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)

Author(s):: Schreiber, C.; Glazebrook, K.; Papovich, C.; Díaz-Santos, T.; Verma, A.; Elbaz, D.; Kacprzak, G.G.; Nanayakkara, W.T.T. (0000-0003-2804-0648); Oesch, P.; Pannella, M.; Spitler, L.; Straatman, C.; Tran, K.V.; Wang, T.

Published: 2021
Publication type: Contribution for newspaper or weekly magazine

Abstract

This article is an erratum for:

[https://doi.org/10.1051/0004-6361/201936460]

Galaxies: evolutionGalaxies: high-redshiftGalaxies: star formationSubmillimeter: galaxiesErrataAddendaAstrophysics - astrophysics of galaxies

Date issued: 2021
Language: English
Is part of: Astronomy and Astrophysics (2021), Vol. 650, p. C2
hdl: 1887/3264002
doi: 10.1051/0004-6361/201936460e
URL: https://ui.adsabs.harvard.edu/abs/2021A&A...650C...2S