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Table 3.

N2CLS galaxies identified in the overdensity.

NIKA2 ID Alt. RA Dec z s , p $ z_{\mathrm{s,p}}^{\ddagger} $ z p h $ z_{\mathrm{p}}^{h} $ 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 0.86 + 1.33 $ _{-0.86}^{+1.33} $ Optically dark
N2GN_1_26 GN38 12:37:41.14 62:12:20.4 5.31 ± 0.08p 4.87 0.19 + 0.21 $ _{-0.19}^{+0.21} $
N2GN_1_57 HRG14 12:37:31.69 62:16:16.5 5.30 ± 0.18p 5.18 0.20 + 0.19 $ _{-0.20}^{+ 0.19} $

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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