Paper
10 November 1998 XMM science simulator: EPIC mode performance issues
David H. Lumb, J. Bakker, Marco W. Beijersbergen, J. Brumfitt, K. Galloway, L. Jalota, Fred A. Jansen, H. Siddiqui, Giuseppe Vacanti, Igor Zayer
Author Affiliations +
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.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David H. Lumb, J. Bakker, Marco W. Beijersbergen, J. Brumfitt, K. Galloway, L. Jalota, Fred A. Jansen, H. Siddiqui, Giuseppe Vacanti, and Igor Zayer "XMM science simulator: EPIC mode performance issues", Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); https://doi.org/10.1117/12.330323
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KEYWORDS
Charge-coupled devices

Calibration

Cameras

Device simulation

Monte Carlo methods

Mirrors

Molybdenum

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