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1.1 Introduction

 

On June 1 tex2html_wrap_inline17187 , 1990 the ROSAT observatory [Trümper1983] was launched successfully into a circular orbit of 575 km altitude and 53 degrees inclination.     The satellite carries two telescope systems on board: an X-ray telescope,   operating in the energy range 0.1 to 2.4 keV, and a smaller XUV telescope sensitive in the range from about 20 to 200 eV.   ROSAT --an abbreviation for Röntgen Satellit-- is a German project with major contributions from the United States and the United Kingdom. Specifically the US (NASA/SAO) provided one of the three focal detectors of the X-ray telescope and launched the satellite, and the XUV telescope was built by a consortium of five British institutes, namely the Universities of Leicester and Birmingham, the Mullard Space Science Laboratory, the Imperial College of Science Technology and Medicine and the Rutherford Appleton Laboratory.

After completing an initial Calibration and Verification Phase (CV Phase)   ROSAT started on July 30, 1990, its main scientific task: to perform the first all sky survey   with an imaging telescope both in the soft X-ray and the XUV regimes. After this survey, which lasted six months, an extended observatory program began (on a guest observer basis) with pointings   to many individual targets. In the meantime the 4 tex2html_wrap_inline17189 pointed observation period (AO-4) has been almost completed and a fith one (AO-5; HRI only) will begin in October 1994.



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