A massive galaxy that formed its stars at z ~ 11.

Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
14 Feb 2024
Historique:
received: 10 08 2023
accepted: 09 02 2024
medline: 15 2 2024
pubmed: 15 2 2024
entrez: 14 2 2024
Statut: aheadofprint

Résumé

The formation of galaxies by gradual hierarchical co-assembly of baryons and cold dark matter halos is a fundamental paradigm underpinning modern astrophysics[1, 2] and predicts a strong decline in the number of massive galaxies at early cosmic times[3-5]. Extremely massive quiescent galaxies (stellar masses > 10

Identifiants

DOI: 10.1038/s41586-024-07191-9 PMID: 38354832
pubmed: 38354832
doi: 10.1038/s41586-024-07191-9
pii: 10.1038/s41586-024-07191-9
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Informations de copyright

© 2024. The Author(s), under exclusive licence to Springer Nature Limited.

Auteurs

Karl Glazebrook (K)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia. kglazebrook@swin.edu.au.
ORCID: 0000-0002-3254-9044

Themiya Nanayakkara (T)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia.
ORCID: 0000-0003-2804-0648

Corentin Schreiber (C)

IBEX Innovations, Sedgefield, Stockton-on-Tees, United Kingdom.

Claudia Lagos (C)

Cosmic DAWN Center, Niels Bohr Institute, University of Copenhagen, Copenhagen N, Denmark.
ARC Centre for Excellence in All-Sky Astrophysics in 3D, Stromlo, ACT, Australia.
International Centre for Radio Astronomy Research, University of Western Australia, Crawley, WA, Australia.
ORCID: 0000-0003-3021-8564

Lalitwadee Kawinwanichakij (L)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia.

Colin Jacobs (C)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia.

Harry Chittenden (H)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia.

Gabriel Brammer (G)

Cosmic DAWN Center, Niels Bohr Institute, University of Copenhagen, Copenhagen N, Denmark.
ORCID: 0000-0003-2680-005X

Glenn G Kacprzak (GG)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia.

Ivo Labbe (I)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia.
ORCID: 0000-0002-2057-5376

Danilo Marchesini (D)

Physics and Astronomy Department, Tufts University, Medford, MA, USA.
ORCID: 0000-0001-9002-3502

Z Cemile Marsan (ZC)

Department of Physics and Astronomy, York University, Toronto, ON, Canada.
ORCID: 0000-0002-7248-1566

Pascal A Oesch (PA)

Cosmic DAWN Center, Niels Bohr Institute, University of Copenhagen, Copenhagen N, Denmark.
Department of Astronomy, University of Geneva, Versoix, Switzerland.
ORCID: 0000-0001-5851-6649

Casey Papovich (C)

Department of Physics and Astronomy, and George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, TX, USA.
ORCID: 0000-0001-7503-8482

Rhea-Silvia Remus (RS)

Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians-Universität München, München, Germany.

Kim-Vy H Tran (KH)

School of Physics, University of New South Wales, Kensington, Australia.
ARC Centre for Excellence in All-Sky Astrophysics in 3D, Stromlo, ACT, Australia.
ORCID: 0000-0001-9208-2143

James Esdaile (J)

Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia.

Angel Chandro-Gomez (A)

International Centre for Radio Astronomy Research, University of Western Australia, Crawley, WA, Australia.

Classifications MeSH