Table 1
Flare properties and their host candidates.
| GWGC name | D L | MJD | Duration | Peak flux | Significance | Counterpart |
| [Mpc] | [days] | [10-10 erg s-1 cm-2] | ||||
|
|
||||||
| Galactic objects | ||||||
| Terzan 5 | 0.001 | 55 483 | 72 | 13.27 | 45.4 | IGR J17480-2446 |
| Liller 1 | 0.001 | 55 812 | 86 | 2.46 | 13.3 | MXB 1730-335 |
| NGC 6388 | 0.001 | 55 771 | 96 | 3.23 | 12.7 | |
| NGC 6293 | 0.001 | 54 583 | 93 | 3.52 | 12.1 | RX J1709.5-2639 |
| PGC 3079807 | 65.2 | 54 798 | 132 | 25.37 | 29.9 | Sw J1539.2-6227 |
| PGC 016029 | 57.3 | 55 240 | 95 | 5.30 | 17.0 | KT Eri |
|
|
||||||
| Gamma-ray bursts | ||||||
| NGC 3835 | 34.1 | 53 833 | 47 | 1.95 | 17.1 | GRB 060319 |
| SDSS J114153.19+510158.7 | 97.5 | 55 125 | 50 | 3.68 | 14.9 | GRB 091020A |
| ESO 542-022 | 76.0 | 55 471 | 55 | 2.91 | 13.3 | GRB 100814A |
|
|
||||||
| Relativistic TDE | ||||||
| NGC 6213 | 78.6 | 55 745 | 121 | 1.92 | 15.2 | Sw J1644+5734 |
|
|
||||||
| TDE candidates | ||||||
| UGC 01791 | 67.2 | 53 429 | 82 | 5.62 | 13.7 | |
| PGC 015259 | 59.1 | 55 238 | 60 | 3.71 | 10.4 | |
| NGC 6021 | 67.0 | 53 405 | 71 | 3.31 | 10.1 | |
| UGC 03317 | 20.8 | 55 469 | 61 | 4.89 | 9.8 | |
| PGC 170392 | 69.3 | 53 730 | 69 | 4.87 | 10.6 | |
| PGC 1185375 | 22.9 | 55 258 | 41 | 6.69 | 19.8 | |
| PGC 133344 | 97.1 | 53 480 | 65 | 3.08 | 11.7 | |
| PGC 1190358 | 33.0 | 55 264 | 108 | 4.57 | 10.4 | |
| PGC 1127938 | 76.8 | 54 116 | 60 | 3.57 | 10.2 | |
|
|
||||||
| Dubious cases | ||||||
| NGC 1367 | 17.3 | 53 737 | 82 | 3.99 | 11.5 | SN 2005ke |
| PGC 053636 | 26.1 | 53 930 | 81 | 2.29 | 10.4 | |
| SDSS J114553.33+635411.6 | 58.0 | 53 828 | 70 | 1.54 | 11.1 | |
| NGC 6206 | 72.5 | 55 750 | 71 | 3.22 | 13.4 | |
| ESO 161-001 | 29.1 | 54 073 | 90 | 2.49 | 11.3 | |
| PGC 2464645 | 31.2 | 55 846 | 92 | 2.70 | 12.9 | |
| PGC 3241255 | 95.7 | 55 214 | 65 | 2.81 | 9.9 | |
Notes. The flare’s properties (peak epoch, duration, peak flux, significance) were measured at the centre of the PSF fit, while the distance refers to the host itself and are taken from White et al. (2011). In the final column we list the most likely counterpart of the flare. The order of the table is as in Sect. 3.
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