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Table 1.

Log of the XMM-Newton AO14 and 2012 observations of RX J1605.3+3249.

obsid Date Inst. Mode Duration GTI
(s) (%)
0764460201 2015-07-21 pn FF 118 344 97
2015-07-21 MOS1 LW 110 089 100
2015-07-21 MOS2 LW 119 079 100
2015-07-21 RGS1 SES 120 169 100
2015-07-21 RGS2 SES 120 113 100
0764460301 2015-07-26 pn FF 65 038 96
2015-07-26 MOS1 LW 66 650 100
2015-07-26 MOS2 LW 66 629 100
2015-07-26 RGS1 SES 66 858 100
2015-07-26 RGS2 SES 66 757 100
0764460401 2015-08-20 pn FF 68 656 81
2015-08-20 MOS1 LW 70 459 91
2015-08-20 MOS2 LW 71 629 90
2015-08-20 RGS1 SES 71 858 91
2015-08-20 RGS2 SES 71 777 89
0764460501 2016-02-10 pn FF 59 932 96
2016-02-10 MOS1 LW 61 540 100
2016-02-10 MOS2 LW 61 495 100
2016-02-10 RGS1 SES 61 749 100
2016-02-10 RGS2 SES 61 675 100

0671620101 2012-03-06 pn FF 58 542 68
2012-03-06 MOS1 FF 57 432 89
2012-03-06 MOS2 FF 57 008 90
2012-03-06 RGS1 SES 60 406 88
2012-03-06 RGS2 SES 60 406 84

Notes. The EPIC cameras were operated in imaging mode and the thin filter was used. The RGS detectors were operated in high event rate with SES spectroscopy mode for readout. We list the percentage of good time intervals (GTIs) after filtering out periods of high background activity (see text for details).

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