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Table 3

Summary of XMM-Newton observations of RX J1605.3+3249 used in the spectral analysis.

Ref. OBSID MJD Science mode Net exposure (ks) Observed flux (10-12 erg s-1 cm-2)



(days) MOS pn RGS MOS pn RGS MOS pn RGS

A 0073140301 52 284.146834 FF TI SES 25.156 17.855 6.06(8) 4.50(24)
B 0073140201 52 290.127905 FF TI SES 27.949 27.254 6.08(8) 4.51(23)
C 0073140501 52 294.123831 FF TI SES 22.102 21.742 6.09(10) 4.4(9)
D 0157360401 52 657.139334 FF LW SES 30.094 27.797 28.898 6.66(9) 6.636(25) 4.66(28)
E 0157360601 52 696.990896 FF LW SES 7.250 7.742 6.50(16) 4.6(3)
AO11 0671620101 55 992.811793 FF FF SES 51.407 39.875 52.125 6.12(9) 6.610(24) 4.12(15)

Notes. The net exposure time per camera (averages are considered for the two MOS and RGS detectors) is filtered for periods of high background activity. All the EPIC observations included in the analysis made use of the thin filter. The instrument science modes are full-frame (FF), timing (TI), large window (LW), and spectroscopy (SES). The observed flux is in energy band 0.2–12 keV (EPIC) and 0.35–2.5 keV (RGS).

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