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Space TelescopesAbstract

Measurements with the Chandra X-ray Observatory's Flight Contamination Monitor

Chandra20191 min read102 words
Elsner, R. F., Kolodziejczak, J. J., ODell, S. L., Swartz, D. A., Tennant, A. F., and Weisskopf, M. C.
Marshall Space Flight Center

NASA's Chandra X-ray Observatory includes a Flight Contamination Monitor (FCM), a system of 16 radioactive calibration sources mounted to the inside of the Observatory's forward contamination cover. The purpose of the FCM is to verify the ground-to-orbit transfer of the Chandra flux scale, through comparison of data acquired during the ground calibration with those obtained in orbit, immediately prior to opening the Observatory's sun-shade door. Here we report results of these measurements., which place limits on the change in the mirror-detector system response and, hence, on any accumulation of molecular contamination on the mirrors' iridium-coated surfaces between the two sets of measurements.


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