The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years
Journal article, 2021
Luminosity function
Galaxy evolution
Star formation
Dust continuum emission
High-redshift galaxies
Submillimeter astronomy
Surveys
Millimeter astronomy
Galaxy counts
Galaxies
Author
J. A. Zavala
University of Texas
C. M. Casey
University of Texas
S. M. Manning
University of Texas
M. Aravena
Diego Portales University
M. Bethermin
Aix Marseille University
K. I. Caputi
University of Copenhagen
University of Groningen
D. L. Clements
Imperial College London
E. da Cunha
University of Western Australia
P. Drew
University of Texas
S. L. Finkelstein
University of Texas
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
G. E. Magdis
Technical University of Denmark (DTU)
National Observatory of Athens
University of Copenhagen
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
Johns Hopkins University
National Aeronautics and Space Administration (NASA)
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