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Galaxy Luminosity Function of the Coma Cluster from Deep ﹩{u}^{{\prime} }﹩ − ﹩{g}^{{\prime} }﹩ − ﹩{r}^{{\prime} }﹩ Wendelstein Imaging Data

  • Authors: Raphael Zöller, Matthias Kluge, Ralf Bender, Jan-Niklas Pippert, Benjamin Seidel, Claus Gössl, Ulrich Hopp, Hanna Kellermann, Christoph Ries, Arno Riffeser, Michael Schmidt, Luis Thomas

Raphael Zöller et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 9.

﹩{u}^{{\prime} }-{g}^{{\prime} }﹩ vs. ﹩{g}^{{\prime} }-{r}^{{\prime} }﹩ number density color–color diagrams for the faint Coma cluster and comparison samples. The top row shows the density distributions for Coma, the combined reference fields, and the individual reference fields Ref1 and Ref2, all without completeness correction. The bottom row shows Coma with EVCC Virgo contours overlaid, followed by residual maps obtained by subtracting each reference sample from the Coma distribution. Galaxies in the top left of the red visualized selection cutoffs are considered to be quenched. The samples are limited to galaxies with ﹩m\lt 24\,{g}^{{\prime} }\,{\rm{mag}}﹩.

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