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Table 1

Observation log showing nights of observation of AD Leo.

Obs. date Start–end time (UTC) Obs (h) Exposure time (s) Number of spectra Flare energy (1031erg)

Hα Hβ He I 5876
2016-11-19 01:29–03:47 2.33 600 14
2016-11-20 00:01–00:32 0.5 600 3
2016-12-09 01:17–01:47 0.5 600 3
2016-12-16 23:25–01:30 2 600 12
2016-12-21 01:23–04:55 3.5 600 21
2017-02-03 23:54–00:15 0.33 600 2
2017-02-04 22:19–00:03 1.83 600 11
2017-02-13 01:11–04:21 3.17 600 19
2017-02-14(†) 22:37–04:44 6 600 36 12.05 ± 0.03 9.495 ± 0.077 0.553 ± 0.004
2017-02-15 22:58–04:26 5.33 600 32
2017-03-10 20:41–21:01 0.33 600 2
2017-03-10 18:51–01:51 6.83 600 41
2017-03-11 18:14–03:15 8.67 600 52
2017-03-12 18:25–02:24 3.83 600 23
2017-04-15 21:41–23:15 1.67 600 10
2017-05-03 20:55–21:25 0.5 600 3
2017-05-06 19:33–22:21 2.83 600 17
2017-05-07 19:17–20:20 1.17 600 7
2017-05-09 20:55–21:26 0.5 600 3
2017-05-10 20:16–21:19 1.17 600 7
2017-05-15(†) 20:31–21:47 1.25 600 8 1.593 ± 0.005 - -
2017-12-24 02:25–03:07 0.5 600 3
2017-12-25 23:53–05:07 3.67 600 22
2017-12-26 00:37–01:40 1.33 600 7
2017-12-28 22:53–00:06 1.25 600 8
2018-01-05 01:28–03:45 2.33 600 14
2018-02-12 19:25–23:23 2.67 600 16
2018-02-13(†) 18:29–04:48 10 600 60 3.155 ± 0.033 1.154 ± 0.012 0.154 ± 0.002
2018-02-14 18:39–03:04 8.17 600 49 5.854 ± 0.031 2.195 ± 0.036 0.443 ± 0.007
21.2 ± 0.4 8.323 ± 0.319 1.998 ± 0.077
2018-02-16(†) 18:26–03:50 7 600 42 19.472 ± 0.079 5.11 ± 0.06 0.428 ± 0.002
2018-02-18 18:25–01:03 5.83 600 35 11.909 ± 0.082 3.715 ± 0.069 0.391 ± 0.003
2018-02-26 21:04–04:17 7 600 42 14.599 ± 0.061 3.081 ± 0.021 0.499 ± 0.004
2018-02-27 18:22–04:05 9.33 600 56
2018-02-28 18:19–04:20 9.67 600 58
2018-03-01 18:14–04:00 9.33 600 56
2018-03-04 00:15–02:21 2.17 600 13
2018-03-05 20:35–02:47 5.67 600 34 8.406 ± 0.135 5.031 ± 0.255 0.536 ± 0.013
2018-03-08 23:03–03:46 3.5 600 21
2018-03-24 18:35–02:16 6.92 300 83
2018-03-29 19:47–01:36 4.58 300 55
2018-04-23 19:34–23:21 3.5 300 42
2018-04-27(†) 19:43–22:22 2.5 300 30 1.913 ± 0.022 0.691 ± 0.035 0.069 ± 0.004
2018-04-29 19:42–22:21 2.5 300 30
2018-05-01 19:58–22:37 2.5 300 30
2018-05-04 19:56–22:35 2.5 300 30
2018-05-05 19:59–22:11 2.08 300 25
2018-05-07 19:52–22:31 2.5 300 30
2019-02-13 23:28–04:31 4.83 300 58
2019-02-14 19:12–04:38 8.67 300 104 8.518 ± 0.025 2.234 ± 0.013 0.524 ± 0.002
2019-02-15 19:31–04:53 8.67 300 104
2019-02-16 19:22–04:38 8.58 300 103 4.505 ± 0.041 1.12 ± 0.01 0.123 ± 0.001
3.19 ± 0.01 0.84 ± 0.01 0.099 ± 0.0005
3.860 ± 0.023 8.61 ± 0.01 0.126 ± 0.001
5.531 ± 0.019 1.364 ± 0.012 0.192 ± 0.0008
2019-02-17 (†) 19:23–04:18 8.33 300 100 6.628 ± 0.039 1.97 ± 0.02 0.300 ± 0.003
2.884 ± 0.019 0.669 ± 0.008 0.100 ± 0.0003
2019-02-18 20:31–04:31 7 300 84 15.479 ± 0.012 3.045 ± 0.049 0.408 ± 0.002
2019-02-23 20:35–04:22 7.08 300 85 5.939 ± 0.017 1.385 ± 0.008 0.466 ± 0.002
5.295 ± 0.032 1.235 ± 0.018 0.419 ± 0.005
2019-02-24 (†) 20:5 04:36 7.17 300 86 5.488±, 0.023 1.582 ± 0.013 0.145 ± 0.0009
11.083 ± 0.048 2.636 ± 0.043 0.292 ± 0.002
2019-02-25 20:39–02:12 5.08 300 61

Notes. The number of hours per night and the corresponding number of spectra obtained are shown in Cols. 3 and 5, respectively. Columns 6–8 correspond to the estimated energies for the flares observed in Hα, Hβ, and He I 5876. (†) indicates nights in which the value of the energy is a lower limit as only the impulsive phase or part of the gradual phase was observed.

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