A low [CII]/[NII] ratio in the center of a massive galaxy at z = 3.7: Evidence for a transition to quiescence at high redshift? (Corrigendum)

¹ Astrophysics, Department of Physics, Keble Road, Oxford OX1 3RH, UK
e-mail: cschreib@orange.fr
² Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia
³ George P. and Cynthia W. Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
⁴ Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Ejército Libertador 441, Santiago 8320000, Chile
⁵ AIM-Paris-Saclay, CEA/DSM/Irfu – CNRS – Université Paris Diderot, CEA-Saclay, Pt Courrier 131, 91191 Gif-sur-Yvette, France
⁶ Leiden Observatory, Leiden University, 2300 RA Leiden, The Netherlands
⁷ Department of Astronomy, University of Geneva, 51 Ch. des Maillettes, 1290 Versoix, Switzerland
⁸ Faculty of Physics, Ludwig-Maximilians Universität, Scheinerstr. 1, 81679 Munich, Germany
⁹ Research Centre for Astronomy, Astrophysics & Astrophotonics, Macquarie University, Sydney, NSW 2109, Australia
¹⁰ Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109, Australia
¹¹ Max-Planck Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
¹² Australia Telescope National Facility, CSIRO Astronomy and Space Science, PO Box 76 Epping, NSW 1710, Australia
¹³ School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
¹⁴ Institute of Astronomy, The University of Tokyo, Osawa, Mitaka, Tokyo 181-0015, Japan
¹⁵ National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan
¹⁶ Chinese Academy of Sciences South America Center for Astronomy (CASSACA), National Astronomical Observatories, CAS, Beijing 100101, PR China
¹⁷ Institute of Astrophysics, Foundation for Research and Technology–Hellas (FORTH), Heraklion 70013, Greece