Table 2.
Outburst properties.
| Source | # of | Year | Duration | Bolometric peak flux | References | References |
|---|---|---|---|---|---|---|
| outbursts | (days) | (×10−8 erg cm−2 s−1) | Light curves | Spectral parameters | ||
| IGR J18245-2452 | 1 | 2014 | 23 | 1.15 | [4] | [4] |
| Swift J1749.4–2807 | 1 | 2010 | 11 | 1.52 | [9] | [9] |
| IGR J17591–2342 | 1 | 2018 | 50 | 1.50 | [b] | [32] |
| SAX J1748.9–2021 | 6 | 1998, 2001, 2005, 2010 | 10, 53, 52, 53 | 0.65, 1.30, 2.10, 4.20, | [1], [1], [1], [m], | [1], [1], [1], [25], |
| 2015, 2017 | 58, 13 | 2.09, 1.73, 0.10 | [m], [30] | [27], [28] | ||
| XTE J1814–338 | 1 | 2003 | 53 | 0.88 | [11] | ( * ) |
| IGR J17498–2921 | 1 | 2011 | 37 | 2.00 | [8] | [8] |
| IGR J17511–3057 | 2 | 2010, 2015 | 30, 25 | 0.40, 0.44 | [20], [23] | [20], [23] |
| IGR J00291+5934 | 4 | 2004, 2008, 2008, 2015 | 14, 9, 15, 25 | 0.29, 0.15, 0.11, 0.35 | [5] (all) | [5] (all) |
| SAX J1808.4–3658 | 7 | 1998, 2000, 2002, 2005 | 15, 14, 42, 28, | 0.72, 0.12, 0.92, 0.63, | [11], [11], [11], [11], | [12], [38], [18], [10], |
| 2008, 2011, 2015 | 21, 16, 25 | 3.31, 2.24, 0.94 | [3], [m], [19] | [3], [21], [6], [17] | ||
| IGR J1737.9-3747 | 3 | 2004, 2008, 2018 | 50, 15, 10 | 0.330, 0.690, 0.014 | [18], [18], [b] | [10], [10], [33] |
| HETE J1900.1–2455 | 1 | 2005 | 3784 | 2.40 | [36] | [22] |
| NGC 6440 X–2 | 10 | 2009, 2009, 2010, 2010, | 3 (all) | 0.088, 0.35, 0.053, 0.088 | [15] (all) | [13], [26] |
| 2010, 2010, 2011, 2011, | 0.035, 0.079, 0.079, 0.026, | |||||
| 2011, 2011 | 0.079, 0.026 | |||||
| Swift J1756.9–2508 | 3 | 2007, 2009, 2018 | 7, 15, 7 | 0.20, 0.26, 0.10 | [15], [a], [2] | [16], [24], [34] |
| IGR J16597–3704 | 1 | 2018 | 17 | 1.80 | [b] | [35] |
| MAXI J0911–655 | 1 | 2016 ( † ) | 910 | 0.13 | [31],[x] | [31] |
| XTE J1751–305 | 4 | 2002, 2005, 2007, 2009 | 7, 3, 3, 3 | 0.81, 0.11, 0.14, 0.22 | [29] (all) | [29] (all) |
| XTE J1807–294 | 1 | 2004 | 100 | 0.49 | [7] | [7] |
| IGR J17062-6143 | 1 | 2006 ( † ) | 4380 | 0.025 | [37] | [14] |
Notes. List of the AMXPs discovered so far and their main properties. The bolometric peak flux is the unabsorbed flux in the range 0.1–300 keV and an intrinsic standard 10% error was attributed to each value. The unpublished light curves were extracted from the public archives of: [a] = All Sky Monitor (ASM) on board RXTE, [b] = BAT on board Swift, [m] = MAXI and [x] = XRT onboard Swift. The references are divided into refereed publications where the light curve of the relative outburst is displayed and publications where the spectral parameters of the source during the outburst were reported. ( † ) indicates that the outburst is still ongoing at the time of writing. ( * ) This work.
References. [1] = Altamirano et al. (2008), [2] = Bult et al. (2018), [3] = Cackett et al. (2009) [4] = De Falco et al. (2017b), [5] = De Falco et al. (2017a), [6] = Di Salvo et al. (2019), [7] = Falanga et al. (2005), [8] = Falanga et al. (2012), [9] = Ferrigno et al. (2011), [10] = Galloway et al. (2005b) [11] = Hartman et al. (2008), [12] = Heindl & Smith (1998), [13] = Heinke et al. (2010), [14] = Keek et al. (2017), [15] = Krimm et al. (2007), [16] = Linares et al. (2008), [17] = Markwardt et al. (2002a), [18] = Markwardt et al. (2008), [19] = Papitto et al. (2007), [20] = Papitto et al. (2010), [21] = Papitto et al. (2011b), [22] = Papitto et al. (2013b), [23] = Papitto et al. (2016), [24] = Patruno et al. (2009), [25] = Patruno et al. (2010), [26] = Patruno & D’Angelo (2013), [27] = Pintore et al. (2016) [28] = Pintore et al. (2018), [29] = Riggio et al. (2011), [30] = Sanna et al. (2016), [31] = Sanna et al. (2017a), [32] = Sanna et al. (2018a), [33] = Sanna et al. (2018c), [34] = Sanna et al. (2018d), [35] = Sanna et al. (2018b), [36] = Šimon (2018), [37] = Strohmayer et al. (2018b), [38] = Wijnands (2003).
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