The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years
Journal article, 2021
Galaxy counts
Submillimeter astronomy
Luminosity function
High-redshift galaxies
Dust continuum emission
Galaxies
Galaxy evolution
Star formation
Surveys
Millimeter astronomy
Author
J. A. Zavala
The University of Texas at Austin
C. M. Casey
The University of Texas at Austin
S. M. Manning
The University of Texas at Austin
M. Aravena
Diego Portales University
M. Bethermin
Aix Marseille University
K. I. Caputi
University of Groningen
University of Copenhagen
D. L. Clements
Imperial College London
E. da Cunha
University of Western Australia
P. Drew
The University of Texas at Austin
S. L. Finkelstein
The University of Texas at Austin
S. Fujimoto
University of Copenhagen
C. Hayward
Flatiron Institute
J. Hodge
Leiden University
J. S. Kartaltepe
Rochester Institute of Technology
Kirsten Kraiberg Knudsen
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
A. M. Koekemoer
Space Telescope Science Institute (STScI)
A. S. Long
University of California at Irvine (UCI)
G. E. Magdis
National Observatory of Athens
University of Copenhagen
Technical University of Denmark (DTU)
A. W. S. Man
University of Toronto
G. Popping
European Southern Observatory Santiago
D. Sanders
University of Hawaii
N. Scoville
California Institute of Technology (Caltech)
K. Sheth
National Aeronautics and Space Administration (NASA)
J. Staguhn
National Aeronautics and Space Administration (NASA)
Johns Hopkins University
S. Toft
University of Copenhagen
E. Treister
Pontificia Universidad Catolica de Chile
J. D. Vieira
University of Illinois
M. S. Yun
University of Massachusetts
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 909 2 165Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
Probability Theory and Statistics
Geosciences, Multidisciplinary
DOI
10.3847/1538-4357/abdb27