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Where Galaxies Go to Die: The Environments of Massive Quiescent Galaxies at 3 < z < 5

  • Authors: Ian McConachie, Anna de Graaff, Michael V. Maseda, Joel Leja, Yunchong Zhang, David J. Setton, Rachel Bezanson, Leindert A. Boogaard, Gabriel Brammer, Nikko J. Cleri, Olivia R. Cooper, Karl Glazebrook, Rashmi Gottumukkala, Jenny E. Greene, Andy D. Goulding, Michaela Hirschmann, Gourav Khullar, Ivo Labbe, Zach Lewis, Jorryt Matthee, Tim B. Miller, Rohan P. Naidu, Themiya Nanayakkara, Erica J. Nelson, Pascal A. Oesch, Sedona H. Price, Katherine A. Suess, Bingjie Wang, Katherine E. Whitaker, Christina C. Williams

Ian McConachie et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 7.

Left: stellar mass as a function of ﹩\mathrm{log}({\delta }_{{\rm{gal}}}+1)﹩ for MQGs (open circles correspond to properties inferred from modeling just photometry). The red line shows the best-fit line to the MQG population using orthogonal distance regression, and the semitransparent bands show the 1σ confidence limits. The best-fit line and the scatter σNMAD are shown in the top of the panel. Right: same as the left panel, but for the MSFG population. We do not fit a line to the MSFG population due to its higher uncertainties on ﹩\mathrm{log}({M}_{* }/{M}_{\odot })﹩, though we do note that there seems to be a visually flat or negative relation between stellar mass and local overdensity.

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