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Proceedings Paper

XMM science simulator: EPIC mode performance issues
Author(s): David H. Lumb; J. Bakker; Marco W. Beijersbergen; J. Brumfitt; K. Galloway; L. Jalota; Fred A. Jansen; H. Siddiqui; Giuseppe Vacanti; Igor Zayer
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Paper Abstract

We describe simulations of the XMM EPIC instruments which suggests the correct operating mode must be chosen to ensure that spectral analysis of the data is not compromised by 'pile-up' effects. We contrast the performance with the AXAF CCD imaging spectrometer, and show that the XMM EPIC instruments will access a larger range of source fluxes due to a combination of higher effective area and better over- sampling of its mirror response function. Targets exceeding a flux of a few 10-12 ergs cm-2s-1 will be compromised for spectral analysis in AXAF. For XMM, the corresponding flux levels will be 10-11 ergs cm-11 ergs cm-2s-1. This feature warrants careful attention in calibration.

Paper Details

Date Published: 10 November 1998
PDF: 11 pages
Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); doi: 10.1117/12.330323
Show Author Affiliations
David H. Lumb, European Space Agency/ESTEC (Netherlands)
J. Bakker, European Space Agency/ESTEC (Netherlands)
Marco W. Beijersbergen, European Space Agency/ESTEC (Netherlands)
J. Brumfitt, European Space Agency/ESTEC (Netherlands)
K. Galloway, European Space Agency/ESTEC (Netherlands)
L. Jalota, European Space Agency/ESTEC (Netherlands)
Fred A. Jansen, European Space Agency/ESTEC (Netherlands)
H. Siddiqui, European Space Agency/ESTEC (Netherlands)
Giuseppe Vacanti, European Space Agency/ESTEC (Netherlands)
Igor Zayer, European Space Agency/ESTEC (Netherlands)


Published in SPIE Proceedings Vol. 3445:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX
Oswald H. W. Siegmund; Mark A. Gummin, Editor(s)

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