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Table 1
XMM-Newton observations of GX 13 + 1.
| Obs | Observation | Observation Times (UTC) | T | C | ||
| Num | ID | Start | End | (ks) | (s-1) | |
| (year month day) | (h:mn) | (h:mn) | ||||
|
|
||||||
| 1 | 0122340101 | 2000 March 30 | 14:10 | 16:58 | 6.0 | 674 |
| 2 | 0122340901 | 2000 April 01 | 04:29 | 07:54 | 8.1 | 781 |
| 3 | 0122341001 | 2000 April 01 | 08:51 | 11:16 | 4.6 | 690 |
| 4 | 0505480101 | 2008 March 09 | 15:48 | 22:50 | 22.9 | 843 |
| 5 | 0505480701 | 2008 March 11 | 19:00 | 23:10 | 12.0 | – |
| 6 | 0505480201 | 2008 March 11 | 23:10 | 27:16 | 12.4 | 909 |
| 7 | 0505480301 | 2008 March 22 | 02:20 | 07:15 | 15.3 | 818 |
| 8 | 0505480501 | 2008 March 25 | 23:01 | 26:59 | 11.9 | 761 |
| 9 | 0505480401 | 2008 September 5 | 21:49 | 26:48 | 15.5 | 746 |
Notes. Results from the first three observations are reported in Sidoli et al. (2002). T is the total EPIC pn exposure time and C is the pn 0.6–10 keV total count rate after dead-time correction. In all cases the EPIC pn thin filter was used. For obs 5 only RGS and OM data are available.
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