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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.

(a)

The average flare detection efficiency above the corresponding non-flaring level.

(b)

The flare duration corresponds to the corresponding observing time.

(c)

The flare mean count rates are computed after subtraction of the non-flaring level.

(d)

Mean unabsorbed flux between 2 and 10 keV determined for NH = 14.3 × 1022 cm-2 and Γ = 2.

(e)

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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