Table 1
Host galaxy sample.
GRB | RA | Dec | Redshift | Redshift | Dark?a | Observing ID | |
(J2000)b | referencec | PACS | SPIRE | ||||
|
|||||||
970828 | 18:08:31.56 | +59:18:51.2 | 0.958 | 1 | Yes | 1342258609,10 | 1342241152 |
980613 | 10:17:57.9 | +71:27:26.3 | 1.097 | 2 | No | 1342270864,65 | − |
980703 | 23:59:06.67 | +08:35:06.7 | 0.966 | 3 | No | − | 1342212419 |
990705 | 05:09:54.50 | −72:07:53.0 | 0.842 | 4 | No | 1342261814,15 | 1342214749 |
020127 | 08:15:01.42 | +36:46:33.9 | 1.9d | 5 | Yes | 1342243296,97 | 1342251906 |
020819B | 23:27:19.52 | +06:15:53.2 | 0.411 | 6 | Yes | 1342246708,09 | 1342212294 |
030115 | 11:18:32.63 | +15:02:59.9 | 2.0e | 7 | Yes | 1342247632,33 | − |
050219A | 11:05:39.07 | −40:41:04.6 | 0.2115 | 8 | Yes | 1342248286,87 | 1342247261 |
050223 | 18:05:32.99 | −62:28:18.8 | 0.584 | 9 | Yes | 1342243788,89 | 1342214756 |
051022 | 23:56:04.1 | +19:36:24.1 | 0.807 | 6 | Yes | 1342238085,86 | 1342247985 |
060904A | 15:50:54.56 | +44:59:10.5 | 2.55d | 11 | Yes | 1342261849,50 | − |
070306 | 09:52:23.3 | +10:28:55.5 | 1.496 | 12 | Yes | 1342254142,43f | − |
071021 | 22:42:34.31 | +23:43:06.5 | 2.452 | 13 | Yes | 1342246178,79 | 1342258356 |
080207 | 13:50:03.01 | +07:30:07.8 | 2.086 | 13 | Yes | 1342257547,48 | 1342261526 |
080325 | 18:31:34.3 | +36:31:24.8 | 1.78 | 14 | Yes | 1342245672,73 | 1342241156 |
090404 | 15:56:57.52 | +35:30:57.5 | 3.00d | 14 | Yes | 1342258433,34 | 1342241163 |
090417B | 13:58:46.66 | +47:01:04.4 | 0.345 | 15 | Yes | 1342257593,94 | 1342259467 |
Notes.
These GRBs are classified as dark according to the definitions by Jakobsson et al. (2004); van der Horst et al. (2009).
These are the positions of the host galaxy, which may or may not be exactly coincident with the position of the GRB afterglow.
(1) Djorgovski et al. (2001); (2) Djorgovski et al. (2003); (3) Djorgovski et al. (1998); (4) Le Floc’h et al. (2002); (5) Berger et al. (2007); (6) Levesque et al. (2010b); (7) Levan et al. (2006); (8) Rossi et al. (2014); (9) Pellizza et al. (2006); (10) Chary et al. (2007); (11) Xiao & Schaefer (2011); (12) Jaunsen et al. (2008); (13) Krühler et al. (2012); (14) Perley et al. (2013); (15) Holland et al. (2010).
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