Luminosity functions (LF) are some of the most basic quantities providing insights into galaxy evolution across cosmic time and enabling a direct comparison between observations and simulations. Here, we present the first [CII]158$\mu$m LF at $z\sim7$ from a sizeable UV-selected ALMA sample. Our analysis makes use of 2...
T. Herard-Demanche, P. Oesch, R. Bouwens et al.· 0 citations
Although less than 1 percent of the baryonic mass budget of a galaxy, cosmic dust profoundly alters the multi-wavelength appearance of galaxies across cosmic time. The (sub)millimeter wavelength regime is uniquely capable of weighing these dust reservoirs, and revealing the total extent of galaxy evolution that remains...
H. Algera, T. Bakx, M. Aravena et al.· 0 citations
A complete overview of the stellar, gas and dust contents of galaxies is key to understanding their assembly at early times. However, an estimation of molecular and atomic gas reservoirs at high redshift relies on various indirect tracers, while robust dust mass measurements require multiband far-infrared continuum obs...
H. Algera, R. Herrera-Camus, M. Aravena et al.· Astronomy & Astrophysics· 0 citations
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