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Cited by 450

The DOI matches its Crossref record; 123 of the 123 references it cites were found in a registry or an index.

The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

Open access
De Looze, Ilse, Cormier, Diane, Lebouteiller, Vianney, Madden, Suzanne, Baes, Maarten, Bendo, George J., Boquien, Médéric, Boselli, Alessandro, Clements, David L., Cortese, Luca, Cooray, Asantha, Galametz, Maud, Galliano, Frédéric, Graciá-Carpio, Javier, Isaak, Kate, Karczewski, Oskar Ł., Parkin, Tara J., Pellegrini, Eric W., Rémy-Ruyer, Aurélie, Spinoglio, Luigi, Smith, Matthew W. L., Sturm, Eckhard·2014·Astronomy & Astrophysics

Abstract

Aims. We analyze the applicability of far-infrared fine-structure lines [Cii] 158 μm, [Oi] 63 μm, and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and, furthermore, extend the analysis to a broad sample of galaxies of various types and metallicities in the literature.

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Crossref · 10.1051/0004-6361/201322489

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Metadata

Authors
De Looze, I., Cormier, D., Lebouteiller, V., Madden, S., Baes, M., Bendo, G. J., Boquien, M., Boselli, A., Clements, D. L., Cortese, L., Cooray, A., Galametz, M., Galliano, F., Graciá-Carpio, J., Isaak, K., Karczewski, O. Ł., Parkin, T. J., Pellegrini, E. W., Rémy-Ruyer, A., Spinoglio, L., Smith, M. W. L., & Sturm, E.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2014-08
Volume
568
Pages
A62
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
OpenAlex
W2017609025
Cited by
450
References
123
FWCI
15.64
Type
journal article
Language
en
Open access
bronze

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The paper
De Looze, I., Cormier, D., Lebouteiller, V., Madden, S., Baes, M., Bendo, G. J., Boquien, M., Boselli, A., Clements, D. L., Cortese, L., Cooray, A., Galametz, M., Galliano, F., Graciá-Carpio, J., Isaak, K., Karczewski, O. Ł., Parkin, T. J., Pellegrini, E. W., Rémy-Ruyer, A., . . . Sturm, E. (2014). The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201322489

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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.