correlates the ROSAT all-sky survey sources (RASS) recorded by the PSPC detector with the about tex2html_wrap_inline14397 entries of the SIMBAD catalogue as well as with 94 user-supplied catalogues with approximately tex2html_wrap_inline14399 entries. These user-supplied catalogues --classified according to their observation method (radio, IR, X-ray, tex2html_wrap_inline14401 -ray band) or their object class (stars, galaxies, cluster of galaxies, supernova remnants, cataclysmic variables)-- are supplied by the ROSAT scientific working groups at MPE to help in identifying the new X-ray sources. In addition, for each RASS source finding charts are produced for follow-up observations using the ROE/NRL object catalogue for the southern sky (on-line) and the APM object catalogue for the northern sky (on-line) [Voges1992].



If you have problems/suggestions please send mail to xray-info @ mpe . mpg . de

© X-Ray Group at MPE (group)
last update:2001/09/27 22:35:13, editor of this page:Ortwin Schwentker


up © Max-Planck-Institut für extraterrestrische Physik