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