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Table 2

Log of observations of the 2010-2011 outbursts used in this paper.

IDa OBS IDb Exp. Start Stop log 10(Flux)c Fluxc LXd
ks MJD MJD  × 10-9  × 1035

95418-01-01-00 3.1 55 292.3306 55 292.3778 –8.2412 ± 0.0007 5.738 74.766
A 95418-01-02-00 3.3 55 298.2106 55 298.2554 –8.4228 ± 0.0008 3.778 49.222
00031690001 4.8 55 299.8793 55 300.0424
95418-01-02-01 3.2 55 301.2178 55 301.2611 –8.7541 ± 0.0013 1.762 22.954

95418-01-03-01 1.0 55 447.0197 55 447.0311 –8.738 ± 0.002 1.827 23.804
S IBIS 56 55 441.2576 55 448.1785
JEM-X 64 55 441.2576 55 448.1785 –8.78 ± 0.01 1.66 21.6
00031690003 5.7 55 443.0294 55 443.2021
95418-01-03-00 2.8 55 447.9302 55 447.9728 –8.894 ± 0.002 1.275 16.615
95418-01-04-00 2.5 55 449.0456 55 449.0763 –9.021 ± 0.003 0.953 12.417
95418-01-04-01 1.5 55 450.2285 55 450.2463 –9.316 ± 0.006 0.483 6.296
95418-01-04-02 1.1 55 451.7385 55 451.7563 –10.37 ± 0.06 0.042 0.55 2
95418-01-04-03 1.0 55 452.9830 55 452.9963 –10.47 ± 0.07 0.034 0.444

96364-01-01-00 1.3 55 594.1491 55 594.1680 –8.937 ± 0.003 1.155  15.051
1 96364-01-01-01 1.5 55 595.6400 55 595.6574 –9.120 ± 0.004 0.759 9.888
00031690005e 0.99 55 595.6759 55 595.6875
2 96364-01-02-00 3.2 55 596.4802 55 596.5271 –9.526 ± 0.006 0.298 3.882
00031690005e 1.46 55 596.5314 55 596.5484
3 00031690006e 0.86 55 597.4755  55 597.4855
96364-01-03-00 3.0 55 597.4921 55 597.5728 –10.33 ± 0.03 0.046 0.604
00031690006e 1.08 55 597.5394 55 597.5520
96364-01-04-00 3.2 55 598.4385 55 598.4848 –10.38 ± 0.02 0.042 0.547
96364-01-05-00 2.9 55 599.4872 55 599.5304 –10.41 ± 0.04 0.039 0.504
4 96364-01-06-00 2.8 55 600.5345 55 600.5763 –9.362 ± 0.004 0.434 5.659
00031690009 1.62 55 600.5450 55 600.5638
96364-01-07-00 3.3 55 601.3754 55 601.4217 –10.40 ± 0.05 0.040 0.515
96364-01-08-00 3.3 55 602.3547 55 602.4000 –10.40 ± 0.04 0.040 0.517
96364-01-09-00 3.0 55 603.4719 55 603.5132 –10.54 ± 0.03 0.029 0.376
96364-01-10-00 3.2 55 604.3171 55 604.3582 –10.63 ± 0.06 0.023 0.304
96364-01-11-00 3.1 55 605.4297 55 605.4710 –10.63 ± 0.03 0.023 0.302

Notes. The three vertical blocks separated by a horizontal line refer from top to bottom to April 2010, September 2010, and February 2011, respectively.

(a)

ID is the conventional name used in our broad-band spectral analysis exploiting quasi-simultaneous observations.

(b)

OBS IDs as 9xxxx-01-xx-xx refer to RXTE, 0003169000x to Swift, IBIS and JEM-X to the INTEGRAL monitoring.

(c)

2–30 keV absorbed flux is in units of erg cm-2 s-1, not reported for instruments operating in different bands.

(d)

2–30 keV luminosity in erg/s assuming a distance of 3.3 kpc.

(e)

Different snapshots with the same OBS ID.

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