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GLOBULAR CLUSTER SYSTEMS IN BRIGHTEST CLUSTER GALAXIES. III. BEYOND BIMODALITY

  • Authors: William E. Harris, Stephanie M. Ciccone, Gwendolyn M. Eadie, Oleg Y. Gnedin, Douglas Geisler, Barry Rothberg, and Jeremy Bailin

2017 The Astrophysical Journal 835 101.

  • Provider: AAS Journals

Caption: Figure 10.

Color–magnitude diagrams for the measured starlike objects around UGC 9799, for the ACS/WFC field (left panel) and the outlying WFC3/WFC field (right panel). Here the native filter magnitudes ﹩F475W,F814W﹩ are plotted, closely equivalent to I vs. ﹩(g^{\prime} -I)﹩ in the VEGAMAG system. These values are not corrected for reddening. For the WFC3 field, objects with ﹩y\lt 95^{\prime\prime} ﹩ are plotted to avoid contamination from another galaxy (see text). Detection completeness levels of f = 0.5 are marked with the red dashed lines, and the photometric measurement uncertainties are indicated by the error bars at left.

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