An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models

Journal: The Astrophysical Journal Letters

Published: 2020-02-05

DOI: 10.3847/2041-8213/ab5b9f

Affiliations: 13

Authors: 20

Go to article
Institutions Share
Department of Physics and Astronomy, UCR, United States of America (USA) 0.20
Tufts Department of Physics and Astronomy, United States of America (USA) 0.20
Department of Physics and Astronomy, York University, Canada 0.10
Center for Cosmology, UCI, United States of America (USA) 0.05
W. M. Keck Observatory, United States of America (USA) 0.05
Department of Astrophysical Sciences, Princeton University, United States of America (USA) 0.05
INAF - Astronomical Observatory of Capodimonte, Italy 0.05
Swinburne Centre for Astrophysics and Supercomputing (CAS), Australia 0.05
Department of Physical Sciences, UNAB, Chile 0.05
INAF - Astronomical Observatory of Trieste (OATs), Italy 0.05
INAF - Astronomical Observatory of Brera (OAB), Italy 0.05
Leiden Observatory (STRW), Netherlands 0.05
European Southern Observatory (ESO), Germany 0.05

Return

Except where otherwise noted © 2021 Springer Nature Limited. All Rights Reserved.
partner of AGORA, HINARI, OARE, INASP, ORCID, CrossRef and COUNTER