Figure 5 from The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies

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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 5.

SFR vs. stellar mass diagram for the ASPECS CO sources, compared to PHIBSS1/2 CO sources at z > 1. The PHIBSS1/2 galaxies are represented by the blue contours. The solid lines represent the observational relationships between SFR and stellar mass at different redshifts derived by Schreiber et al. (2015). These redshifts are denoted in different colors as shown by the color bar to the right. Three of the ASPECS CO-selected galaxies lie >0.4 dex below the MS at their respective redshifts (3 mm.2 and 3 mm.10).

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