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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 9.

Molecular gas depletion timescale (tdep) as a function of the specific SFR for the ASPECS CO galaxies. In both panels, the background blue contour levels represent the distribution of z > 1 PHIBSS1/2 CO galaxies (Tacconi et al. 2013, 2018), and the coloring of each ASPECS source represents its respective redshift. The left panel shows tdep as a function of sSFR. Here the dashed lines represent curves of fixed gas fraction (Mmol/Mstars). The right panel shows the sSFR normalized by the value of the sSFR expected for the MS (which is a function of the redshift and stellar mass) from Schreiber et al. (2015). In this case, the dashed lines are shown only for visualization purposes. 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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