ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CO LUMINOSITY FUNCTIONS AND THE EVOLUTION OF THE COSMIC DENSITY OF MOLECULAR GAS

In this paper we use ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field in band. 3 and band. 6, to place blind constraints on the CO luminosity function and the evolution of the cosmic molecular gas density as a function of redshift up to z similar to 4.5. This study is based on ga...

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Bibliographic Details
Main Authors:	Decarli, Roberto, Walter, Fabian, Aravena, Manuel, Carilli, Chris, Bouwens, Rychard, da Cunha, Elisabete, Daddi, Emanuele, Ivison, R. J., Popping, Gergö, Riechers, Dominik, Smail, Ian R., Swinbank, Mark, Weiss, Axel, Anguita, Timo, Assef, Roberto J., Bauer, Franz E., Bell, Eric F., Bertoldi, Frank, Chapman, Scott, Colina, Luis, Cortes, Paulo C., Cox, Pierre, Dickinson, Mark, Elbaz, David, Gónzalez-López, Jorge, Ibar, Edo, Infante, Leopoldo, Hodge, Jacqueline, Karim, Alex, Fevre, Olivier Le, Magnelli, Benjamin, Neri, Roberto, Oesch, Pascal, Ota, Kazuaki, Rix, Hans-Walter, Sargent, Mark, Sheth, Kartik, van der Wel, Arjen, van der Werf, Paul, Wagg, Jeff
Other Authors:	Univ Arizona, Steward Observ
Language:	en
Published:	IOP PUBLISHING LTD 2016
Subjects:	galaxies: evolution galaxies: formation galaxies: high-redshift galaxies: ISM surveys
Online Access:	http://hdl.handle.net/10150/623950 http://arizona.openrepository.com/arizona/handle/10150/623950

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http://hdl.handle.net/10150/623950
http://arizona.openrepository.com/arizona/handle/10150/623950

ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CO LUMINOSITY FUNCTIONS AND THE EVOLUTION OF THE COSMIC DENSITY OF MOLECULAR GAS

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