Table 3.
General properties of sources and data coverage of fluctuating bursts (literature bursts below the dividing line).
| Burst | Object | Ultracompact? | NH/1022 | P/T | Date | Instrument | Data coverage (s) |
|---|---|---|---|---|---|---|---|
| 1 | IGR J17062–6143 | Confirmed[3, 4, 13] | 0.12[17] | P[4] | 2012-06-25 | Swift/BAT+XRT | −89/+1321 |
| 2 | SAX J1712.6–3739 | Candidate[1],[5] | 1.54[6] | P[1] | 2011-09-26 | Swift/BAT+XRT | −119/+924a |
| 3 | SAX J1712.6–3739 | “ | “ | “ | 2014-08-18 | Swift/BAT+XRT | 0/+5200 |
| 4 | Swift J1734.5–3027 | Possibly | 0.57 | T[2] | 2013-09-01 | Swift/BAT+XRT | −215/+1691b |
| 5 | 4U 1850–087 | Confirmed[1] | 0.48[9] | P[1] | 2014-03-10 | Swift/BAT+XRT | −39/+1444 |
| 6 | 2S 0918–549 | Semi-confirmed[10] | 0.35[9] | P[1] | 1996-10-01 | BeppoSAX/WFC | −13/+1002 |
| 7 | 2S 0918–549 | “ | “ | 2008-02-08 | RXTE/PCA | −768/+315 | |
| 8 | A 1246–58 | Candidate[1] | 0.50[8] | P[1] | 1996-07-22 | BeppoSAX/WFC | −31/+199 |
| 9 | SLX 1735–269 | Candidate[1] | 1.50[7] | P[1] | 2003-09-15 | INTEGRAL/JEM-X | −1200/+2235 |
| 10 | GRS 1741.9–2853 | Probably not[11, 14] | 11.4[11, 14] | T | 2013-08-03 | NuSTAR | < − 100/+800 |
| 11 | 4U 1820–30 | Confirmed[15] | 0.16 | P | 1999-09-09 | RXTE/PCA | −152/+9200 |
| 12 | M15 X-2 | Confirmed[16] | 0.07[12] | P | 1988-10-20 | Ginga/LAC | < − 100/+160 |
Notes. All times are in seconds after the start of the burst, unless noted otherwise. (a)This data coverage is continuous. The rest of the XRT data beyond 5713 s are short intervals with count rates below 9.5 c s−1; (b)this data coverage is continuous. The rest of the XRT data beyond 5007 s are short intervals with count rates below 30 c s−1.
References. [1]: in ’t Zand et al. (2007), [2]: Bozzo et al. (2015), [3]: Keek et al. (2017), Hernandez Santisteban et al. (2018), [4]: Degenaar et al. (2013, 2017), [5]: Wiersema et al. (2009), [6]: Fiocchi et al. (2008b), [7]: David et al. (1997), [8]: in ’t Zand et al. (2008), [9]: Sidoli et al. (2005), [10]: Zhong & Wang (2011), [11]: Barrière et al. (2015), [12]: van Paradijs et al. (1990), [13]: Strohmayer et al. (2018), [14]: Trap et al. (2009), [15]: Stella et al. (1987), [16]: Dieball et al. (2005), and [17]: van den Eijnden et al. (2018).
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