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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 6.

Smoothed ﹩{g}^{{\prime} }﹩ band image cutout ﹩(2\mathop{.}\limits^{^{\prime} }1\times 2\mathop{.}\limits^{^{\prime} }1)﹩ before (left panel) and after (middle panel) the aggressive background subtraction. The created masks (blue) for faint point sources are shown in the right panel, applied to the nonsmoothed image.

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