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MAGAZ3NE: Far-IR and Radio Insights into the Nature and Properties of Ultramassive Galaxies at z ≳ 3

  • Authors: Wenjun Chang, Gillian Wilson, Ben Forrest, Ian McConachie, Tracy Webb, Allison Noble, Adam Muzzin, M. C. Cooper, Danilo Marchesini, Gabriela Canalizo, A. J. Battisti, Aurelien Henry, Percy Gomez, Stephanie M. Urbano Stawinski, M.E. Wisz

Wenjun Chang et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 6.

Molecular gas mass as a function of SFR (left panel) and depletion timescale as a function of specific SFR (right panel). The symbols are the same as in Figure 5, but note that only A3COSMOS galaxies with a stellar mass of ﹩{\mathrm{log}}({M}_{\star }/{M}_{\odot })﹩ > 11 were used to make this figure (see Table 5). The dashed black lines in the left panel correspond to gas depletion timescales of 50 Myr, 500 Myr, and 5 Gyr.

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