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Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations

  • Authors: Ruxin Barré, Arif Babul, Ghassem Gozaliasl, Alexis Finoguenov, Romeel Davé, Aviv Padawer-Blatt, Douglas Rennehan, Vida Saeedzadeh, Renier T. Hough, Thomas R. Quinn

Ruxin Barré et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

BGG mass-weighted stellar age (Agew) distributions. Formatting follows that of Figure 4. The table contains the results of K-S tests comparing the simulations’ ﹩\mathrm{log}({{\rm{Age}}}_{w}/{\rm{yr}})﹩ distribution to that of COSMOS, where the top, middle, and bottom rows, respectively, compare the full, low-M*, and high-M* samples.

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