Table 1
Stellar hosts and times of arrival for the 21 detected stellar bursts.
| Burst ID | Obs. ID | Source Namea | Spectral type | X-ray luminosityb (erg s−1) | Distance (pc) | Time of arrivalc (MJD) |
|---|---|---|---|---|---|---|
| B01 | L695587 | LP 192-44 | M6Vg | <9.52 × 1028 | 53.30 | 58534.67984606 |
| B02d | L800676 | G 250-25 | M3.5Vh | (1.58 ± 0.52) × 1029 | 30.03 | 59188.19808440 |
| B03 | L798434 | PM J07349+1445 | M3Vh | (4.64 ± 0.60) × 1029 | 16.30 | 59175.18451620 |
| B04d | L664734 | PM J09190+4610 | M3.5Vi | (1.32 ± 0.27) × 1029 | 30.03 | 58351.72629861 |
| B05 | L727610 | G 236-2 | M3.5Vh | (1.09 ± 0.13) × 1028 | 11.86 | 58668.82176042 |
| B06 | L665242 | LP 261-57 | M4Vi | <3.11 × 1029 | 81.82 | 58362.39292940 |
| B07 | L728721 | AD Leo | M3Vh | (1.95 ± 0.09) × 1029 | 4.97 | 58677.81698611 |
| B08 | L258201 | G 123-35 | M3.5Vh | (1.65 ± 0.21) × 1029 | 23.51 | 57044.53220486 |
| B09 | L612032 | LSPM J1228+6515 | M3.5Vi | <1.34 × 1029 | 71.57 | 58023.74614583 |
| B10d,e | L400133 | 2MASS J14333139+3417472 | M5Vi | <1.12 × 1029 | 48.21 | 57305.49466319 |
| B11d,e | L603984 | G 223-74 | M3Vh | (6.61 ± 0.73) × 1028 | 18.46 | 57982.14790972 |
| B12d,e | L259433 | i Boo | G9/F5Vj | (1.84 ± 0.03) × 1030 | 12.95 | 57058.28746528 |
| B13 | L763737 | LP 443-17 | M5Vh | <1.38 × 1028 | 17.10 | 58845.44449653 |
| B14d | L746965 | BD+19 5116B | M4Vh | (2.90 ± 0.09) × 1029 | 6.25 | 58753.94009722 |
| B15 | L719904 | HD 147379B | M3Vh | (2.76 ± 0.29) × 1028 | 10.76 | 58636.10437963 |
| B16d | L652062 | G 240-45A | M4Vh | <8.61 × 1027 | 27.49 | 58240.94514236 |
| B17d | L857710 | BD+68 946 | M3Vh | (5.35 ± 0.30) × 1027 | 4.55 | 59687.44707176 |
| B18 | L694975 | HD 239960A | M3Vh | (6.02 ± 0.54) × 1027 | 4.01 | 58521.61115394 |
| B19 | L696951 | EV Lac | M4Vh | (1.13 ± 0.03) × 1029 | 5.05 | 58550.55276620 |
| B20d,f | L470106 | StKM 1-1262 | M0Vf | (3.80 ± 0.32) × 1029 | 40.88 | 57525.92432407 |
| B21 | L695755 | LP 215-56 | M2.4Vh | <5.59 × 1029 | 62.13 | 58552.21916088 |
Notes. aSee https://simbad.cds.unistra.fr/guide/otypes.htx bX-ray catalogue flux values are taken from Dwelly et al. (2017) when available (0.1–2.4 keV for ROSAT, 0.2–12 keV for XMMSL); otherwise, detections or upper limits were derived using the XMM Upper Limit Server4 for the ROSAT mission (0.2–2 keV), assuming a power law model Γ = 2, and NH = 1020 cm−2. cUncertainties of ~4 seconds. dThese bursts are presented in detail by Tasse et al. (2025). eThese bursts are presented in detail by Callingham et al. (2023). fThis burst is presented in detail by Callingham et al. (2025). gSpectral types based on effective temperature hSpectral types adopted from Wenger et al. (2000). iSpectral types adopted from Cook et al. (2016). jBinary system, unknown which star is the host.
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