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Cited by 168

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Star Formation in the Nearby Universe: The Ultraviolet and Infrared Points of View

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Iglesias‐Paramo, J., Buat, V., Takeuchi, T. T., Xu, K., Boissier, S., Boselli, A., Burgarella, D., Madore, B. F., Gil de Paz, A., Bianchi, L., Barlow, T. A., Byun, Y.‐I., Donas, J., Forster, K., Friedman, P. G., Heckman, T. M., Jelinski, P. N., Lee, Y.‐W., Malina, R. F., Martin, D. C., Milliard, B., Morrissey, P. F., Neff, S. G., Rich, R. M., Schiminovich, D., Seibert, M., Siegmund, O. H. W., Small, T., Szalay, A. S., Welsh, B. Y., Wyder, T. K.·2006·The Astrophysical Journal Supplement Series

Abstract

This work presents the main ultraviolet (UV) and far-infrared (FIR) properties of two samples of nearby galaxies selected from the GALEX (λ = 2315 Å, hereafter NUV) and IRAS (λ = 60 μm) surveys, respectively. They are built in order to obtain detection at both wavelengths for most of the galaxies. Star formation rate (SFR) estimators based on the UV and FIR emissions are compared. Systematic differences are found between the SFR estimators for individual galaxies based on the NUV fluxes corrected for dust attenuation and on the total IR luminosity. A combined estimator based on NUV and IR luminosities seems to be the best proxy over the whole range of values of SFR. Although both samples present similar average values of the birthrate parameter b , their star-formation-related properties are substantially different: NUV-selected galaxies tend to show larger values of b for lower masses, SFRs, and dust attenuation, supporting previous scenarios of star formation history (SFH). Conversely, about 20% of the FIR-selected galaxies show high values of b , SFR, and NUV attenuation. These galaxies, most of them being LIRGs and ULIRGs, break down the downsizing picture of SFH; however, their relative contribution per unit volume is small in the local universe. Finally, the cosmic SFR density of the local universe is estimated in a consistent way from the NUV and IR luminosities.

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Metadata

Authors
Iglesias‐Paramo, J., Buat, V., Takeuchi, T. T., Xu, K., Boissier, S., Boselli, A., Burgarella, D., Madore, B. F., Gil de Paz, A., Bianchi, L., Barlow, T. A., Byun, Y. ‐., Donas, J., Forster, K., Friedman, P. G., Heckman, T. M., Jelinski, P. N., Lee, Y. ‐., Malina, R. F., Martin, D. C., Milliard, B., Morrissey, P. F., Neff, S. G., Rich, R. M., Schiminovich, D., Seibert, M., Siegmund, O. H. W., Small, T., Szalay, A. S., Welsh, B. Y., & Wyder, T. K.
Venue
The Astrophysical Journal Supplement Series
Published
2006-05
Volume
164
Issue
1
Pages
38-51
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W2157441368
Cited by
168
References
1
FWCI
7.52
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Star Formation in the Nearby Universe: The Ultraviolet and Infrared Points of View. https://app.cochat.ai/papers/10.1086/502628
The paper
Iglesias‐Paramo, J., Buat, V., Takeuchi, T. T., Xu, K., Boissier, S., Boselli, A., Burgarella, D., Madore, B. F., Gil de Paz, A., Bianchi, L., Barlow, T. A., Byun, Y. ‐., Donas, J., Forster, K., Friedman, P. G., Heckman, T. M., Jelinski, P. N., Lee, Y. ‐., Malina, R. F., . . . Wyder, T. K. (2006). Star Formation in the Nearby Universe: The Ultraviolet and Infrared Points of View. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/502628

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

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