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Table 2

Burst characteristics observed with RXTE/PCA, Swift/XRT, and INTEGRAL/JEM-X.

# Observatory Burst Tstart Fpers,bola Fpeakb fbc τbd k Tbb,peake
(UT) 10-9 erg cm-2 s-1 10-9 erg cm-2 s-1 10-7 erg cm-2 s  keV

1 INTEGRAL 2011-08-14 03:21:26 1.95 ± 0.15 56.0 ± 2.2 6.0 ± 0.8 10.7 ± 1.5 2.0 ± 0.5
2 RXTE 2011-08-16 15:21:45 2.05 ± 0.70 48.8 ± 1.5 4.3 ± 0.4 8.9 ± 0.8 2.69 ± 0.07
3f Swift 2011-08-18 11:23:52 2.02 ± 0.80 49.0 ± 1.9 4.0 ± 0.6 8.2 ± 1.3 1.9 ± 0.3
4 INTEGRAL 2011-08-19 03:24:26 1.95 ± 0.11 49.0 ± 2.2 4.5 ± 0.8 9.2 ± 1.7 2.0 ± 0.5
5 INTEGRAL 2011-08-19 19:59:09 1.89 ± 0.11 67.8 ± 2.2 4.7 ± 0.8 6.9 ± 1.2 2.3 ± 0.5
6g RXTE 2011-08-20 14:10:08 1.85 ± 0.20 27.0 ± 0.2 5.56 ± 0.04 20.6 ± 0.2 2.13 ± 0.01
7 INTEGRAL 2011-08-27 00:35:40 1.42 ± 0.80 61.0 ± 2.2 5.1 ± 0.8 8.4 ± 1.3 2.2 ± 0.5
8 Swift 2011-08-28 10:13:22 1.25 ± 0.10 42.0 ± 1.9 3.9 ± 0.7 9.3 ± 1.7 2.3 ± 0.3

Notes. 

(a)

Pre-burst unabsorbed flux in the 0.1–300 keV energy range.

(b)

Burst peak flux in the 0.1–40 keV energy band.

(c)

Burst fluence in the 0.1–40 keV energy band.

(d)

Effective duration τb = fb/Fpeak.

(e)

Burst peak temperature.

(f)

Burst also observed in the INTEGRAL/JEM-X data.

(g)

Burst analysis using RXTE/PCA standard two mode data with 16 s time resolution, therefore, Fpeak and kTbb,peak are more accurately interpreted as limits, owing to the low time resolution of the source data.

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