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  5. A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging
 

A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging

Journal
THE ASTROPHYSICAL JOURNAL LETTERS  
Date Issued
2022
Author(s)
Finkelstein, Steven L.
•
Bagley, Micaela B.
•
Arrabal Haro, Pablo
•
DICKINSON, MARK  
•
Ferguson, Henry C.
•
Kartaltepe, Jeyhan S.
•
Papovich, Casey
•
Burgarella, Denis
•
Kocevski, Dale D.
•
Huertas-Company, Marc
•
Iyer, Kartheik G.
•
Koekemoer, Anton M.
•
Larson, Rebecca L.
•
Pérez-González, Pablo G.
•
Rose, Caitlin
•
Tacchella, Sandro
•
Wilkins, Stephen M.
•
Chworowsky, Katherine
•
Medrano, Aubrey
•
Morales, Alexa M.
•
Somerville, Rachel S.
•
Yung, L. Y. Aaron
•
FONTANA, Adriano  
•
Giavalisco, Mauro
•
GRAZIAN, Andrea  
•
Grogin, Norman A.
•
Kewley, Lisa J.
•
Kirkpatrick, Allison
•
Kurczynski, Peter
•
Lotz, Jennifer M.
•
PENTERICCI, Laura  
•
Pirzkal, Nor
•
Ravindranath, Swara
•
Ryan, Russell E.
•
Trump, Jonathan R.
•
Yang, Guang
•
Almaini, Omar
•
Amorín, Ricardo O.
•
Annunziatella, Marianna
•
Backhaus, Bren E.
•
Barro, Guillermo
•
Behroozi, Peter
•
Bell, Eric F.
•
Bhatawdekar, Rachana
•
BISIGELLO, Laura  
•
Bromm, Volker
•
Buat, Véronique
•
Buitrago, Fernando
•
CALABRO', Antonello  
•
Casey, Caitlin M.
•
CASTELLANO, Marco  
•
Chávez Ortiz, Óscar A.
•
Ciesla, Laure
•
Cleri, Nikko J.
•
Cohen, Seth H.
•
Cole, Justin W.
•
Cooke, Kevin C.
•
Cooper, M. C.
•
Cooray, Asantha R.
•
COSTANTIN, LUCA
•
Cox, Isabella G.
•
Croton, Darren
•
Daddi, Emanuele
•
Davé, Romeel
•
de La Vega, Alexander
•
Dekel, Avishai
•
Elbaz, David
•
Estrada-Carpenter, Vicente
•
Faber, Sandra M.
•
Fernández, Vital
•
Finkelstein, Keely D.
•
Freundlich, Jonathan
•
Fujimoto, Seiji
•
García-Argumánez, Ángela
•
Gardner, Jonathan P.
•
Gawiser, Eric
•
Gómez-Guijarro, Carlos
•
Guo, Yuchen
•
Hamblin, Kurt
•
Hamilton, Timothy S.
•
Hathi, Nimish P.
•
Holwerda, Benne W.
•
HIRSCHMANN, Michaela Monika  
•
Hutchison, Taylor A.
•
Jaskot, Anne E.
•
Jha, Saurabh W.
•
Jogee, Shardha
•
Juneau, Stéphanie
•
Jung, Intae
•
Kassin, Susan A.
•
Le Bail, Aurélien
•
Leung, Gene C. K.
•
Lucas, Ray A.
•
Magnelli, Benjamin
•
Mantha, Kameswara Bharadwaj
•
Matharu, Jasleen
•
McGrath, Elizabeth J.
•
McIntosh, Daniel H.
•
MERLIN, Emiliano  
•
Mobasher, Bahram
•
Newman, Jeffrey A.
•
Nicholls, David C.
•
Pandya, Viraj
•
Rafelski, Marc
•
Ronayne, Kaila
•
SANTINI, Paola  
•
Seillé, Lise-Marie
•
Shah, Ekta A.
•
Shen, Lu
•
Simons, Raymond C.
•
Snyder, Gregory F.
•
Stanway, Elizabeth R.
•
Straughn, Amber N.
•
Teplitz, Harry I.
•
Vanderhoof, Brittany N.
•
Vega-Ferrero, Jesús
•
Wang, Weichen
•
Weiner, Benjamin J.
•
Willmer, Christopher N. A.
•
Wuyts, Stijn
•
Zavala, Jorge A.
•
Ceers Team
DOI
10.3847/2041-8213/ac966e
Abstract
We report the discovery of a candidate galaxy with a photo-z of z ~ 12 in the first epoch of the James Webb Space Telescope (JWST) Cosmic Evolution Early Release Science Survey. Following conservative selection criteria, we identify a source with a robust z phot = ${11.8}_{-0.2}^{+0.3}$ (1σ uncertainty) with m F200W = 27.3 and ≳7σ detections in five filters. The source is not detected at λ < 1.4 μm in deep imaging from both Hubble Space Telescope (HST) and JWST and has faint ~3σ detections in JWST F150W and HST F160W, which signal a Lyα break near the red edge of both filters, implying z ~ 12. This object (Maisie's Galaxy) exhibits F115W - F200W > 1.9 mag (2σ lower limit) with a blue continuum slope, resulting in 99.6% of the photo-z probability distribution function favoring z > 11. All data-quality images show no artifacts at the candidate's position, and independent analyses consistently find a strong preference for z > 11. Its colors are inconsistent with Galactic stars, and it is resolved (r h = 340 ± 14 pc). Maisie's Galaxy has log M */M ⊙ ~ 8.5 and is highly star-forming (log sSFR ~ -8.2 yr-1), with a blue rest-UV color (β ~ -2.5) indicating little dust, though not extremely low metallicity. While the presence of this source is in tension with most predictions, it agrees with empirical extrapolations assuming UV luminosity functions that smoothly decline with increasing redshift. Should follow-up spectroscopy validate this redshift, our universe was already aglow with galaxies less than 400 Myr after the Big Bang.
Volume
940
Issue
2
Start page
L55
Uri
http://hdl.handle.net/20.500.12386/36453
Url
https://iopscience.iop.org/article/10.3847/2041-8213/ac966e
https://api.elsevier.com/content/abstract/scopus_id/85144295804
Issn Identifier
2041-8205
Ads BibCode
2022ApJ...940L..55F
Rights
open.access
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Format

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