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Globular Clusters in the Galaxy Cluster MACS0416 at z = 0.397

Authors: Jessica M. Berkheimer, Rogier A. Windhorst, William E. Harris, Anton M. Koekemoer, Timothy Carleton, Seth H. Cohen, Rolf A. Jansen, Dan Coe, Jose Diego, Christopher J. Conselice, Simon P. Driver, Brenda L. Frye, Norman A. Grogin, Kate Hartman, Tyler R. Hinrichs, Benne W. Holwerda, Patrick S. Kamieneski, Kaitlyn E. Keatley, William C. Keel, Ray A. Lucas, Madeline A. Marshall, Mario Nonino, Nor Pirzkal, Massimo Ricotti, Clayton D. Robertson, Aaron Robotham, Russell E. Ryan, Jake Summers, Christopher N.A. Willmer, Haojing Yan

Jessica M. Berkheimer et al 2026 The Astronomical Journal 171 .

Provider: AAS Journals

Caption: Figure 6.

Two-component GMM fits to the F115W − F200W (top) and F150W − F200W (bottom) color distributions at the 95% and 97%completeness levels. Histograms show our MACS0416 GC data, with individual Gaussian components (dashed lines) and total fits (solid lines) overlaid. Error bars in the upper-left corners display the photometric color error in the displayed completeness level.

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