Table 1
Joint observations of SRG/eROSITA (ObsID 300003) and XMM-Newton (0853000101) of 1H 0707-495.
| eROSITA | ||||
|---|---|---|---|---|
| Start (a) | End (b) | expo (c) | rate (d,e) | |
| TM1 | 19:00:00 | 22:59:12 | 14.2 | 1.43 ± 0.11 |
| TM2 | 20:06:50 | 22:59:12 | 10.3 | 1.20 ± 0.12 |
| TM5 | 09:00:48 | 22:59:12 | 49.4 | 2.68 ± 0.08 |
| TM6 | 09:00:48 | 22:59:12 | 50.3 | 2.91 ± 0.08 |
| TM7 | 09:00:48 | 22:59:12 | 49.8 | 2.89 ± 0.08 |
| XMM-Newton | ||||
| EPIC-pn | 09:38:14 | 01:21:40 (b) | 52.0 | 14.70 ± 0.19 |
| EPIC-MOS2 | 09:06:53 | 01:14:49 (b) | 57.3 | 3.49 ± 0.08 |
| OM | 09:14:54 | 11:46:42 | ||
| 14:58:42 | 01:21:10 (b) | 44.0 | 12.56 ± 0.26 | |
Notes. All eROSITA cameras were operated in FrameStore mode with the FILTER setup (TM3 and TM4 were still switched off), EPIC-pn and MOS2 cameras in LargeWindow mode with MEDIUM filter, OM in Image/Fast mode in several exposures. 1H 0707-495 was too weak forRGS1 and RGS2. EPIC-MOS1 was still in its non-scientific CALCLOSED setup due to a Single-Event-Upset in a previous observation. (a) For eROSITA the start and end date is October 11, 2019 (times in UTC). (b) For XMM-Newton the start date is October 11, 2019 and the end date is October 12, 2019 (times in UTC). Note the gap in OM exposure. (c) Net exposure time is given in ks. (d) For eROSITA and XMM-Newton the 0.5–0.8 keV net count rates are given in units of 10−2 counts s−1 after background subtraction. Note the different time ranges for the cameras. (e) The OM count rates are not re-scaled.
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