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Cross-calibration of the XMM-Newton EPIC pn and MOS on-axis effective areas using 2XMM sources

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journal contribution
posted on 2015-10-08, 11:30 authored by Andrew M. Read, M. Guainazzi, S. Sembay
Aims. We aim to examine the relative cross-calibration accuracy of the on-axis effective areas of the XMM-Newton EPIC pn and MOS instruments. Methods. Spectra from a sample of 46 bright, high-count, non-piled-up, isolated on-axis point sources are stacked together, and model residuals are examined to characterize the EPIC MOS-to-pn inter-calibration. Results. The MOS1-to-pn and MOS2-to-pn results are broadly very similar. The cameras show the closest agreement below 1 keV, with MOS excesses over pn of 0–2% (MOS1/pn) and 0–3% (MOS2/pn). Above 3 keV, the MOS/pn ratio is consistent with energy-independent (or only mildly increasing) excesses of 7–8% (MOS1/pn) and 5–8% (MOS2/pn). In addition, between 1–2 keV there is a “silicon bump” − an enhancement at a level of 2–4% (MOS1/pn) and 3–5% (MOS2/pn). Tests suggest that the methods employed here are stable and robust. Conclusions. The results presented here provide the most accurate cross-calibration of the effective areas of the XMM-Newton EPIC pn and MOS instruments to date. They suggest areas of further research where causes of the MOS-to-pn differences might be found, and allow the potential for corrections and possible rectification of the EPIC cameras to be made in the future.

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Citation

Astronomy and Astrophysics, 2014, 564, pp. ?-? (7)

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Astronomy and Astrophysics

Publisher

EDP Sciences

issn

0004-6361

Copyright date

2014

Available date

2015-10-08

Publisher version

http://www.aanda.org/articles/aa/abs/2014/04/aa23422-14/aa23422-14.html

Language

en

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