Image Details

Choose export citation format:

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 5.

Molecular gas mass versus stellar mass with 195616 (209435) shown by the solid blue (red) star. The top and right panels show the normalized histogram of stellar mass and molecular gas mass, respectively, for A3COSMOS galaxies in the redshift range 2.1 ≤ z < 2.9 (red) and 2.9 ≤ z < 3.7 (blue). The colored contours enclose 25%, 50%, and 75% of the galaxy population, showing the 2D density distributions for A3COSMOS catalog in each redshift range, constructed using kernel density estimation (KDE). The open colored circles show medians, with 3σ bootstrap uncertainties. The dashed black lines show gas-to-stellar-mass ratios of 0.1, 0.3, and 1. The magenta vertical line in the top panel shows the lower mass limit (﹩{\mathrm{log}}({M}_{\star }/{M}_{\odot })﹩ > 11) used to make Figure 6.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse