The Einstein All-Sky IPC slew survey

Details The Einstein All-Sky IPC slew survey The Einstein All-Sky IPC slew survey

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..847e&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 2: AGN and the X Ray Background p 847-851 (SEE N90-258

Astronomy and Astrophysics

Astronomy

Background Radiation, Galactic Clusters, Galactic Radiation, Heao 2, Imaging Techniques, Proportional Counters, Surveys, Astro Missions (Sts), Bl Lacertae Objects, Cataclysmic Variables, Data Reduction, Quasars, Rosat Mission, Stellar Parallax, X Ray Spectra

Scientific paper

The construction of the Einstein All-Sky Imaging Proportional Counter (IPC) slew survey is considered. It contains approximately 1000 sources between 10-12 and 10-10 erg/sq cm/s with a concentration toward the ecliptic poles and away from the galactic plane. Several sizable samples of bright soft X-ray selected objects for follow-up ROSAT and ASTRO-D observations and statistical study are presented. The survey source list is expected to be available by late 1989. Both paper and remote access online data base versions are to be available. An identification program is considered.

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