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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.

(a)

These GRBs are classified as dark according to the definitions by Jakobsson et al. (2004); van der Horst et al. (2009).

(b)

These are the positions of the host galaxy, which may or may not be exactly coincident with the position of the GRB afterglow.

(d)

Photometric redshift.

(e)

Photometric redshift determined by our grasil fits.

(f)

Although this source was in our target list, this observation was acquired in the OT2 proposal, OT2_ppschady_2.

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