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
From the onset of observations of JWST we have discovered unexpectedly luminous galaxies at redshifts z > 10 and as high as z = 14. With their discovery, the question immediately followed as to where their progenitors are, since such progenitors should be within reach of existing surveys. However, the discovery of seve...
M. Bradač, C. Willott, Y. Asada et al.· Astrophysical Journal Letter...· 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
The finding that galaxies in the first 500Myr were much more numerous and/or brighter than expected is often cited as one of the main discoveries of the James Webb Space Telescope in its first four years of operation. This result is now solidly based on an impressive number of surveys that have detected, spectroscopica...
A. Fontana, H. Atek, V. Bromm et al.· 0 citations
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