Table 1
The 20 short bursts of our sample.
# | GRB | RA (J2000) | Dec | Inst. | Error [′′] | Ref. | T90 [s] | Ref. | E(B − V) | z | Ref. |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
|
|||||||||||
1 | 070729 | 03:45:16.02 | −39:19:20.6 | XRT | 2.5 | 1 | 0.9 ± 0.1 | 1 | 0.02 | – | – |
2 | 071112B | 17:20:51.0 | −80:53:02 | BAT | 132 | 2 | 0.3 ± 0.05 | 2 | 0.12 | – | – |
3 | 071227 | 03:52:31.26 | −55:59:03.5 | OT | 0.3 | 4 | 1.8 ± 0.4 | 3 | 0.01 | 0.381 | 39 |
4 | 080905A | 19:10:41.73 | −18:52:47.3 | OT | 0.6 | 6, 7 | 1.0 ± 0.1 | 5 | 0.14 | 0.122 | 41 |
5 | 080919 | 17:40:53.78 | −42:22:05.7 | XRT | 1.6 | 8 | 0.6 ± 0.1 | 8 | 0.49 | – | – |
6 | 081226A | 08:02:00.45 | −69:01:49.5 | OT | 0.2 | this work | 0.4 ± 0.1 | 9 | 0.16 | – | – |
7 | 081226B | 01:41:59 | −47:26:19 | IBIS | 150 | 11 | 0.7 | 11 | 0.02 | – | – |
8 | 090305 | 16:07:07.59 | −31:33:21.9 | OT | 0.2 | this work | 0.4 ± 0.1 | 14 | 0.22 | – | – |
9 | 090426 | 12:36:18.07 | +32:59:09.6 | OT | 0.5 | this work | 1.2 ± 0.3 | 17 | 0.02 | 2.609 | 32 |
10 | 090510 | 22:14:12.50 | −26:34:59.0 | OT | 0.2 | 42 | 0.3 ± 0.1 | 18 | 0.02 | 0.903 | 33, 43 |
11 | 090927 | 22:55:53.39 | −70:58:49.50 | OT | 0.2 | this work | 2.2 ± 0.4 | 19 | 0.03 | 1.37 | 34 |
12 | 091109B | 07:30:56.61 | −54:05:22.85 | OT | 0.5 | 20, 38 | 0.3 ± 0.03 | 21 | 0.03 | – | – |
13 | 091117A | 02:03:46.9 | −16:56:38 | BAT | 156 | 22, 23 | 0.43 ± 0.05 | 24 | 0.03 | – | – |
14 | 100117A | 00:45:04.66 | −01:35:41.89 | OT | 0.26 | 40 | 0.30 ± 0.05 | 25 | 0.02 | 0.915 | 40 |
15 | 100206A | 03:08:39.03 | +13:09:25.3 | XRT | 3.3 | 26 | 0.12 ± 0.03 | 26 | 0.38 | 0.41 | 35 |
16 | 100625A | 01:03:10.91 | −39:05:18.4 | XRT | 1.8 | 27 | 0.33 ± 0.03 | 27 | 0.01 | – | – |
17 | 100628A | 15:03:52.41 | −31:39:30.2 | XRT | 7.0 | 28 | 0.036 ± 0.009 | 28 | 0.17 | 0.102 | 36 |
18 | 100702A | 16:22:47.26 | −56:31:53.8 | XRT | 2.4 | 29 | 0.16 ± 0.03 | 29 | 0.41 | – | – |
19 | 101129A | 10:23:41 | −17:38:42 | BAT | 180 | 30 | 0.35 ± 0.05 | 30 | 0.07 | – | – |
20 | 101219A | 04:58:20.49 | −02:32:23.0 | XRT | 1.7 | 31 | 0.6 ± 0.2 | 32 | 0.06 | 0.718 | 37 |
Notes. Columns 5–7 give the instrument on which the coordinates are based (OT stands for optical transient detected), the corresponding radius of the error circle, and the reference, respectively. BAT and XRT stand for the instruments onboard of the Swift satellite, IBIS stands for the instrument onboard the INTEGRAL satellite. Columns 8 and 9 provide T90 and the corresponding reference. The last columns give the Galactic reddening E(B − V) (mag) along the line of sight according to Schlegel et al. (1998) as well as the redshift. If available, enhanced Swift/XRT positions are given in Cols. 3 and 4 as well as the revised error circles, taken from http://www.swift.ac.uk/xrt_positions/index.php and Evans (2011a,b).
References. 1 = Guidorzi et al. (2007c); 2 = Perri et al. (2007); 3 = Sakamoto et al. (2007b); 4 = D’Avanzo et al. (2008); 5 = Pagani et al. (2008b); 6 = Malesani et al. (2008); 7 = de Ugarte Postigo et al. (2008); 8 = Preger et al. (2008b); 9 = Krimm et al. (2008); 11 = Mereghetti et al. (2008); 14 = Krimm et al. (2009); 17 = Sato et al. (2009); 18 = Hoversten et al. (2009); 19 = Grupe et al. (2009b); 20 = Levan et al. (2009b); 21 = Oates et al. (2009b); 22 = Cummings et al. (2009); 23 = D’Elia et al. (2009); 24 = Sakamoto et al. (2009); 25 = de Pasquale et al. (2010c); 26 = Krimm et al. (2010c); 27 = Holland et al. (2010b); 28 = Immler et al. (2010); 29 = Siegel et al. (2010b); 30 = Cummings et al. (2010); 31 = Gelbord et al. (2010); 32 = Krimm et al. (2010a); 32 = Levesque et al. (2009); 33 = Rau et al. (2009); 34 = Levan et al. (2009a); 35 = Cenko et al. (2010a); 36 = Cenko et al. (2010b); 37 = Chornock & Berger (2011); 38 = Malesani et al. (2009); 39 = D’Avanzo et al. (2009); 40 = Fong et al. (2011); 41 = Rowlinson et al. (2010); 42 = Nicuesa Guelbenzu et al. (2012); 43 = McBreen et al. (2010).
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