The ALMA Spectroscopic Survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history

We use the results from the ALMA large program ASPECS, the spectroscopic survey in the Hubble Ultra Deep Field (HUDF), to constrain CO luminosity functions of galaxies and the resulting redshift evolution of \(\rho\)(H\(_2\)). The broad frequency range covered enables us to identify CO emission line...

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Veröffentlicht in:	arXiv.org 2019-03
Hauptverfasser:	Decarli, Roberto, Fabian, Walter, Gónzalez-López, Jorge, Aravena, Manuel, Boogaard, Leindert, Carilli, Chris, Cox, Pierre, Daddi, Emanuele, Popping, Gergö, Riechers, Dominik, Bade Uzgil, Weiss, Axel, Assef, Roberto J, Bacon, Roland, Bauer, Franz Erik, Bertoldi, Frank, Bouwens, Rychard, Contini, Thierry, Cortes, Paulo C, da Cunha, Elisabete, Díaz-Santos, Tanio, Elbaz, David, Inami, Hanae, Hodge, Jacqueline, Ivison, Rob, Olivier Le Fèvre, Magnelli, Benjamin, Novak, Mladen, Oesch, Pascal, Hans-Walter Rix, Sargent, Mark T, Smail, Ian R, Swinbank, A Mark, Somerville, Rachel S, van der Werf, Paul, Wagg, Jeff, Wisotzki, Lutz
Format:	Artikel
Sprache:	eng
Schlagworte:	Cosmic gases Excitation Frequency ranges Galactic evolution Galaxies Gas density Hubble deep field Knee Luminosity Molecular gases Physics - Astrophysics of Galaxies Red shift Spectroscopy Star & galaxy formation Star formation rate Stellar evolution
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