Image Details

Choose export citation format:

The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations

  • Authors: Hassen M. Yesuf, Connor Bottrell, Luis C. Ho, Aaron S. G. Robotham, Sabine Bellstedt, Robin H. W. Cook, Lei Hao, Fengshan Liu

Hassen M. Yesuf et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 6.

Galaxy concentration function. Number densities of galaxies as a function of concentration C82, are shown in panels for three stellar mass bins (﹩{\rm{log}}({M}_{\star }/{M}_{\odot })=10.0﹩–10.5, 10.5–11.0, 11.0–11.5) and three star formation categories (all galaxies, star-forming: ﹩{\rm{\Delta }}\mathrm{log}{\rm{SFR}}\gt -1﹩, quiescent: ﹩{\rm{\Delta }}\mathrm{log}{\rm{SFR}}\lt -1﹩). Each panel shows the logarithmic number density, ﹩{\rm{log}}(\phi (C)/{{\rm{Mpc}}}^{-3})﹩, versus concentration. Simulations are indicated by colored lines: TNG50 (dark green, solid), TNG100 (forest green, dotted), EAGLE (crimson, dashed), and SIMBA (dark orange, dashed–dotted). Observational data from HSC+GAMA are shown as blue circles.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse