Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...30..569a&link_type=abstract
(European Space Agency, ESLAB Symposium on X-ray Astronomy, 15th, Amsterdam, Netherlands, June 22-26, 1981.) Space Science Revie
Astronomy and Astrophysics
Astronomy
6
Rosat Mission, Satellite-Borne Instruments, Spaceborne Astronomy, Spaceborne Telescopes, X Ray Sources, X Ray Telescopes, Angular Resolution, Focal Plane Devices, German Space Program, Germany, International Cooperation
Scientific paper
It is expected that a large number (more than 100,000) of new sources will be discovered and located to an accuracy of 1 arcmin. After the survey, which will take about half a year, the instrument will be used for detailed observations of selected targets. The X-ray telescope comprises a fourfold nested Wolter type I mirror system, with an aperture of 80 cm and a focal length of 240 cm, and three focal plane detectors. In the baseline version, these will be imaging proportional counters (0.1-2 keV) giving a field of view of 2 deg x 2 deg.
Aschenbach Bernd
Braeuninger Heinrich
Briel Ulrich
Brinkmann Wolfgang
Fink Henner
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