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Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). II. Cold Molecular Gas Evolution out to Redshift 6

  • Authors: Daizhong Liu, E. Schinnerer, B. Groves, B. Magnelli, P. Lang, S. Leslie, E. Jiménez-Andrade, D.A. Riechers, G. Popping, Georgios E. Magdis, E. Daddi, M. Sargent, Yu Gao, Y. Fudamoto, P.A. Oesch, and F. Bertoldi

2019 The Astrophysical Journal 887 235.

  • Provider: AAS Journals

Caption: Figure 1.

Overview of popular molecular gas mass (﹩{M}_{\mathrm{mol}\mathrm{gas}}﹩) calibration methods for high-redshift (i.e., ﹩z\gt 1﹩) galaxies sorted into three categories: (a) (sub)millimeter emission line observations, (b) galaxy SED-fitted dust mass, and (c) RJ-tail dust continuum. See description in Section 3. The corresponding sections in this paper are labeled in the flow chart. The references for the ﹩{\alpha }_{850,\mathrm{mol}}﹩ conversion factors are Scoville et al. (2017; S17) and Hughes et al. (2017; H17); and for α160–500,mol, Groves et al. (2015; G15).

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