HAL Id: hal-01582860
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Submitted on 18 Jan 2021
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Hidden starbursts and active galactic nuclei at 0 < z < 4
from the Herschel-VVDS-CFHTLS-D1 field: Inferences
on coevolution and feedback
Brian C. Lemaux, Emeric Le Floc’H, Olivier Le Fèvre, Olivier Ilbert,
Laurence Tresse, Lori M. Lubin, Giovanni Zamorani, Roy R. Gal, Paolo
Ciliegi, Paolo Cassata, et al.
To cite this version:
Brian C. Lemaux, Emeric Le Floc’H, Olivier Le Fèvre, Olivier Ilbert, Laurence Tresse, et al..
Hid-den starbursts and active galactic nuclei at 0 < z < 4 from the Herschel-VVDS-CFHTLS-D1 field:
Inferences on coevolution and feedback.
Astron.Astrophys., 2014, 572, pp.A90.
�10.1051/0004-6361/201323089e�. �hal-01582860�
A&A 597, C1 (2017) DOI:10.1051/0004-6361/201323089e c ESO 2016
Astronomy
&
Astrophysics
Hidden starbursts and active galactic nuclei at 0
<
z
<
4
from the Herschel
?
-VVDS-CFHTLS-D1 field:
Inferences on coevolution and feedback
(Corrigendum)
B. C. Lemaux
1, E. Le Floc’h
2, O. Le Fèvre
1, O. Ilbert
1, L. Tresse
1, L. M. Lubin
3, G. Zamorani
4, R. R. Gal
5, P. Ciliegi
4,
P. Cassata
1, 9, D. D. Kocevski
6, 7, E. J. McGrath
7, S. Bardelli
4, E. Zucca
4, and G. K. Squires
81 Aix-Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, France e-mail: brian.lemaux@lam.fr
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 Breta˜na 1111, Playa Ancha, Valparaíso
Chile
A&A 572, A90 (2014),DOI: 10.1051/0004-6361/201323089
Key words. galaxies: active – galaxies: evolution – galaxies: high-redshift – galaxies: starburst – techniques: spectroscopic – submilimeter: galaxies – errata, addenda
Due to a typographical error, the constant of proportionality in Eq. (5) was incorrectly reported in the original manuscript. The correct equation is:
SF R(L[OII])= −(7.87 ± 1.97) × 10−10 10−(hMu0 i+48.6)2.5 × c λ2 eff hEW([OII)i , (5)
? Herschelis an ESA space observatory with science instruments pro-vided by European-led Principal Investigator consortia and with impor-tant participation from NASA.
with the meaning of all values remaining the same as in the orig-inal manuscript. None of the results in the origorig-inal manuscript are affected as a result of this error as the correct (above) for-mula was used in all calculations.
