Table 1.
Observed Wide pointings.
| Field | RA | Dec | APA | Obs. date |
|---|---|---|---|---|
| (J2000) | (J2000) | (deg) | ||
| GOODS-N (PID 1211) | ||||
| 00 | 12:36:16 | 62:13:05 | 318.70 | 2023-03-26 |
| 01 | 12:36:38 | 62:16:28 | 322.76 | 2023-03-25 |
| 02 | 12:36:39 | 62:08:23 | 322.57 | 2023-03-25 |
| 03 | 12:37:06 | 62:20:20 | 322.90 | 2023-03-28 |
| 04 | 12:37:20 | 62:13:22 | 322.77 | 2024-03-24 ( * ) |
| 05 | 12:37:22 | 62:16:07 | 31.21 | 2024-01-30 ( * ) |
| 06 | 12:37:47 | 62:17:08 | 322.94 | 2023-03-26 |
| 07 | 12:36:53 | 62:16:40 | 322.79 | 2023-03-26 |
| 08 | 12:37:30 | 62:18:38 | 322.96 | 2023-03-26 |
| GOODS-S (PID 1212) | ||||
| 09 | 03:32:16 | −27:48:02 | 89.52 | 2023-10-14 |
| 10 | 03:32:36 | −27:42:02 | 88.52 | 2023-10-14 |
| 11 | 03:32:12 | −27:43:59 | 89.49 | 2023-10-08 |
| 12 | 03:32:18 | −27:51:30 | 202.74 | 2024-01-27 ( * ) |
| 13 | 03:32:33 | −27:50:15 | 89.56 | 2023-10-12 |
| 14 | 03:32:28 | −27:54:09 | 89.52 | 2023-10-13 |
| 15 | 03:32:42 | −27:53:14 | 89.55 | 2023-10-14 |
| AEGIS (PID 1213) | ||||
| 17 | 14:20:38 | 53:03:42 | 17.34 | 2023-03-08 |
| 18 | 14:20:20 | 52:59:16 | 17.24 | 2023-03-08 |
| 19 | 14:19:55 | 52:55:49 | 17.11 | 2023-03-09 |
| 20 | 14:19:31 | 52:50:09 | 17.01 | 2023-03-09 |
| 21 | 14:19:11 | 52:48:00 | 268.75 | 2023-06-28 ( * ) |
| COSMOS (PID 1214) | ||||
| 23 | 10:00:40 | 02:27:39 | 71.56 | 2023-12-02 |
| 24 | 10:00:24 | 02:22:38 | 71.55 | 2023-12-08 |
| 25 | 10:00:40 | 02:20:36 | 71.56 | 2023-12-09 |
| 27 | 10:00:36 | 02:14:22 | 71.56 | 2024-01-06 |
| 28 | 10:00:26 | 02:13:53 | 71.55 | 2023-12-03 |
| UDS (PID 1215) | ||||
| 29 | 02:18:12 | −05:10:55 | 32.47 | 2023-07-23 |
| 30 | 02:17:48 | −05:10:08 | 32.45 | 2023-08-19 |
| 31 | 02:17:48 | −05:15:29 | 32.43 | 2023-08-19 |
| 32 | 02:17:26 | −05:09:59 | 32.43 | 2023-08-19 |
| 33 | 02:17:06 | −05:14:06 | 32.41 | 2023-08-20 |
Notes. APA refers to the aperture position angle (in degrees), i.e. the angle that the rectangular microshutters make as projected onto the sky, not the “V3PA” of the instrument itself. Fields 16, 22, and 26 were initially planned but never observed and are omitted from this table. ( * )Observation was repeated as original exposures were affected by either a telescope guide star acquisition error or a bright short in the MSA control electronics.
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