First ALMA [CII] observations of high-redshift quiescent galaxies reveal gas fractions from 0.1% to 25%, dust temperatures of 40-50 K, strong [CII] deficits, and merger-like features, suggesting merger-driven quenching with non-stellar dust heating.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2representative citing papers
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.
citing papers explorer
-
A first [CII] view of high-z quiescent galaxies
First ALMA [CII] observations of high-redshift quiescent galaxies reveal gas fractions from 0.1% to 25%, dust temperatures of 40-50 K, strong [CII] deficits, and merger-like features, suggesting merger-driven quenching with non-stellar dust heating.
-
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.