2004A&A...414..767K


Query : 2004A&A...414..767K

2004A&A...414..767K - Astronomy and Astrophysics, volume 414767-776 (2004/2-1)

Properties of the background of EPIC-pn onboard XMM-Newton.

KATAYAMA H., TAKAHASHI I., IKEBE Y., MATSUSHITA K. and FREYBERG M.J.

Abstract (from CDS):

We have investigated the background properties of EPIC-pn onboard XMM-Newton to establish the background subtraction method. Count rates of the background vary violently by two orders of magnitude at the maximum, while during the most quiet period, these are stable within 8% at a 1σ level. The overall spectrum is dominated by particle events above 5keV, and its spatial variation is also found. The long-term variation of the background is also investigated with CAL CLOSED data, where the filter wheel was in closed position with the internal calibration source illuminating the sensitive area. The average background count rate decreased by 20% from March 2000 to January 2001, but it regained in February 2001. For the modeling of the background spectrum, we investigate relations between the 2.0-7.0keV count rate and some characteristic parameters. The 2.0-7.0keV background count rate shows a good correlation with the count rate of events outside the field of view. This correlation is usable for the modeling of the background.

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Journal keyword(s): X-rays: general - instrumentation: detectors

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* WW Hor CV* 02 36 11.4433563560 -52 19 13.934884433           ~ 81 0
2 RX J0720.4-3125 N* 07 20 24.961 -31 25 50.21   26.1   27.0   ~ 316 0
3 QSO B0737+744 BLL 07 44 05.3750968872 +74 33 58.256429832     16.89 16.6   ~ 144 0
4 NAME Lockman Hole reg 10 45 00.0 +58 00 00           ~ 910 0
5 QSO B1229+6430 BLL 12 31 31.3949261640 +64 14 18.280701600   18.36 17.62 14.3   ~ 160 2

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