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Table A.2

List of flares with a peak above the 95% confidence level in the power spectrum.

Flare no. Start time End time Instrument Method Period (s) References

008* 2014-09-23 23:08:20 2014-09-23 23:13:52 GOES 0.5–4 Å Regular
010* 2014-09-24 17:49:04 2014-09-24 17:50:18 GOES 1–8 Å Rebinned (2) 2
010* 2014-09-24 17:49:01 2014-09-24 17:49:50 Vernov Rebinned (2) 2
022 2014-10-17 05:23:18 2014-10-17 05:26:35 NoRH Rebinned (3)
024 2014-10-17 15:35:30 2014-10-17 15:37:54 GOES 1–8 Å Rebinned (2)
027 2014-10-18 01:04:10 2014-10-18 01:08:30 NoRH Rebinned (3)
029 2014-10-18 07:36:14 2014-10-18 07:48:48 GOES 1–8 Å Regular 1
030 2014-10-18 13:14:38 2014-10-18 13:15:52 GOES 0.5–4 Å Regular
035 2014-10-18 19:02:30 2014-10-18 19:06:58 GOES 1–8 Å Regular 2
037 2014-10-19 01:35:00 2014-10-19 01:43:00 GOES 0.5–4 Å Regular
037 2014-10-19 01:36:28 2014-10-19 01:42:42 NoRH Regular
038 2014-10-19 04:20:24 2014-10-19 04:24:56 GOES 1–8 Å Regular
038 2014-10-19 04:20:24 2014-10-19 04:24:56 GOES 0.5–4 Å Regular
038 2014-10-19 04:41:39 2014-10-19 04:50:00 GOES 0.5–4 Å Regular
049* 2014-10-20 09:05:45 2014-10-20 09:08:14 GOES 0.5–4 Å Rebinned (3) 1
052* 2014-10-20 14:41:47 2014-10-20 14:43:33 GOES 1–8 Å Regular
054* 2014-10-20 16:23:02 2014-10-20 16:31:20 GOES 1–8 Å Regular
056* 2014-10-20 18:57:51 2014-10-20 18:59:01 Fermi 25–50 keV Rebinned (3) 1, 2
056* 2014-10-20 18:57:53 2014-10-20 18:59:02 Vernov Regular 1, 2
058* 2014-10-20 22:45:18 2014-10-20 22:49:46 GOES 1–8 Å Rebinned (2) 1, 3
058* 2014-10-20 22:45:18 2014-10-20 22:49:46 GOES 0.5–4 Å Rebinned (2) 1, 3
068* 2014-10-22 01:43:04 2014-10-22 01:46:36 GOES 1–8 Å Regular
068* 2014-10-22 01:43:04 2014-10-22 01:46:36 GOES 0.5–4 Å Regular
072* 2014-10-22 14:06:55 2014-10-22 14:12:02 Fermi 50–100 keV Regular 5
072* 2014-10-22 14:06:56 2014-10-22 14:09:30 GOES 1–8 Å Regular 5
072* 2014-10-22 14:15:24 2014-10-22 14:23:40 GOES 0.5–4 Å Regular 5
079* 2014-10-24 02:38:30 2014-10-24 02:41:20 NoRH Rebinned (2)
081* 2014-10-24 03:59:30 2014-10-24 04:01:00 NoRH Rebinned (3)
085* 2014-10-24 21:19:38 2014-10-24 21:23:47 GOES 0.5–4 Å Regular
092* 2014-10-25 17:02:11 2014-10-25 17:10:10 GOES 1–8 Å Regular 1
092* 2014-10-25 17:02:11 2014-10-25 17:10:10 GOES 0.5–4 Å Regular 1
098* 2014-10-26 10:48:52 2014-10-26 10:50:34 Fermi 25–50 keV Regular
104* 2014-10-26 18:11:18 2014-10-26 18:15:24 GOES 0.5–4 Å Regular 1
104* 2014-10-26 18:12:40 2014-10-26 18:15:28 Fermi 25–50 keV Regular 1
105* 2014-10-26 18:45:04 2014-10-26 18:48:02 GOES 1–8 Å Regular 1
106* 2014-10-26 20:03:42 2014-10-26 20:11:18 GOES 1–8 Å Rebinned (2) 1
106* 2014-10-26 20:03:42 2014-10-26 20:11:18 GOES 0.5–4 Å Rebinned (2) 1
106* 2014-10-26 20:03:38 2014-10-26 20:09:02 Fermi 25–50 keV Regular 1
117* 2014-10-27 17:36:36 2014-10-27 17:37:26 GOES 1–8 Å Regular 1
129 2014-10-29 09:58:00 2014-10-29 10:01:45 EVE Rebinned (2) 1
135 2014-10-29 21:21:33 2014-10-29 21:22:19 Fermi 25–50 keV Rebinned (3) 1, 2
135 2014-10-29 21:21:28 2014-10-29 21:22:52 Vernov Rebinned (3) 1, 2
138 2014-10-29 23:44:16 2014-10-29 23:45:48 NoRH Regular
140 2014-10-30 01:28:38 2014-10-30 01:30:30 GOES 1–8 Å Rebinned (2) 1, 3
141 2014-10-30 04:22:08 2014-10-30 04:28:00 GOES 1–8 Å Regular 1
142 2014-10-30 05:44:27 2014-10-30 05:45:45 GOES 1–8 Å Regular
142 2014-10-30 05:44:27 2014-10-30 05:45:43 NoRH Regular
147 2014-11-13 06:04:59 2014-11-13 06:07:15 NoRH Regular
152 2014-11-15 11:56:08 2014-11-15 12:02:58 GOES 1–8 Å Regular 1
152 2014-11-15 11:56:08 2014-11-15 12:02:58 GOES 0.5–4 Å Regular 1
152 2014-11-15 11:56:08 2014-11-15 12:02:58 EVE Regular 1
153 2014-11-15 20:42:57 2014-11-15 20:44:28 GOES 0.5–4 Å Rebinned (2) 1
161* 2014-11-16 17:42:46 2014-11-16 17:45:24 GOES 0.5–4 Å Regular
177* 2014-11-22 06:02:16 2014-11-22 06:04:48 GOES 1–8 Å Regular
177* 2014-11-22 06:02:16 2014-11-22 06:04:48 GOES 0.5–4 Å Regular

Notes. The first column contains a numerical label for the flares (see also Table A.1), the second and third columns give the start and end times of the section of the flare where the QPP signal is most visible in the power spectrum, the fourth column is the instrument used, the fifth column is the type of power spectrum in which the signal was detected (the numbers for the rebinned power spectra refer to the number of frequency bins that were summed over, see Sect. 3), the sixth column is the QPP period, and finally the seventh column references other studies that find pulsations in the flare. Flare numbers marked with an asterisk indicate those that occurred while the active region was far enough away from the solar limb so that active region properties could be determined.

Reference. (1) Inglis et al. (2016); (2) Myagkova et al. (2016); (3) Cho et al. (2016); (5) Kuznetsov et al. (2016).

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