The SMC SNR 1E0102.2-7219 as a calibration standard for X-ray astronomy in the 0.3-2.5 keV bandpass
The flight calibration of the spectral response of CCD instruments below 1.5 keV is difficult in general because of the lack of strong lines in the on-board calibration sources typically available. We have been using E0102, the brightest supernova remnant in the Small Magellanic Cloud, to evaluate t...
Main Authors: | , , , , , , , , , , |
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Other Authors: | |
Format: | Article |
Language: | en_US |
Published: |
Society of Photo-optical Instrumentation Engineers
2010
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Online Access: | http://hdl.handle.net/1721.1/52653 |