201. Herschel-ATLAS: The far-infrared--radio correlation at z<0.5
- Author
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Jarvis, Matt J., Smith, D. J. B., Bonfield, D. G., Hardcastle, M. J., Falder, J. T., Stevens, J. A., Ivison, R. J., Auld, R., Baes, M., Baldry, I. K., Bamford, S. P., Bourne, N., Buttiglione, S., Cava, A, Cooray, A., Dariush, A., de Zotti, G., Dunlop, J. S., Dunne, L., Dye, S., Eales, S., Fritz, J., Hill, D. T., Hopwood, R., Hughes, D. H., Ibar, E., Jones, D. H., Kelvin, L., Lawrence, A., Leeuw, L., Loveday, J., Maddox, S. J., Michalowski, M. J., Negrello, M., Norberg, P., Pohlen, M., Prescott, M., Rigby, E. E., Robotham, A., Rodighiero, G., Scott, D., Sharp, R., Temi, P., Thompson, M. A., van der Werf, P., Vlahakis, C., and White, G.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared--radio correlation over the redshift range 0
5sigma sources in the Herschel-ATLAS Science Demonstration Field and cross-matching these data with radio data from the Faint Images of the Radio Sky at Twenty-Centimetres (FIRST) survey and the NRAO VLA Northern Sky Survey (NVSS), we obtain 104 radio counterparts to the Herschel sources. With these data we find no evidence for evolution in the far-infrared--radio correlation over the redshift range 0 - Published
- 2010
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