Investigating the off-axis GRB afterglow scenario for extragalactic fast X-ray transients

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Volume 690 (October 2024)

A&A, 690 (2024) A101

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Table B.2.

Final Sample of 13 merger-induced GRBs analysed in this work.

GRB	z	Γ_X	T₉₀ (EE) (s)	References	References optical data
050709	0.160 ± 0.001	2.24±0.35^†	0.07±0.01 (130±7)	[1], [2]	[1], [24], [25], [26], [27], [28], [29]
050724	0.2582 ± 0.0003	1.80 $_{- 0.04}^{+ 0.05}$ $^{+0.05}_{-0.04}$	3.0±0.1 (152.4±9.2)	[3], [4]	[3], [4], [29], [30]
051227	1 assumed	1.85 $_{- 0.09}^{+ 0.12}$ $^{+0.12}_{-0.09}$	8.0±0.2 (∼100)	[5], [6]	[5], [31], [32], [33], [34],
					[35], [36], [37], [38]
061006	0.436 ± 0.002	2.03 $_{- 0.08}^{+ 0.11}$ $^{+0.11}_{-0.08}$	∼0.5 (130±10)	[5], [7]	[5], [29], [37], [39], [40], [41]
061201	0.111 uncertain	1.87 $_{- 0.14}^{+ 0.19}$ $^{+0.19}_{-0.14}$	0.8±0.1	[8]	[8], [42], [43], [44]
070714B	0.9225 ± 0.0001	1.66 $_{- 0.08}^{+ 0.11}$ $^{+0.11}_{-0.08}$	∼3 (∼100)	[9], [10]	[45], [46], [47], [48], [49], [50]
070724A	0.457 ± 0.0007	1.78 $_{- 0.10}^{+ 0.13}$ $^{+0.13}_{-0.10}$	0.4±0.04	[11]	[11], [29], [51], [52], [53]
071227	0.381	1.64 $_{- 0.11}^{+ 0.14}$ $^{+0.14}_{-0.11}$	1.8±0.4 (≳300)	[5], [12]	[5], [29], [54], [55], [56], [57], [58], [59]
090510	0.903 ± 0.001	2.05 $_{- 0.09}^{+ 0.12}$ $^{+0.12}_{-0.09}$	0.3±0.1 (∼100)	[13], [14], [15]	[29], [59], [60], [61], [62]
110112A	0.5 assumed	2.04 $_{- 0.07}^{+ 0.09}$ $^{+0.09}_{-0.07}$	0.5±0.1	[16], [17]	[63], [64], [65], [66], [67], [68]
111020A	0.5 assumed	1.70 $_{- 0.07}^{+ 0.10}$ $^{+0.10}_{-0.07}$	0.40±0.09	[18], [19]
111117A	2.211 ± 0.001	1.63 $_{- 0.07}^{+ 0.09}$ $^{+0.09}_{-0.07}$	0.47±0.09	[20], [21]
160821B	0.1619 ± 0.0002	1.88±0.24^††	0.48±0.07	[22], [23]	[69], [70], [71], [72], [73]

Notes. Columns: (1) name of GRB, (2) redshift, (3) X-ray photon index (averaged over times when detections were included in the fitting), (4) duration T₉₀ over which central 90% of the total observed 15–150 keV photon counts are detected (in parentheses: duration including the duration of the extended emission (EE) if T₉₀> 2s; see Kann et al. 2011), (5) references for columns (2)–(4), (6) references for the optical data.

^† Photon index taken from Fox et al. 2005.

^†† Photon index taken from Troja et al. 2019.

References: [1] Fox et al. 2005, [2] Nysewander et al. 2009, [3] Malesani et al. 2007, [4] Berger et al. 2005, [5] D’Avanzo et al. 2009, [6] Hullinger et al. 2005, [7] Krimm et al. 2006, [8] Stratta et al. 2007, [9] Gao et al. 2017, [10] Barbier et al. 2007, [11] Kocevski et al. 2010, [12] Sato et al. 2007, [13] McBreen et al. 2010, [14] Ackermann et al. 2010, [15] Grupe & Hoversten 2009, [16] Fong et al. 2013, [17] Barthelmy et al. 2011, [18] Fong et al. 2012, [19] Sakamoto et al. 2011a, [20] Selsing et al. 2018, [21] Sakamoto et al. 2011b, [22] Fong et al. 2022, [23] Palmer et al. 2016, [24] Hjorth et al. 2005, [25] Covino et al. 2006, [26] Morgan et al. 2005, [27] Haislip et al. 2005, [28] Monard 2005, [29] Leibler & Berger 2010, [30] Gorosabel et al. 2006, [31] Roming et al. 2005, [32] Kodaka et al. 2006, [33] Yanagisawa et al. 2005, [34] Cenko et al. 2005, [35] Garimella et al. 2005, [36] Sonoda et al. 2005, [37] Berger et al. 2007a, [38] Halpern & Tyagi 2005, [39] Schady et al. 2006, [40] Mundell et al. 2006, [41] Fong et al. 2009, [42] Holland & Marshall 2006, [43] Marshall et al. 2006, [44] Berger 2010, [45] Landsman et al. 2007, [46] Weaver et al. 2007, [47] Melandri et al. 2008, [48] Graham et al. 2009, [49] Perley et al. 2007, [50] Kann et al. 2011, [51] Ziaeepour et al. 2007, [52] Berger et al. 2009, [53] Cenko et al. 2007, [54] Cucchiara & Sakamoto 2007 , [55] Sakamoto et al. 2007, [56] Eyles et al. 2019, [57] Berger et al. 2007b, [58] D’Avanzo et al. 2007, [59] Nicuesa Guelbenzu et al. 2012a, [60] Pasquale et al. 2010, [61] Olofsson et al. 2009, [62] McBreen et al. 2010, [63] Breeveld & Stamatikos 2011, [64] Gorbovskoy et al. 2011, [65] Xin et al. 2011, [66] Nakajima et al. 2011, [67] Grankin et al. 2011, [68] Fong et al. 2013, [69] Breeveld & Siegel 2016, [70] Troja et al. 2019, [71] Rebolo et al. 2016, [72] Lamb et al. 2019, [73] Jin et al. 2018.

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