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dc.contributor.authorHainline, Kevin N.
dc.contributor.authorJohnson, Benjamin D.
dc.contributor.authorRobertson, Brant
dc.contributor.authorTacchella, Sandro
dc.contributor.authorHelton, Jakob M.
dc.contributor.authorSun, Fengwu
dc.contributor.authorEisenstein, Daniel J.
dc.contributor.authorSimmonds, Charlotte
dc.contributor.authorTopping, Michael W.
dc.contributor.authorWhitler, Lily
dc.contributor.authorWillmer, Christopher N. A.
dc.contributor.authorRieke, Marcia
dc.contributor.authorSuess, Katherine A.
dc.contributor.authorHviding, Raphael E.
dc.contributor.authorCameron, Alex J.
dc.contributor.authorAlberts, Stacey
dc.contributor.authorBaker, William M.
dc.contributor.authorBhatawdekar, Rachana
dc.contributor.authorBoyett, Kristan
dc.contributor.authorBunker, Andrew J.
dc.contributor.authorCarniani, Stefano
dc.contributor.authorCharlot, Stephane
dc.contributor.authorChen, Zuyi
dc.contributor.authorCurti, Mirko
dc.contributor.authorCurtis-Lake, Emma
dc.contributor.authorD'Eugenio, Francesco
dc.contributor.authorEgami, Eiichi
dc.contributor.authorEndsley, Ryan
dc.contributor.authorHausen, Ryan
dc.contributor.authorJi, Zhiyuan
dc.contributor.authorLooser, Tobias J.
dc.contributor.authorLyu, Jianwei
dc.contributor.authorMaiolino, Roberto
dc.contributor.authorNelson, Erica
dc.contributor.authorPuskas, David
dc.contributor.authorRawle, Tim
dc.contributor.authorSandles, Lester
dc.contributor.authorSaxena, Aayush
dc.contributor.authorSmit, Renske
dc.contributor.authorStark, Daniel P.
dc.contributor.authorWilliams, Christina C.
dc.contributor.authorWillott, Chris
dc.contributor.authorWitstok, Joris
dc.date.accessioned2024-03-25T13:33:34Z
dc.date.available2024-03-25T13:33:34Z
dc.date.issued2024-03-18
dc.identifier.citationHainline , K N , Johnson , B D , Robertson , B , Tacchella , S , Helton , J M , Sun , F , Eisenstein , D J , Simmonds , C , Topping , M W , Whitler , L , Willmer , C N A , Rieke , M , Suess , K A , Hviding , R E , Cameron , A J , Alberts , S , Baker , W M , Bhatawdekar , R , Boyett , K , Bunker , A J , Carniani , S , Charlot , S , Chen , Z , Curti , M , Curtis-Lake , E , D'Eugenio , F , Egami , E , Endsley , R , Hausen , R , Ji , Z , Looser , T J , Lyu , J , Maiolino , R , Nelson , E , Puskas , D , Rawle , T , Sandles , L , Saxena , A , Smit , R , Stark , D P , Williams , C C , Willott , C & Witstok , J 2024 , ' The Cosmos in its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N ' , The Astrophysical Journal , vol. 964 , no. 1 , 71 . https://doi.org/10.3847/1538-4357/ad1ee4
dc.identifier.issn0004-637X
dc.identifier.otherArXiv: http://arxiv.org/abs/2306.02468v3
dc.identifier.otherORCID: /0000-0002-9551-0534/work/156079590
dc.identifier.urihttp://hdl.handle.net/2299/27619
dc.description© 2024. The Author(s). Published by the American Astronomical Society. This is an open access article distributed under the Creative Commons Attribution License, to view a copy of the license, see: https://creativecommons.org/licenses/by/4.0/
dc.description.abstractWe present a catalog of 717 candidate galaxies at z > 8 selected from 125 square arcmin of NIRCam imaging as part of the JWST Advanced Deep Extragalactic Survey (JADES). We combine the full JADES imaging data set with data from the JWST Extragalactic Medium Survey and First Reionization Epoch Spectroscopic COmplete Survey (FRESCO) along with extremely deep existing observations from Hubble Space Telescope (HST)/Advanced Camera for Surveys (ACS) for a final filter set that includes 15 JWST/NIRCam filters and five HST/ACS filters. The high-redshift galaxy candidates were selected from their estimated photometric redshifts calculated using a template-fitting approach, followed by visual inspection from seven independent reviewers. We explore these candidates in detail, highlighting interesting resolved or extended sources, sources with very red long-wavelength slopes, and our highest-redshift candidates, which extend to z phot ∼ 18. Over 93% of the sources are newly identified from our deep JADES imaging, including 31 new galaxy candidates at z phot > 12. We also investigate potential contamination by stellar objects, and do not find strong evidence from spectral energy distribution fitting that these faint high-redshift galaxy candidates are low-mass stars. Using 42 sources in our sample with measured spectroscopic redshifts from NIRSpec and FRESCO, we find excellent agreement to our photometric redshift estimates, with no catastrophic outliers and an average difference of 〈Δz = z phot − z spec〉 = 0.26. These sources comprise one of the most robust samples for probing the early buildup of galaxies within the first few hundred million years of the Universe’s history.en
dc.format.extent35
dc.format.extent4873825
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.subjectastro-ph.GA
dc.subjectAstronomy and Astrophysics
dc.subjectSpace and Planetary Science
dc.titleThe Cosmos in its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-Nen
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85188115603&partnerID=8YFLogxK
rioxxterms.versionofrecord10.3847/1538-4357/ad1ee4
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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