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Cited by 800

The DOI matches its Crossref record; 575 of the 575 references it cites were found in a registry or an index.

Dusty star-forming galaxies at high redshift

Open access
Casey, Caitlin M., Narayanan, Desika, Cooray, Asantha·2014·Physics Reports
DOI 10.1016/j.physrep.2014.02.009
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Abstract

Abstract Far-infrared and submillimeter wavelength surveys have now established the important role of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of massive galaxies in the Universe. The brightest of these galaxies have infrared luminosities in excess of 10 13 L ⊙ with implied star-formation rates of thousands of solar masses per year. They represent the most intense starbursts in the Universe, yet many are completely optically obscured. Their easy detection at submm wavelengths is due to dust heated by ultraviolet radiation of newly forming stars. When summed up, all of the dusty, star-forming galaxies in the Universe produce an infrared radiation field that has an equal energy density as the direct starlight emission from all galaxies visible at ultraviolet and optical wavelengths. The bulk of this infrared extragalactic background light emanates from galaxies as diverse as gas-rich disks to mergers of intense starbursting galaxies. Major advances in far-infrared instrumentation in recent years, both space-based and ground-based, has led to the detection of nearly a million DSFGs, yet our understanding of the underlying astrophysics that govern the start and end of the dusty starburst phase is still in nascent stage. This review is aimed at summarizing the current status of DSFG studies, focusing especially on the detailed characterization of the best-understood subset (submillimeter galaxies, who were summarized in the last review of this field over a decade ago, Blain et al., 2002), but also the selection and characterization of more recently discovered DSFG populations. We review DSFG population statistics, their physical properties including dust, gas and stellar contents, their environments, and current theoretical models related to the formation and evolution of these galaxies.

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Metadata

Authors
Casey, C. M., Narayanan, D., & Cooray, A.
Venue
Physics Reports
Publisher
Elsevier BV
Published
2014-08
Volume
541
Issue
2
Pages
45-161
ISSN
0370-1573 (ISSN-L)
DOI
10.1016/j.physrep.2014.02.009
OpenAlex
W2025105301
Cited by
800
References
575
FWCI
35.29
Type
journal article
Language
en
Open access
green

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