Table 1
Log of the simultaneous observations of J1023 on 2016 May 8–9.
Satellite | Obs. ID | Instrument | Mode | Start – End time of exposure | Exposurea | Source net count rateb |
---|---|---|---|---|---|---|
(UTC) | (ks) | (counts s−1) | ||||
XMM–Newton | 0784700201 | EPIC pn | FT | 2016/05/08 04:21:57 – 2016/05/09 14:46:27 | 121.7 | 3.641 ± 0.008 |
EPIC MOS 1 | SW | 2016/05/08 03:47:12 – 2016/05/09 12:08:48 | 112.9 | 1.001 ± 0.003 | ||
EPIC MOS 2 | SW | 2016/05/08 03:47:57 – 2016/05/09 12:09:02 | 113.0 | 1.004 ± 0.004 | ||
RGS 1 | Spectroscopy | 2016/05/08 03:47:02 – 2016/05/09 14:42:33 | 125.4 | 0.0893 ± 0.0008 | ||
RGS 2 | 2016/05/08 03:47:10 – 2016/05/09 14:43:21 | 125.6 | ||||
OM | Image | 2016/05/08 07:49:52 – 2016/05/09 16:46:19 | 100.0 | – | ||
NuSTAR | 30201005002 | FPMA | Science | 2016-05-07 15:34:34 – 2016-05-09 15:13:26 | 86.0 | 0.173 ± 0.001 (70%) |
FPMB | 85.7 | 0.166 ± 0.001 (71%) | ||||
Swift | 0790180101 | UVOT | event | 2016/05/08 18:45:01 – 2016/05/09 12:21:57 | 9.5 | 0.90 ± 0.01 |
Notes. (a) Deadtime corrected on-source exposure.(b) Background-subtracted count rate in the 0.3–10 keV energy band for the EPIC instruments, in the 0.35–2.5 keV energy bandfor the combined RGS first order data sets, in the 3–79 keV energy band for the NuSTAR data (the number in parentheses representing the fractional contributionfrom the 3–10 keV band), and in the UV M2 filter for the Swift UVOT data.
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