The DOI matches its Crossref record; 66 of the 66 references it cites were found in a registry or an index.
Radio Properties of Infrared‐Selected Galaxies in the IRAS 2 Jy Sample
Open accessAbstract
The radio counterparts to the IRAS Redshift Survey galaxies are identified in the NRAO VLA Sky Survey (NVSS) catalog. Our new catalog of the IR flux-limited ( S 60 μm ≥ 2 Jy) complete sample of 1809 galaxies lists accurate radio positions, redshifts, and 1.4 GHz radio and IRAS fluxes. This sample is 6 times larger in size and 5 times deeper in redshift coverage (to z ≈ 0.15) than those used in earlier studies of the radio and far-IR (FIR) properties of galaxies in the local volume. The well-known radio-FIR correlation is obeyed by the overwhelming majority (≥98%) of the IR-selected galaxies, and the radio AGNs identified by their excess radio emission constitute only about 1% of the sample, independent of the IR luminosity. These FIR-selected galaxies can account for the entire population of late-type field galaxies in the local volume, and their radio continuum may be used directly to infer the extinction-free star formation rate in most cases. Both the 1.4 GHz radio and 60 μm IR luminosity functions are reasonably well described by linear sums of two Schechter functions, one representing normal, late-type field galaxies and the other representing starbursts and other luminous IR galaxies. The integrated FIR luminosity density for the local volume is (4.8 ± 0.5) × 10 7 L ☉ Mpc -3 , less than 10% of which is contributed by the luminous IR galaxies with L FIR ≥ 10 11 L ☉ . The inferred extinction-free star formation density for the local volume is 0.015 ± 0.005 M ☉ yr -1 Mpc -3 .
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Cites
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Self-citationThe Dust Content and Opacity of Actively Star‐forming Galaxies
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The Global Schmidt Law in Star‐forming Galaxies
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Self-citationHigh-redshift galaxies in the Hubble Deep Field: colour selection and star formation history to z 4
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Cited by
Star Formation in the Milky Way and Nearby Galaxies
Kennicutt, R. C., & Evans, N. J. (2012) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125610 · Cited by 2,902
“The steep synchrotron spectrum makes this calibration strongly wavelength dependent, and most are referenced to 1.4GHz (e.g., Yun et al. 2001; Condon 1992; Bell 2003).”
BackgroundA HIGHLY CONSISTENT FRAMEWORK FOR THE EVOLUTION OF THE STAR-FORMING “MAIN SEQUENCE” FROM z ∼ 0-6
Speagle, J. S., Steinhardt, C. L., Capak, P. L., & Silverman, J. D. (2014) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/214/2/15 · Cited by 1,646
A Redshift Survey of the Submillimeter Galaxy Population
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GOODS–Herschel: an infrared main sequence for star-forming galaxies
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Metadata
- Authors
- Yun, M. S., Reddy, N. A., & Condon, J. J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2001-06-20
- Volume
- 554
- Issue
- 2
- Pages
- 803-822
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2077326407
- Cited by
- 928
- References
- 66
- FWCI
- 16.09
- Type
- journal article
- Language
- en
- Open access
- bronze
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