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Star Formation under a Cosmic Microscope: Highly Magnified z = 11 Galaxy behind the Bullet Cluster

  • Authors: Maruša Bradač, Jon Judež, Chris Willott, Gregor Rihtaršic, Nicholas S. Martis, Anishya Harshan, Giordano Felicioni, Yoshihisa Asada, Guillaume Desprez, Douglas Clowe, Anthony H. Gonzalez, Christine Jones, Brian C. Lemaux, Maxim Markevitch, Vladan Markov, Lamiya Mowla, Gaël Noirot, Annika H. G. Peter, Andrew Robertson, Ghassan T. E. Sarrouh, Marcin Sawicki, Tim Schrabback, Roberta Tripodi

Maruša Bradač et al 2025 The Astrophysical Journal Letters 995 .

  • Provider: AAS Journals

Caption: Figure 5.

Results of the SED fitting using original full photometry using Photutils corrected by dividing by μ (labeled “All”; see also Table 1) and derived using Galfit for the smooth light component (G) and the three clumps (labeled C1–3). Shown are fluxes in red and SED-predicted fluxes in open circles in units of μJy. Derived stellar properties are given in the inset. While fluxes in F150W and shortward are shown, they were not included in the fit, as the redshift is only allowed to vary based on spectroscopic redshift measurement.

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