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, multiwavelength SED fitting, the dust mass function, the evolution of the dust mass density, and the physical characterization of the detected galaxy population.
Berta et al. (Fri,) studied this question.