The N2CLS survey observed the GOODS-N and COSMOS fields at 260 GHz and 150 GHz with the NIKA2 camera, reaching the confusion limit in GOODS-N at 1.2 mm and approaching it at 2.0 mm. In this short proceedings, we present the results of the survey, including the source number counts, multi-wavelength SED fitting, the dust mass function, the evolution of the dust mass density, and the physical characterization of the detected galaxy population.
N2CLS. The NIKA2 view of the distant Universe / Berta, S., Adam, R., Ade, P., Ajeddig, H., Amarantidis, S., André, P., Aussel, H., Beelen, A., Benoît, A., Béthermin, M., Bongiovanni, A., Bounmy, J., Bourrion, O., Calvo, M., Catalano, A., Chérouvrier, D., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E.F.C., et al.. - In: EPJ WEB OF CONFERENCES. - ISSN 2100-014X. - 353:(2026), pp. 1-6. [10.1051/epjconf/202635301002]
N2CLS. The NIKA2 view of the distant Universe
De Petris, M.;Pisano, G.;
2026
Abstract
The N2CLS survey observed the GOODS-N and COSMOS fields at 260 GHz and 150 GHz with the NIKA2 camera, reaching the confusion limit in GOODS-N at 1.2 mm and approaching it at 2.0 mm. In this short proceedings, we present the results of the survey, including the source number counts, multi-wavelength SED fitting, the dust mass function, the evolution of the dust mass density, and the physical characterization of the detected galaxy population.| File | Dimensione | Formato | |
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