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Cited by 959

The DOI matches its Crossref record; 305 of the 305 references it cites were found in a registry or an index.

Modeling the Panchromatic Spectral Energy Distributions of Galaxies

Open access
Conroy, Charlie·2013·Annual Review of Astronomy and Astrophysics

Abstract

The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical property of the system, including the star-formation history, metal content, abundance pattern, dust mass, grain size distribution, star-dust geometry, and interstellar radiation field. The principal goal of stellar population synthesis (SPS) is to extract these variables from observed SEDs. In this review I provide an overview of the SPS technique and discuss what can be reliably measured from galaxy SEDs. Topics include stellar masses, star-formation rates and histories, metallicities and abundance patterns, dust properties, and the stellar initial mass function.

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Metadata

Authors
Conroy, C.
Venue
Annual Review of Astronomy and Astrophysics
Published
2013-08-18
Volume
51
Issue
1
Pages
393-455
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2121516375
Cited by
959
References
305
FWCI
3.02
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Modeling the Panchromatic Spectral Energy Distributions of Galaxies. https://app.cochat.ai/papers/10.1146/annurev-astro-082812-141017
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Conroy, C. (2013). Modeling the Panchromatic Spectral Energy Distributions of Galaxies. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev-astro-082812-141017

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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.