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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 8.

Distribution of derived ISM properties (gas depletion timescale and gas fraction) for the CO line sources in the ASPECS field. The black solid, yellow shaded histogram represents the distributions of all ASPECS sources (both CO and MUSE based). The gray shaded histogram shows the distribution of the MUSE-based sources only. The light blue histograms show the distribution of z > 1 PHIBSS1/2 CO sources (Tacconi et al. 2013, 2018). Due to its uncertain counterpart photometry, 3 mm.12 is not considered in this figure. Sources 3 mm.1 and 3 mm.13 have high values of Mmol/Mstars falling outside the range covered by this figure. 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 (K km s−1 pc2)−1 for the ASPECS CO sources.

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