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Cited by 829

The DOI matches its Crossref record; 179 of the 179 references it cites were found in a registry or an index.

The Dust Opacity of Star‐forming Galaxies

Open access
Calzetti, Daniela·2001·Publications of the Astronomical Society of the Pacific

Abstract

Presence of dust in galaxies removes half or more of the stellar energy from the UV-optical budget of the Universe and has profound impact on our understanding of how galaxies evolve. Measures of opacity in local galaxies are reviewed together with widely used theoretical and empirical methods for quantifying its effects. Existing evidence shows that the dust content of nearby galaxies depends not only on their morphology, but also on their luminosity and activity level. A digression is devoted to starbursts in view of their potential relevance for measures of opacity in distant galaxies. Scarcity of coherent multiwavelength datasets hampers our ability to derive reliable obscuration estimates in intermediate and high redshift galaxies. This, in turn, limits the reliability of inferred physical quantities, such as star formation rates, stellar population ages, galaxy luminosity functions, and others.

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Metadata

Authors
Calzetti, D.
Venue
Publications of the Astronomical Society of the Pacific
Published
2001-12
Volume
113
Issue
790
Pages
1449-1485
ISSN
  • 0004-6280 (ISSN-L)
  • 1538-3873
OpenAlex
W1992881800
Cited by
829
References
179
FWCI
15.07
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The Dust Opacity of Star‐forming Galaxies. https://app.cochat.ai/papers/10.1086/324269
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Calzetti, D. (2001). The Dust Opacity of Star‐forming Galaxies. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/324269

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.