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The Astro -E/XRS Calibration Program and ResultsXRS is the microcalorimeter X-ray detector aboard the US-Japanese ASTRO-E observatory, which is scheduled to be launched in early 2000. XRS is a high resolution spectrometer- with less than 9 eV resolution at 3 keV and better than 14 eV resolution over its bandpass ranging from about 0.3 keV to 15 keV. Here we present the results of our first calibration of the XRS instrument. We describe the methods used to extract detailed information about the detection efficiency and spectral redistribution of the instrument. We also present comparisons of simulations and real data to test our detector models
Document ID
20010035865
Acquisition Source
Goddard Space Flight Center
Document Type
Other
Authors
Gendreau, Keith C. (Maryland Univ. College Park, MD United States)
Audley, M. Damian (Tokyo Univ. Sagamihara, Japan)
Arnaud, Keith A. (Maryland Univ. College Park, MD United States)
Boyce, Kevin R. (NASA Goddard Space Flight Center Greenbelt, MD United States)
Fujimoto, Ryuichi (Tokyo Univ. Sagamihara, Japan)
Ishisaki, Yoshitaka (Tokyo Metropolitan Univ. Japan)
Kelley, Richard L. (NASA Goddard Space Flight Center Greenbelt, MD United States)
Mihara, Tatehiro (Institute of Physical and Chemical Research Japan)
Mitsuda, Kazuhisa (Tokyo Univ. Sagamihara, Japan)
Porter, F. Scott (NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 1999
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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