Globular Clusters in the Galaxy Cluster MACS0416 at <i>z</i>  = 0.397

Abstract We present a photometric analysis of globular clusters (GCs) in the massive galaxy cluster MACS J0416.1−2403 ( z = 0.397) using deep JWST/NIRCam imaging from the PEARLS program. Point-spread function photometry was performed in the short wavelength filters, F090W, F115W, F150W, and F200W, yielding a catalog of ∼3 × 10 3 unresolved, point-like sources consistent with a GC population. Artificial-star tests indicate 80% completeness at F200W ≃ 30.36 mag. The color–magnitude diagrams show a narrow GC sequence well reproduced by PARSEC single-stellar-population models spanning ages of 5–9 Gyr and metallicities from [M/H] ≈ −2.0 to +0.2, consistent with evolved GC systems at this redshift. The GC luminosity function follows a log-normal form truncated by incompleteness at the faint end. The brightest sources extend slightly beyond the locus of classical GCs, suggesting a small number of ultracompact dwarf-like systems or stripped nuclei, while the bulk of the population exhibits the luminosities and colors expected for mature GCs at z ≃ 0.4.

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Publication Details

Journal
The Astronomical Journal
Published
2025-12-19
DOI
https://doi.org/10.3847/1538-3881/ae209a
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
0.00
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article

Globular Clusters in the Galaxy Cluster MACS0416 at z  = 0.397

Ray A. Lucas, Jake Summers, Kate Hartman, Massimo Ricotti et al.
The Astronomical Journal
Galaxies: Formation, Evolution, Phenomena
article

Globular Clusters in the Galaxy Cluster MACS0416 at z  = 0.397

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

Abstract

Abstract We present a photometric analysis of globular clusters (GCs) in the massive galaxy cluster MACS J0416.1−2403 ( z = 0.397) using deep JWST/NIRCam imaging from the PEARLS program. Point-spread function photometry was performed in the short wavelength filters, F090W, F115W, F150W, and F200W, yielding a catalog of ∼3 × 10 3 unresolved, point-like sources consistent with a GC population. Artificial-star tests indicate 80% completeness at F200W ≃ 30.36 mag. The color–magnitude diagrams show a narrow GC sequence well reproduced by PARSEC single-stellar-population models spanning ages of 5–9 Gyr and metallicities from [M/H] ≈ −2.0 to +0.2, consistent with evolved GC systems at this redshift. The GC luminosity function follows a log-normal form truncated by incompleteness at the faint end. The brightest sources extend slightly beyond the locus of classical GCs, suggesting a small number of ultracompact dwarf-like systems or stripped nuclei, while the bulk of the population exhibits the luminosities and colors expected for mature GCs at z ≃ 0.4.

The Astronomical JournalVol. 171(1)
Herzberg Institute of Astrophysics (CA), Space Telescope Science Institute (US), University of Arizona (US), University of Louisville (US), University of Alabama (US), The University of Western Australia (AU), Trieste Astronomical Observatory (IT), University of Manchester (GB), Université Bourgogne Franche-Comté (FR), Instituto de Física de Cantabria (ES), International Centre for Radio Astronomy Research (AU), Arizona State University (US), University of Maryland, College Park (US), University of Missouri (US), McMaster University (CA)
Openalex Percentile: Top 71%
Galaxies: Formation, Evolution, Phenomena
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