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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 11.

﹩{g}^{{\prime} }-{r}^{{\prime} }﹩ vs. ﹩{m}_{{g}^{{\prime} }}﹩ number-density color–magnitude diagrams for the Coma cluster and reference fields. The top row shows the full galaxy samples for Coma, the combined reference fields, and the residual distribution obtained by subtracting the reference field distribution from the Coma distribution. The bottom row shows the corresponding distributions after applying the quiescent color–color preselection. The red dashed lines indicate the adopted 3σ intrinsic width around the fitted Coma red sequence.

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