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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 3.

Source plane modeling using Lenstruction (L. Yang et al. 2020). From the top left, we plot the observed image (in F200W), the source model, the best-fit image model (after lensing and PSF convolution have been applied), and normalized residuals. The source was modeled using an underlying galaxy component G and three small clumps (#1–3) modeled using Gaussian profiles.

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