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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 9.

Same as Figure 8, but splitting MQGs and MSFGs into different stellar mass bins (low to high, left to right) and different regions (top to bottom, inside overdense peak versus immediately nearby overdense peak). The black line representing all spectroscopically confirmed galaxies is uniform across the mass bins. At lower stellar masses, the clustering of MQGs and MSFGs is indistinguishable from the overall spectroscopic sample; at higher stellar masses, however, MQGs appear to cluster much more strongly in overdense peaks.

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