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- W2062704457 abstract "ABSTRACT The prime focal instrument of the ROSAT X -ray telescope, the position sensitive proportio-nal counter (PSPC), has been calibrated extensively with X -rays in the energy range from 0.28 to1.7 keV. We developed a method to measure the differential spatial non -linearities caused by thedigitizing effects of the anode and cathode grids, and the bulging of the thin entrance window, and also the position dependent gain of the counter. From these measurements we derivedtables, which are used to correct each single recorded event in position as well as in pulse height. We will present the calibration method and the performance achieved for the PSPC. 1. INTRODUCTION The ROSAT (ROentgen SATellit) missions will be the first all sky survey in the energy bandfrom 0.1 to 2.0 keV, performed with an X -ray telescope and imaging X -ray detectors. The teles- cope is a Wolter type I mirror system, fourfold nested to increase the collecting area, with a maximum aperture of 83 cm and with a focal length of 240 cm. The mirror system and its per-" @default.
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- W2062704457 date "1988-12-21" @default.
- W2062704457 modified "2023-09-25" @default.
- W2062704457 title "X-Ray Calibration Of The Rosat Position Sensitive Proportional Counter" @default.
- W2062704457 doi "https://doi.org/10.1117/12.948738" @default.
- W2062704457 hasPublicationYear "1988" @default.
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