The VLA-COSMOS perspective on the infrared-radio relation I. New constraints on 
selection biases and the non-evolution of the infrared/radio properties of 
star-forming and active galactic nucleus galaxies at intermediate and high 
redshift

Sargent, M. T.; Schinnerer, E.; Murphy, E.; Aussel, H.; Le Floc'h, E.; Frayer, D. T.; Martínez-Sansigre, A.; Oesch, P.; Salvato, M.; Smolčić, V.; Zamorani, G.; Brusa, M.; Cappelluti, N.; Carilli, C. L.; Carollo, C. M.; Ilbert, O.; Kartaltepe, J.; Koekemoer, A. M.; Lilly, S. J.; Sanders, D. B.; Scoville, N. Z.

doi:10.1088/0067-0049/186/2/341

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The VLA-COSMOS perspective on the infrared-radio relation I. New constraints on selection biases and the non-evolution of the infrared/radio properties of star-forming and active galactic nucleus galaxies at intermediate and high redshift

Sargent, M. T., Schinnerer, E., Murphy, E., Aussel, H., Le Floc'h, E., Frayer, D. T., et al. (2010). The VLA-COSMOS perspective on the infrared-radio relation I. New constraints on selection biases and the non-evolution of the infrared/radio properties of star-forming and active galactic nucleus galaxies at intermediate and high redshift. The Astrophysical Journal. Supplement Series, 186(2), 341-377. doi:10.1088/0067-0049/186/2/341.

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Urheber:
Sargent, M. T.¹, Autor
Schinnerer, E.¹, Autor
Murphy, E.¹, Autor
Aussel, H.¹, Autor
Le Floc'h, E.¹, Autor
Frayer, D. T.¹, Autor
Martínez-Sansigre, A.¹, Autor
Oesch, P.¹, Autor
Salvato, M.^{2, 3}, Autor
Smolčić, V.¹, Autor
Zamorani, G.¹, Autor
Brusa, M.¹, Autor
Cappelluti, N.¹, Autor
Carilli, C. L.¹, Autor
Carollo, C. M.¹, Autor
Ilbert, O.¹, Autor
Kartaltepe, J.¹, Autor
Koekemoer, A. M.¹, Autor
Lilly, S. J.¹, Autor
Sanders, D. B.¹, Autor
Scoville, N. Z.¹, Autor mehr..

Affiliations:
1Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany; Spitzer Science Center, MC 314-6, California Institute of Technology, Pasadena, CA 91125, USA; AIM Unité Mixte de Recherche CEA CNRS Université Paris VII UMR n158, France; CEA-Saclay, Service d'Astrophysique, F-91191 Gif-sur-Yvette, France; Institute for Astronomy, 2680 Woodlawn Dr., University of Hawaii, Honolulu, HI 96822, USA; Infrared Processing and Analysis Center, California Institute of Technology 100-22, Pasadena, CA 91125, USA; Astrophysics, Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK; Department of Physics, ETH Zurich, CH-8093 Zurich, Switzerland; California Institute of Technology, MC 105-24, 1200 East California Boulevard, Pasadena, CA 91125, USA; INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna, Italy; Max Planck Institut für Extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching bei München, Germany; National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801-0387, USA; Laboratoire d'Astrophysique de Marseille, BP 8, Traverse du Siphon, F-13376 Marseille Cedex 12, France; National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85726, USA; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA, ou_persistent22
2Group 'Astrophysics and Laboratory Plasma Studies' (ALPS), Max Planck Institute for Plasma Physics, Max Planck Society, ou_1856335
3Office of the Director (DI), Max Planck Institute for Plasma Physics, Max Planck Society, ou_1856325