Hunting high and low: XMM monitoring of the eclipsing polar HU Aquarii

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Table 1:

Log of the XMM X-ray observations of HU Aqr.
Date	Detector¹	$T_{\rm Exp}$	Mean rate²
		(ks)	(cts/s)
2002 May 16-17	PN-sw	36.4	1.11
	MOS1-sw	37.2	0.19
	MOS2-sw	37.2	0.26
2003 May 19	PN-ti	18.5	0.94
	MOS1-ti	20.2	0.21
	MOS2-ti	20.0	0.18
2003 Oct. 24-25	PN-sw	11.4	0.011
	MOS1-sw	11.6	-
	MOS2-sw	11.6	-
2005 May 16	PN-ti	18.6	-
	MOS1-sw	19.4	0.0025
	MOS2-sw	19.4	0.0022

¹ The abbreviations after the PN/MOS detector indicate the instrument mode: sw = small window, ti = timing. ² In the bright phase interval $\phi = 0.62{-}0.91$ and $\phi = 0.05{-}0.18$ . Energy range used 0.18-10 keV and 0.3-10 keV for imaging and timing modes, respectively. Count rates have been corrected for the 65% encircled energy fraction corresponding to the aperture used.

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