Table 2
Details of the Herschel observations.
| OD | Target | Instrument | Duration | Start date and time | ObsId | Field size |
| (s) | (UT) | (arcmin) | ||||
|
|
||||||
| 395 | NGC 4013 | SPIRE | 349 | 2010-06-12 16:29:39 | 1342198241 | 8 × 8 |
| 467 | NGC 5907 | SPIRE | 770 | 2010-08-24 00:47:30 | 1342203599 | 16 × 16 |
| 500 | UGC 4277 | SPIRE | 349 | 2010-09-26 16:16:14 | 1342205086 | 8 × 8 |
| 558 | NGC 4217 | SPIRE | 541 | 2010-11-22 21:56:09 | 1342210500 | 11 × 11 |
| 558 | IC 2531 | SPIRE | 529 | 2010-11-23 05:49:48 | 1342210524 | 10 × 10 |
| 572 | NGC 5529 | SPIRE | 529 | 2010-12-07 11:06:03 | 1342210882 | 10 × 10 |
| 715 | NGC 5907 | PACS | 2124 | 2011-04-29 13:57:35 | 1342220804 | 16 × 16 |
| 715 | NGC 5907 | PACS | 2124 | 2011-04-29 14:34:02 | 1342220805 | 16 × 16 |
| 723 | NGC 4217 | PACS | 1217 | 2011-05-07 11:07:33 | 1342220109 | 11 × 11 |
| 723 | NGC 4217 | PACS | 1217 | 2011-05-07 11:28:53 | 1342220110 | 11 × 11 |
| 723 | UGC 4277 | PACS | 813 | 2011-05-07 12:43:07 | 1342220119 | 8 × 8 |
| 723 | UGC 4277 | PACS | 813 | 2011-05-07 12:57:43 | 1342220120 | 8 × 8 |
| 731 | NGC 4013 | PACS | 813 | 2011-05-15 12:13:15 | 1342220968 | 8 × 8 |
| 731 | NGC 4013 | PACS | 813 | 2011-05-15 12:27:51 | 1342220969 | 8 × 8 |
| 733 | IC 2531 | PACS | 909 | 2011-05-17 05:29:37 | 1342221271 | 10 × 10 |
| 733 | IC 2531 | PACS | 909 | 2011-05-17 05:45:49 | 1342221272 | 10 × 10 |
| 758 | NGC 5529 | PACS | 909 | 2011-06-11 17:40:01 | 1342222509 | 10 × 10 |
| 758 | NGC 5529 | PACS | 909 | 2011-06-11 17:56:13 | 1342222510 | 10 × 10 |
| 787 | NGC 973 | PACS | 813 | 2011-07-10 10:55:12 | 1342223868 | 8 × 8 |
| 787 | NGC 973 | PACS | 813 | 2011-07-10 11:09:48 | 1342223869 | 8 × 8 |
| 828 | NGC 973 | SPIRE | 349 | 2011-08-20 10:49:43 | 1342226629 | 8 × 8 |
Notes. OD indicates the operational day of the Herschel Space Observatory, ObsId is the observation identification number. The PACS observations always consist of two concatenated observing blocks, one for the nominal and the other for the orthogonal scan directions. The indicated duration of the observations includes both on-source integration time and instrument and observation overheads.
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