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Table 1.

Statistics of the multi-wavelength counterparts adopted in the N2GN catalog.

Survey Instrument Nr. Ref.
and band sources
N2CLS GOODS-N Total 71 This work
With z 68 This work
NIKA2 65 Bing et al. (2023)
1.2 mm 63 Bing et al. (2023)
2.0 mm 26 Bing et al. (2023)
NOEMA 1.2 or 2.0 mm 31 ( * ) W21CV, this work
NOEMA 1.2 or 2.0 mm 2 W16EE, E16AI, Bing (2022)

Others sub-mm to radio SMA 860 μm 22 Cowie et al. (2017)
SCUBA2 850 μm 46 Cowie et al. (2017)
SCUBA2 450 μm 31 Barger et al. (2022)
NOEMA 5 Aa.Vv. (Sect. 2.4)
VLA 1−2 GHz 53 Owen (2018)

CANDELS/GOODS Optical U to K 59 Barro et al. (2019)
FRESCO, JADES, PANORAMIC, Congress JWST F090W to F770W 24 New extraction
CANDELS/GOODS IRAC 3.6 to 8.0 μm 59 Barro et al. (2019), Liu et al. (2018)
PeakUp IRS IRS 16 μm 10 Liu et al. (2018)
GOODS MIPS 24 μm 43 Barro et al. (2019), Liu et al. (2018)
PEP + GOODS-H PACS 100, 160 μm 28 Magnelli et al. (2013), Liu et al. (2018)
GOODS-H/HerMES SPIRE 250−500 μm 22 Elbaz et al. (2011), Oliver et al. (2012), Liu et al. (2018)
CDFN Chandra 0.5 to 7.0 keV 5 Evans et al. (2024)

Notes. ( * )26/27 NIKA2 detected/targeted; five are split in two components by NOEMA.

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