Notes. The average and central noise levels of N2CLS are provided as values in and out of parentheses, respectively. For surveys not exactly observing at 1.2 mm (i.e., AzTEC observations at 1.1 mm), the rms noise is normalized to 1.2 mm assuming the average IR SED of star-forming galaxies at z = 2 from Béthermin et al. (2015a). Under this assumption, the depths of AzTEC and SCUBA2 observations are divided by a factor of 1.25 and 2.10, respectively. v_obs is the central frequency of the instruments.

References.⁽¹⁾Perera et al. (2008), ⁽²⁾Cowie et al. (2017, Central region), ⁽³⁾Staguhn et al. (2014), ⁽⁴⁾Aretxaga et al. (2011), ⁽⁵⁾Bertoldi et al. (2007),⁽⁶⁾ Simpson et al. (2019), ⁽⁷⁾Magnelli et al. (2019).