Table 3.
Most significant intra-day flare from AGL J1736−3250 in the 100 MeV−10 GeV energy range during each of the 1-day flaring episodes reported in Table 2.
| 1-day flare | Most significant intra-day flare | ||||||
|---|---|---|---|---|---|---|---|
| Flare | Counts | Integration time | Duration |  |
Counts | Photon Flux | Luminosity |
| ID | ph | MJD | h | ph | [10−6 ph s−1 cm−2] | [1037 erg s−1] | |
| E01 | 33 ± 12 | 54343.000–54343.083 | 2 | 3.5 | 11 ± 5 | 10.09 ± 4.36 | 3.78 ± 1.63 |
| E02 | 31 ± 12 | 54732.250–54732.500 | 6 | 3.1 | 19 ± 8 | 2.96 ± 1.25 | 1.11 ± 0.47 |
| E03 | 28 ± 11 | 54746.416–54746.500 | 2 | 3.3 | 11 ± 5 | 6.46 ± 3.03 | 2.42 ± 1.13 |
| E04 | 44 ± 13 | 54915.333–54915.416 | 2 | 3.5 | 8 ± 4 | 7.55 ± 3.71 | 2.83 ± 1.39 |
| E05 | 62 ± 14 | 54935.666–54936.750 | 2 | 4.1 | 15 ± 6 | 6.89 ± 2.66 | 2.58 ± 1.00 |
| E06 | 26 ± 10 | – | |||||
| E07 | 27 ± 10 | 55109.000–55109.166 | 4 | 4.3 | 19 ± 7 | 5.04 ± 1.79 | 1.89 ± 0.67 |
| E08 | 37 ± 13 | 55112.583–55112.666 | 2 | 3.6 | 12 ± 5 | 6.64 ± 2.76 | 2.48 ± 1.03 |
| E09 | 14 ± 6 | 55599.000–55599.083 | 2 | 3.9 | 7 ± 4 | 13.14 ± 6.80 | 4.92 ± 2.54 |
| E10 | 15 ± 7 | 56182.000–56183.250 | 6 | 3.5 | 7 ± 4 | 4.57 ± 2.35 | 1.71 ± 0.88 |
| E11 | 18 ± 7 | – | |||||
| E12 | 12 ± 6 | 56351.500–56351.666 | 4 | 3.3 | 7 ± 4 | 7.37 ± 3.87 | 2.76 ± 1.45 |
| E13 | 21 ± 7 | 57786.000–57786.250 | 6 | 3.2 | 8 ± 4 | 7.57 ± 3.84 | 2.83 ± 1.44 |
| E14 | 27 ± 9 | – | |||||
| E15 | 19 ± 8 | 58199.333–58199.500 | 4 | 3.9 | 11 ± 5 | 10.69 ± 4.69 | 4.00 ± 1.76 |
| E16 | 16 ± 7 | 58368.000–58368.166 | 4 | 3.6 | 8 ± 4 | 9.98 ± 4.83 | 3.73 ± 1.81 |
| E17 | 21 ± 8 | 58744.000–58744.250 | 6 | 4.0 | 12 ± 5 | 8.45 ± 3.52 | 3.16 ± 1.32 |
| E18 | 16 ± 7 | – | |||||
| E19 | 14 ± 6 | 59806.250–59806.500 | 6 | 3.3 | 7 ± 4 | 6.18 ± 3.30 | 2.31 ± 1.23 |
Notes. Column (1) provides the flare ID, (2) the excess counts associated with AGL J1736−3250 in Table 2. The other columns are relative to the intra-day flare and provide: (3) integration range in MJD; (4) integration time in hours; (5) statistical significance expressed in 
of the detection according to the maximum likelihood ratio test; (6) number of excess counts and 1σ statistical error associated with AGL J1736−3250; (7) the average photon flux and its 1σ statistical error, evaluated assuming a power-law spectrum with index 2.1; and (8) the corresponding luminosity assuming a distance of 4.1 kpc. The horizontal line separates the ‘pointing’ and the ‘spinning’ mode periods.
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