Table 2.
Observed pointings.
| Pointing ID | RAcen | Deccen | Exp_time | Filter | UT date | Success rate |
|---|---|---|---|---|---|---|
| (deg) | (deg) | (s) | (yyyy.mm.dd) | (3 ≤ Q ≤ 4/Q = 2/Observed) | ||
| P99_COSMOS_HaHP1 | 149.8900 | 1.9003 | 2 × 1800 | H | 2017.04.03 | 14/4/22 |
| P99_COSMOS_HaHP3 | 150.1672 | 1.8391 | 1800 | H | 2017.04.02 | 16/4/22 |
| 1800 | H | 2017.04.04 | ||||
| P99_VVDS_HaHP2 | 36.3758 | −4.2529 | 2 × 1800 | H | 2017.12.23 | 18/2/22 |
| P99_VVDS_HaHP3 | 36.2548 | −4.4108 | 1800 | H | 2017.09.06 | 14/3/22 |
| 1800 | H | 2017.09.14 | ||||
| P99_VVDS_HaKP1 | 36.2005 | −4.0997 | 1800 | K | 2017.07.12 | 5/5/22 |
| 1800 | K | 2017.09.14 | ||||
| P100_COSMOS_HaHP1 | 150.3757 | 2.5168 | 1800 | H | 2018.03.03 | 12/1/22 |
| 1800 | H | 2018.03.17 | ||||
| P100_COSMOS_HaHP2 | 150.3964 | 2.4168 | 2 × 1800 | H | 2018.03.24 | 11/0/22 |
| P100_COSMOS_HaHP3 | 150.3342 | 2.3114 | 2 × 1800 | H | 2018.04.07 | 17/2/22 |
| P100_COSMOS_HaKP1 | 150.3758 | 2.5113 | 1800 | K | 2018.03.17 | 7/1/22 |
| 1800 | K | 2018.03.24 | ||||
| P100_COSMOS_HaKP2 | 150.4966 | 2.5003 | 1800 | K | 2018.04.04 | 9/0/22 |
| 1800 | K | 2018.04.06 | ||||
| P100_SXDF_haHP1 | 34.6131 | −5.3581 | 2 × 1800 | H | 2017.10.01 | 8/2/22 |
| P100_SXDF_haHP2 | 34.7924 | −4.8665 | 2 × 1800 | H | 2017.12.25 | 16/0/22 |
| P100_SXDF_haKP1 | 34.6130 | −5.3587 | 1800 | K | 2017.10.26 | 3/1/22 |
| 1800 | H | 2018.07.29 | ||||
| P100_SXDF_haKP2 | 34.7925 | −4.8669 | 1800 | K | 2018.07.27 | 1/0/22 |
| 1800 | H | 2018.09.09 | ||||
| P100_VVDS_haHP1 | 36.5006 | −4.0833 | 1800 | H | 2018.01.20 | 14/3/22 |
| 1800 | H | 2018.01.21 | ||||
| P100_VVDS_haHP2 | 36.6674 | −4.4833 | 1800 | H | 2018.07.29 | 12/5/22 |
| 1800 | H | 2018.08.27 | ||||
| P100_VVDS_haKP1 | 36.6257 | −4.4940 | 1800 | K | 2017.11.09 | 7/3/22 |
| 1800 | K | 2018.01.15 | ||||
| P100_VVDS_haKP2 | 36.7924 | −4.5337 | 1800 | K | 2018.09.08 | 11/0/22 |
| 1800 | K | 2018.09.09 | ||||
| P100_VVDS_haHP3 | 36.7922 | −4.4501 | 1800 | H | 2018.10.30 | 11/0/22 |
| 1800 | H | 2018.10.31 | ||||
| P101_ECDFS_haHP1 | 53.0840 | −27.7418 | 1800 | H | 2018.07.03 | 12/1/22 |
| 1800 | H | 2018.08.30 | ||||
| P101_SXDF_haHP1 | 34.0842 | −5.1167 | 1800 | H | 2018.09.03 | 12/0/22 |
| 1800 | H | 2018.10.31 | ||||
| P101_SXDF_haKP1 | 34.3047 | −5.3420 | 2 × 1800 | K | 2018.12.09 | 5/1/22 |
| 1800 | K | 2018.12.11 | ||||
| 1800 | K | 2018.12.14 | ||||
| P101_VVDS_haHP1 | 36.8047 | −4.1669 | 2 × 1800 | H | 2018.09.04 | 17/0/22 |
| P101_VVDS_haHP2 | 36.9217 | −4.5527 | 2 × 1800 | H | 2018.12.14 | 15/1/22 |
| P101_VVDS_haKP1 | 36.7296 | −4.4668 | 2 × 1800 | K | 2018.11.12 | 8/0/22 |
| P102_P100_VVDS_HaKP1 ( ⋆ ) | 36.6257 | −4.4944 | 1800 | K | 2018.12.20 | 15/3/22 |
| 1800 | K | 2018.12.21 | ||||
| P102_P99_VVDS_HaKP1 ( ⋆ ) | 36.2009 | −4.1000 | 1800 | K | 2018.12.21 | 15/0/22 |
| 1800 | K | 2018.12.22 | ||||
| P102_VVDS_HaHP1 | 36.5424 | −4.8001 | 1800 | H | 2018.12.22 | 12/3/22 |
| 1800 | H | 2018.12.24 | ||||
| P102_VVDS_HaHP2 | 36.3672 | −4.2446 | 2 × 1800 | H | 2018.12.24 | 14/2/22 |
| P102_COSMOS_HaHP1 | 150.0840 | 2.2193 | 1800 | H | 2019.02.14 | 8/5/22 |
| 1800 | H | 2019.02.23 | ||||
| P102_COSMOS_HaHP2 | 150.2464 | 1.8080 | 1800 | H | 2019.02.21 | 12/0/22 |
| 1800 | H | 2019.02.23 | ||||
| P102_COSMOS_HaHP3 | 149.7305 | 2.1500 | 2 × 1800 | H | 2019.02.22 | 12/0/22 |
| P102_COSMOS_HaHP4 | 149.8884 | 2.5663 | 1800 | H | 2019.02.27 | 14/0/22 |
| 1800 | H | 2019.03.12 | ||||
| P102_COSMOS_HaHP5 | 150.4503 | 2.0366 | 2 × 1800 | H | 2019.01.19 | 12/0/22 |
| P102_SXDF_HaKP1 | 34.6756 | −5.2782 | 1800 | K | 2019.01.25 | 1/0/22 |
| 1800 | K | 2019.02.13 | ||||
| 1800 | K | 2019.02.14 | ||||
| 1800 | K | 2019.02.18 | ||||
| P102_SXDF_HaHP1 | 34.6673 | −5.2670 | 1800 | H | 2019.02.19 | 12/3/22 |
| 1800 | H | 2019.07.14 | ||||
| P102_SXDF_HaHP2 | 34.2004 | −5.2056 | 1800 | H | 2019.07.17 | 9/3/22 |
| 1800 | H | 2019.07.18 | ||||
| P102_SXDF_HaHP3 | 34.6981 | −5.0032 | 1800 | H | 2019.07.30 | 10/0/22 |
Notes. ( ⋆ )These pointings are replicated configurations of two K-band VVDS pointings with low success rates observed during P99 (P102_P99_VVDS_HaKP1) and P100 (P102_P100_VVDS_HaKP1); the overall configuration is maintained, but new objects have been allocated to arms in which a good spectroscopic redshift was derived during the earlier observations (quality flag from three to four, which means that we replaced five to seven galaxies per pointing).
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