Table A.3
Observation log of public Swift observations and the X-ray flares detected in this work.
Observations | Flares | ||||||||||
Mean | |||||||||||
First | Last | Number | Total exposure | Non-flaring level | η obs a | # | Start | Stop | Durationb | Count ratec | Fluxd |
(UT) | (UT) | (ks) | (count s-1) | (%) | (UT) | (UT) | (s) | (count s-1) | (10-12 erg s-1 cm-2) | ||
|
|||||||||||
2006-02-24 22:55:12 | 2006-11-02 14:22:34 | 198 | 261.7 | 0.021 ± 0.002 | 24.6 | 1 | 2006-07-13 21:57:36 | 2006-07-13 23:39:50 | 924 | 0.031 ± 0.007 | 15.3 |
2007-02-16 21:38:52 | 2007-11-02 13:52:19 | 163 | 174.6 | 0.025 ± 0.004 | 24.6 | 2 | 2007-03-03 00:38:21 | 2007-03-03 02:34:56 | 2018 | 0.012 ± 0.004 | 9.21 |
2008-02-19 23:02:24 | 2008-10-30 09:14:24 | 161 | 199.3 | 0.024 ± 0.003 | 24.6 | 3 | 2008-03-25 20:24:00 | 2008-03-25 23:36:58 | 707 | 0.056 ± 0.011 | 20.8 |
4 | 2008-05-01 14:15:22 | 2008-05-01 20:39:50 | 1056 | 0.029 ± 0.007 | 8.66 | ||||||
5 | 2008-10-17 17:15:22 | 2008-10-17 22:09:07 | 1369 | 0.036 ± 0.007 | 11.9 | ||||||
2009-06-04 07:23:31 | 2009-11-01 21:37:26 | 36 | 34.64 | 0.028 ± 0.009 | 24.6 | ..................... | ..................... | ...... | ............... | ...... | |
2010-04-07 01:10:34 | 2010-10-31 10:10:34 | 62 | 70.33 | 0.030 ± 0.006 | 24.6 | 6 | 2010-06-12 10:23:31 | 2010-06-12 12:07:12 | 1081 | 0.127 ± 0.012 | 49.3 |
2011-02-04 16:53:46 | 2011-11-02 15:38:53 | 81 | 76.78 | 0.025 ± 0.006 | 24.6 | ..................... | ..................... | ...... | ............... | ...... | |
2012-02-05 20:12:29 | 2012-10-31 23:21:07 | 79 | 73.95 | 0.020 ± 0.005 | 24.6 | ..................... | ..................... | ...... | ............... | ...... | |
2013-02-03 22:26:24 | 2013-10-31 01:17:46 | 191 | 185.4 | 0.145 ± 0.009 | 20.0e | ..................... | ..................... | ...... | ............... | ...... | |
2014-02-03 18:57:36 | 2014-11-02 12:56:09 | 236 | 231.4 | 0.056 ± 0.007 | 24.3 | 7 | 2014-09-09 11:41:17 | 2014-09-09 11:58:34 | 975 | 0.128 ± 0.013 | 59.4 |
2015-02-03 00:18:43 | 2015-11-02 15:14:24 | 231 | 211.1 | 0.033 ± 0.004 | 24.6 | 8 | 2015-11-02 14:58:34 | 2015-11-02 15:14:24 | 993 | 0.074 ± 0.009 | 22.3 |
Notes.
Mean flare detection efficiency. Owing to the decay phase of the Galactic center magnetar, the average flare detection efficiency increases during this campaign: 16.2, 17.9, 18.5, 21.7, 22.5, and 23.3% during 2013 April 4–May 11, May 12–17, May 18–29, May 30–June 28, June 29–September 7 and September 8–October 31, respectively.
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