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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 2.

MUV-versus-redshift plot for BulletArc-z11 (star) and the spectroscopically confirmed sources from the literature (circles, collated in G. Roberts-Borsani et al. 2025). Fill colors represent magnification μ given by the color bar. Open circles are blank-field sources with μ = 1. MUV values for different characteristic luminosities L* (at z ∼ 10, taken from C. J. Willott et al. 2024) are shown as dashed horizontal lines. The uncertainty on MUV for BulletArc-z11 is partly hidden behind the symbol and includes lensing uncertainties.

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