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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 4.

RGB (F277W, F357W, and F444W) image of the Bullet Cluster. Overlaid (in red) is the critical curve calculated at the redshift of BulletArc-z11 used in this Letter. In the inset (10″ × 10″), we use high-resolution RGB images (F115W, F150W, and F200W) to show BulletArc-z11 and the same red critical curve as well as in cyan the one with a cluster member added as described in Section 3.3.

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