The radio spectral energy distribution and star-formation rate calibration in galaxies
We study the spectral energy distribution (SED) of the radio continuum (RC) emission from the Key Insight in Nearby Galaxies Emitting in Radio (KINGFISHER) sample of nearby galaxies to understand the energetics and origin of this emission. Effelsberg multi-wavelength observations at 1.4, 4.8, 8.4, a...
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| Main Authors: | , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
2017 February 21
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| In: |
The astrophysical journal
Year: 2017, Volume: 836, Issue: 2, Pages: 185 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/1538-4357/836/2/185 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/1538-4357/836/2/185
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| Author Notes: | F.S. Tabatabaei, E. Schinnerer, M. Krause, G. Dumas, S. Meidt, A. Damas-Segovia, R. Beck, E.J. Murphy, D.D. Mulcahy, B. Groves, A. Bolatto, D. Dale, M. Galametz, K. Sandstrom, M. Boquien, D. Calzetti, R.C. Kennicutt, L.K. Hunt, I. De Looze, and E.W. Pellegrini |
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The radio spectral energy distribution and star formation rate calibration in galaxies
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