The SMC SNR 1E0102.2-7219 as a calibration standard for x-ray astronomy in the 0.3-2.5 keV bandpass
@inproceedings{Plucinsky2008TheSS, title={The SMC SNR 1E0102.2-7219 as a calibration standard for x-ray astronomy in the 0.3-2.5 keV bandpass}, author={P. Plucinsky and F. Haberl and D. Dewey and A. Beardmore and J. DePasquale and O. Godet and V. Grinberg and E. Miller and A. Pollock and S. Sembay and R. Smith}, booktitle={Astronomical Telescopes + Instrumentation}, year={2008} }
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 the response models of the ACIS CCDs on the Chandra X-ray Observatory (CXO), the EPIC CCDs on the XMM-Newton Observatory, the XIS CCDs on the Suzaku Observatory, and the XRT CCD on the Swift… CONTINUE READING
8 Citations
Cross-calibration of the x-ray instruments onboard the Chandra, Suzaku, Swift, and XMM-Newton Observatories using the SNR 1E 0102.2-7219
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AN X-ray upper limit on the presence of a neutron star for the small magellanic cloud supernova remnant 1E0102.2-7219
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The evolution of the ACIS contamination layer over the 16-year mission of the Chandra X-ray Observatory
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Comparative analysis and variability of the Jovian X‐ray spectra detected by the Chandra and XMM‐Newton observatories
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The complicated evolution of the ACIS contamination layer over the mission life of the Chandra X-ray Observatory
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