Table 3.
N2CLS galaxies identified in the overdensity.
| NIKA2 ID | Alt.† | RA | Dec | ![]() |
![]() |
Comment |
|---|---|---|---|---|---|---|
| [hh:mm:ss] | [dd:mm:ss] | |||||
| N2GN_1_01 | GN10, S2 | 12:36:33.44 | 62:14:08.7 | 5.303s | Optically dark | |
| N2GN_1_06 | HDF850.1 | 12:36:51.99 | 62:12:25.7 | 5.185s | Optically dark | |
| N2GN_1_13 | GN32 | 12:36:58.61 | 62:14:51.1 | 5.182s | Optically dark | |
| N2GN_1_23 | GN15, S3 | 12:36:56.54 | 62:12:07.5 | 5.179s | Optically dark | |
| N2GN_1_61 | P-40 | 12:36:57.48 | 62:16:54.4 | 5.201s | Optically dark | |
| N2GN_1_43 | 12:37:11.95 | 62:11:19.7 | 5.87 ± 0.38p | 5.31![]() |
Optically dark | |
| N2GN_1_26 | GN38 | 12:37:41.14 | 62:12:20.4 | 5.31 ± 0.08p | 4.87![]() |
|
| N2GN_1_57 | HRG14 | 12:37:31.69 | 62:16:16.5 | 5.30 ± 0.18p | 5.18![]() |
|
Notes. The majority are not detected in the deepest HST image, which reaches a 5σ depth of 27.3 mag in F160W (Barro et al. 2019). These sources are labelled ‘Optically dark’.
†The HDF850, GN, HRG14, S and P- nomenclatures were defined by Hughes et al. (1998), Pope et al. (2005), Finkelstein et al. (2015), Xiao et al. (2024), Greve et al. (2008).
‡s: spectroscopic redshift and p: photometric redshift, from B25;
hphotometric redshift from New-Hyperz.
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