The ALMA REBELS survey : the dust-obscured cosmic star formation rate density at redshift 7

Cosmic dust is an essential component shaping both the evolution of galaxies and their observational signatures. How quickly dust builds up in the early Universe remains an open question that requires deep observations at (sub-)millimetre wavelengths to resolve. Here, we use Atacama Large Millimeter...

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Hauptverfasser:	Algera, Hiddo S B, Inami, Hanae, Oesch, Pascal A, Sommovigo, Laura, Bouwens, Rychard J, Topping, Michael W, Schouws, Sander, Stefanon, Mauro, Stark, Daniel P, Aravena, Manuel, Barrufet, Laia, da Cunha, Elisabete, Dayal, Pratika, Endsley, Ryan, Ferrara, Andrea, Fudamoto, Yoshinobu, Gonzalez, Valentino, Graziani, Luca, Hodge, Jacqueline A, Hygate, Alexander P S, De Looze, Ilse, Nanayakkara, Themiya, Schneider, Raffaella, van der Werf, Paul P
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy and Astrophysics DOMINANT MODE FORMING GALAXIES galaxies: evolution galaxies: high-redshift INFRARED EXCESS LUMINOSITY FUNCTION MASSIVE GALAXIES PHYSICAL-PROPERTIES Physics and Astronomy REIONIZATION ERA Space and Planetary Science SPECTRAL ENERGY-DISTRIBUTION SPECTROSCOPIC SURVEY submillimetre: galaxies ULTRA-DEEP FIELD
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