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Spatially Resolved Physical Properties of Young Star Clusters and Star-forming Clumps in the Brightest z > 6 Galaxy, the Strongly Lensed Cosmic Spear at z = 6.2

Authors: Abdurro'uf, Dan Coe, Tom Resseguier, Calla Murphy, Xinfeng Xu, Angela Adamo, Namrata Roy, Alaina Henry, Vasily Kokorev, Gabriel Brammer, Seiji Fujimoto, Henry C. Ferguson, Amanda Pagul, Rogier A. Windhorst, Timothy Heckman, Jose M. Diego, Hollis B. Akins, Joseph F. V. Allingham, Ricardo O. Amorín, Danielle A. Berg, Maruša Bradač, Larry D. Bradley, Wenlei Chen, John Chisholm, Christopher J. Conselice, Pratika Dayal, Miroslava Dessauges-Zavadsky, Andreas L. Faisst, Steven L. Finkelstein, Yoshinobu Fudamoto, Lukas J. Furtak, Yuichi Harikane, Tiger Yu-Yang Hsiao, Yolanda Jimenez-Teja, Anton M. Koekemoer, Rebecca L. Larson, Ray A. Lucas, Matteo Messa, Lamiya Mowla, Minami Nakane, Gaël Noirot, Richard Pan, Massimo Pascale, Johan Richard, Massimo Ricotti, Luke Robbins, Daniel Schaerer, Fengwu Sun, Eros Vanzella, Brian Welch, Chris Willott, Adi Zitrin

Abdurro’uf et al 2026 The Astrophysical Journal 1011 .

Provider: AAS Journals

Caption: Figure D1.

Photometric redshift estimation for the CI using EAZY and BAGPIPES. Black circles denote the observed photometry. The best-fit models (spectra and photometry) from EAZY and BAGPIPES are shown in green and blue, respectively. The derived photometric redshifts are 6.12 ± 0.17 (EAZY) and ﹩{6.28}_{-0.13}^{+0.14}﹩ (BAGPIPES). The inset panel shows the redshift posterior probability distributions. The vertical dashed red line indicates the spectroscopic redshift of the Cosmic Spear.

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