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...

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Bibliographic Details
Main Authors: Plucinsky, Paul P., Haberl, F., Dewey, Dan, Beardmore, Andrew P., DePasquale, Joseph M., Godet, Olivier, Grinberg, Victoria, Pollock, A. M. T., Sembay, Steven, Smith, Randall K., Miller, Eric D
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: Society of Photo-optical Instrumentation Engineers 2010
Online Access:http://hdl.handle.net/1721.1/52653