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The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5 σ Source Catalog and Redshift Distribution

Title: The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5 σ Source Catalog and Redshift Distribution
Authors: Long, Arianna, S; Casey, Caitlin, M; Mckinney, Jed; Zavala, Jorge, A; Akins, Hollis, B; Cooper, Olivia, R; Lambrides, Erini, L; Franco, Maximilien; Aravena, Manuel; Bethermin, Matthieu; Caputi, Karina; Champagne, Jaclyn, B; Clements, D, L; da Cunha, Elisabete; Faisst, Andreas, L; Gentile, Fabrizio; Hodge, Jacqueline; Man, Allison, W S; Manning, Sinclaire, M; Sanders, David, B; Talia, Margherita; Treister, Ezequiel; Brammer, Gabriel; Brusa, Marcella; Finkelstein, Steven, L; Fujimoto, Seiji; Hayward, Christopher, C; Ilbert, Olivier; Jolly, Jean-Baptiste; Kartaltepe, Jeyhan, S; Knudsen, Kirsten; Koekemoer, Anton, M; Liu, Daizhong; Magdis, Georgios; Mccracken, Henry, Joy; Rhodes, Jason; Robertson, Brant, E; Scoville, Nick; Sheth, Kartik; Smolcic, Vernesa; Spilker, Justin; Taniguchi, Yoshiaki; Toft, Sune; Urry, C. Megan; Yun, Min
Contributors: Department of Physics and Astronomy Washington; Howard University; Department of Astronomy and Texas Center for Cosmology and Astroparticle Physics, The University of Texas at Austin, Austin, TX 78712-1083, USA; National Astronomical Observatory of Japan (NAOJ); Department of Astronomy Austin; University of Texas at Austin Austin; epartment of Astronomy, The University of Texas at Austin, 2515 Speedway Blvd Stop C1400, Austin, TX 78712, USA; NASA Goddard Space Flight Center (GSFC); Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)); Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité); Instituto de Estudios Astrofísicos Santiago; Universidad Diego Portales Santiago - Chili (UDP); Observatoire astronomique de Strasbourg (ObAS); Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS); Cosmic Dawn Center (DAWN); Kapteyn Astronomical Institute Groningen; University of Groningen Groningen; Steward Observatory; University of Arizona; University of Warwick Coventry; International Centre for Radio Astronomy Research (ICRAR); The University of Western Australia (UWA)-Government of Western Australia-Curtin University; California Institute of Technology (CALTECH); Max-Planck-Institut für Astronomie = Max Planck Institute for Astronomy (MPIA); Max-Planck-Gesellschaft; UBC Department of Physics and Astronomy - University of British Columbia; UBC; Dunlap Institute for Astronomy and Astrophysics Toronto; University of Toronto; Institute for Astronomy Honolulu; University of Hawai‘i Mānoa (UHM); INAF – Osservatorio di Astrofisica e Scienza dello Spazio, Via Gobetti 93/3, I-40129, Bologna, Italy; Pontificia Universidad Católica de Chile = Pontifical Catholic University of Chile Santiago (PUC); Niels Bohr Institute Copenhagen (NBI); Faculty of Science Copenhagen; Københavns Universitet = University of Copenhagen = Université de Copenhague (UCPH)-Københavns Universitet = University of Copenhagen = Université de Copenhague (UCPH); National Space Institute Lyngby (DTU Space); Danmarks Tekniske Universitet = Technical University of Denmark (DTU); Osservatorio di Astrofisica e Scienza dello Spazio di Bologna; Center for Computational Astrophysics New York; Flatiron Institute; Simons Foundation-Simons Foundation; Laboratoire d'Astrophysique de Marseille (LAM); Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS); Max-Planck-Institut für Extraterrestrische Physik (MPE); Rochester Institute of Technology (RIT); Chalmers University of Technology Gothenburg, Sweden; Space Telescope Science Institute (STSci); Institut d'Astrophysique de Paris (IAP); Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); Jet Propulsion Laboratory (JPL); NASA-California Institute of Technology (CALTECH); Department of Astronomy and Astrophysics, University of California, Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA; Spitzer Science Center, California Institute of Technology, Pasadena; NASA Headquarters; NASA, Space Telescope Science Institute, programme de bourses NASA Hubble Fellowship subventions n° HST-HF2-51511 et HST-HF2-51484, Association of Universities for Research in Astronomy, Inc., pour la NASA, sous contrat NAS5-26555; CER, subvention ERC Consolidator Grant 101088676 (« VOYAJ »), subvention PRIN MIUR 2017-20173ML3WW_001 « Ouvrir la fenêtre ALMA sur l'évolution cosmique du gaz,des étoiles et des trous noirs supermassifs ».; JSPS, subvention JSPS KAKENHI n° KG23K13150; Programme ANID Basal (FB210003 CATA ) etFONDECYT (subventions régulières 1190818 et 1200495); Contrat de chercheur postdoctoral JWST Arizona/Steward en galaxies précoces et réionisation (JASPER) à l'Université d'Arizona; Conseil de recherches en sciences naturelles et en génie du Canada (CRSNG), subvention n° RGPIN-2021-03046.; NRAO; JWST
Source: ISSN: 0004-637X.
Publisher Information: CCSD; American Astronomical Society
Publication Year: 2026
Subject Terms: Astrophysics - Astrophysics of Galaxies; Redshift surveys; High-redshift galaxies; Infrared galaxies; Submillimeter astronomy; [SDU]Sciences of the Universe [physics]; [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]; [SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]
Description: International audience ; One of the greatest challenges in galaxy evolution over the last decade has been constraining the prevalence of heavily dust-obscured galaxies in the early Universe. At z > 3, these galaxies are increasingly rare, and difficult to identify, as they are interspersed among the more numerous dust-obscured galaxy population at z = 1-3, making
Document Type: article in journal/newspaper
Language: English
DOI: 10.3847/1538-4357/ae2fda
Availability: https://insu.hal.science/insu-05537910; https://insu.hal.science/insu-05537910v1/document; https://insu.hal.science/insu-05537910v1/file/Long_2026_ApJ_999_47.pdf; https://doi.org/10.3847/1538-4357/ae2fda
Rights: https://creativecommons.org/licenses/by/4.0/ ; info:eu-repo/semantics/OpenAccess
Accession Number: edsbas.162EB3C9
Database: BASE