Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2966
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dc.contributor.authorCastellano, Marcoen_US
dc.contributor.authorFontana, Adrianoen_US
dc.contributor.authorTreu, Tommasoen_US
dc.contributor.authorSantini, Paolaen_US
dc.contributor.authorMerlin, Emilianoen_US
dc.contributor.authorLeethochawalit, Nichaen_US
dc.contributor.authorTrenti, Micheleen_US
dc.contributor.authorVanzella, Erosen_US
dc.contributor.authorMeštrić, Urošen_US
dc.contributor.authorBonchi, Andreaen_US
dc.contributor.authorBelfiori, Davideen_US
dc.contributor.authorNonino, Marioen_US
dc.contributor.authorParis, Diegoen_US
dc.contributor.authorPolenta, Gianlucaen_US
dc.contributor.authorRoberts-Borsani, Guidoen_US
dc.contributor.authorBoyett, Kristanen_US
dc.contributor.authorBradač, Marušaen_US
dc.contributor.authorCalabrò, Antonelloen_US
dc.contributor.authorGlazebrook, Karlen_US
dc.contributor.authorGrillo, Claudioen_US
dc.contributor.authorMascia, Saraen_US
dc.contributor.authorMason, Charlotteen_US
dc.contributor.authorMercurio, Amataen_US
dc.contributor.authorMorishita, Takahiroen_US
dc.contributor.authorNanayakkara, Themiyaen_US
dc.contributor.authorPentericci, Lauraen_US
dc.contributor.authorRosati, Pieroen_US
dc.contributor.authorVulcani, Benedettaen_US
dc.contributor.authorWang, Xinen_US
dc.contributor.authorYang, Lilanen_US
dc.date.accessioned2025-12-03T11:34:34Z-
dc.date.available2025-12-03T11:34:34Z-
dc.date.issued2022-10-01-
dc.identifier.issn20418205-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2966-
dc.description.abstractWe 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 <inf>phot</inf> ≥ 9. In particular, we identify two bright candidates at M <inf>UV</inf> ≃ −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.en_US
dc.language.isoenen_US
dc.publisherIOP Scienceen_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.titleEarly Results from GLASS-JWST. III. Galaxy Candidates at z ∼9-15en_US
dc.typeArticleen_US
dc.identifier.doi10.3847/2041-8213/ac94d0-
dc.identifier.scopus2-s2.0-85141240419-
dc.identifier.isi000869458300001-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85141240419-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn2041-8205en_US
dc.description.rankM21aen_US
dc.relation.firstpageL15en_US
dc.relation.volume938en_US
dc.relation.issue2en_US
item.openairetypeArticle-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-0441-8629-
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