An empirical correction that folds map power-spectrum clustering strength into the P(D) histogram recovers unbiased submillimetre galaxy counts, revising Herschel-SPIRE GOODS-N results by up to a factor 1.6 at 500 µm.
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The N2CLS 2mm survey measures a mean S2/S1.2 color of 0.222 and mean redshifts of 3.2-3.6, finds no exotic 2mm-only population, and shows 2mm samples miss z~2 galaxies compared to 1.2mm samples.
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How to count clustered galaxies
An empirical correction that folds map power-spectrum clustering strength into the P(D) histogram recovers unbiased submillimetre galaxy counts, revising Herschel-SPIRE GOODS-N results by up to a factor 1.6 at 500 µm.
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The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
The N2CLS 2mm survey measures a mean S2/S1.2 color of 0.222 and mean redshifts of 3.2-3.6, finds no exotic 2mm-only population, and shows 2mm samples miss z~2 galaxies compared to 1.2mm samples.