Volume 597, January 2017
|Number of page(s)||1|
|Section||Cosmology (including clusters of galaxies)|
|Published online||20 December 2016|
Hidden starbursts and active galactic nuclei at 0 < z < 4 from the Herschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback (Corrigendum)⋆
1 Aix-Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, France
2 Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu – CNRS – Université Paris Diderot, CE-Saclay, pt courrier 131, 91191 Gif-sur-Yvette, France
3 Department of Physics, University of California, Davis, 1 Shields Avenue, Davis, CA 95616, USA
4 INAF – Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
5 University of Hawai’i, Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
6 Department of Physics and Astronomy, University of Kentucky, Lexington, KY 40506-0055, USA
7 Department of Physics and Astronomy, Colby College, Waterville, ME 04901, USA
8 Spitzer Science Center, California Institute of Technology, M/S 220-6, 1200 E. California Blvd., Pasadena, CA 91125, USA
9 Instituto de Fisica y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Gran Bretaña 1111, Playa Ancha, Valparaíso Chile
Key words: galaxies: active / galaxies: evolution / galaxies: high-redshift / galaxies: starburst / techniques: spectroscopic / submilimeter: galaxies / errata, addenda
with the meaning of all values remaining the same as in the original manuscript. None of the results in the original manuscript are affected as a result of this error as the correct (above) formula was used in all calculations.
© ESO, 2016
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