Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2966
Title: Early Results from GLASS-JWST. III. Galaxy Candidates at z ∼9-15
Authors: Castellano, Marco
Fontana, Adriano
Treu, Tommaso
Santini, Paola
Merlin, Emiliano
Leethochawalit, Nicha
Trenti, Michele
Vanzella, Eros
Meštrić, Uroš 
Bonchi, Andrea
Belfiori, Davide
Nonino, Mario
Paris, Diego
Polenta, Gianluca
Roberts-Borsani, Guido
Boyett, Kristan
Bradač, Maruša
Calabrò, Antonello
Glazebrook, Karl
Grillo, Claudio
Mascia, Sara
Mason, Charlotte
Mercurio, Amata
Morishita, Takahiro
Nanayakkara, Themiya
Pentericci, Laura
Rosati, Piero
Vulcani, Benedetta
Wang, Xin
Yang, Lilan
Affiliations: Astronomy 
Issue Date: 1-Oct-2022
Rank: M21a
Publisher: IOP Science
Journal: Astrophysical Journal Letters
Abstract: 
We present the results of a first search for galaxy candidates at z ∼ 9-15 on deep seven-band NIRCam imaging acquired as part of the GLASS-James Webb Space Telescope (JWST) Early Release Science Program on a flanking field of the Frontier Fields cluster A2744. Candidates are selected via two different renditions of the Lyman-break technique, isolating objects at z ∼ 9-11, and z ∼ 9-15, respectively, supplemented by photometric redshifts obtained with two independent codes. We find five color-selected candidates at z > 9, plus one additional candidate with photometric redshift z phot ≥ 9. In particular, we identify two bright candidates at M UV ≃ −21 that are unambiguously placed at z ≃ 10.6 and z ≃ 12.2, respectively. The total number of galaxies discovered at z > 9 is in line with the predictions of a nonevolving luminosity function. The two bright ones at z > 10 are unexpected given the survey volume, although cosmic variance and small number statistics limits general conclusions. This first search demonstrates the unique power of JWST to discover galaxies at the high-redshift frontier. The candidates are ideal targets for spectroscopic follow-up in Cycle-2.
URI: https://research.matf.bg.ac.rs/handle/123456789/2966
ISSN: 20418205
DOI: 10.3847/2041-8213/ac94d0
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