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The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies

  • Authors: Manuel Aravena, Roberto Decarli, Jorge Gónzalez-López, Leindert Boogaard, Fabian Walter, Chris Carilli, Gergö Popping, Axel Weiss, Roberto J. Assef, Roland Bacon, Franz Erik Bauer, Frank Bertoldi, Richard Bouwens, Thierry Contini, Paulo C. Cortes, Pierre Cox, Elisabete da Cunha, Emanuele Daddi, Tanio Díaz-Santos, David Elbaz, Jacqueline Hodge, Hanae Inami, Rob Ivison, Olivier Le Fèvre, Benjamin Magnelli, Pascal Oesch, Dominik Riechers, Ian Smail, Rachel S. Somerville, A. M. Swinbank, Bade Uzgil, Paul van der Werf, Jeff Wagg, and Lutz Wisotzki

2019 The Astrophysical Journal 882 136.

  • Provider: AAS Journals

Caption: Figure 10.

Evolution of the tdepl and fmol = Mmol/Mstars with redshift. The background blue contour levels represent the distribution of galaxies from the PHIBSS1/2 compilation (Tacconi et al. 2013, 2018). As a reference in redshift, we also show as green contours the distribution of galaxies detected in CO line emission at z < 0.5 from the PHIBSS1/2 compilation (e.g., from xCOLDGASS, GOALS, and EgNOG surveys). The solid lines show the expected evolution of tdepl and fmol with redshift, based on previous targeted observations of star-forming galaxies. A fixed conversion factor αCO = 3.6 (K km s−1 pc2)−1 has been assumed for the ASPECS CO sources. The comparison sample uses a metallicity-based prescription for this parameter. Typical values will range between αCO = 2–5 M (K km s−1 pc2)−1 for the ASPECS CO sources.

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