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)

Schreiber, C.; Glazebrook, K.; Papovich, C.; Díaz-Santos, T.; Verma, A.; Elbaz, D.; ... ; Wang, T. (2021)

Contribution for newspaper or weekly magazine

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201936460]

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• Galaxies: evolution
• Galaxies: high-redshift
• Galaxies: star formation
• Submillimeter: galaxies
• Errata
• Addenda
• Astrophysics - astrophysics of galaxies

• All authors: Schreiber, C.; Glazebrook, K.; Papovich, C.; Díaz-Santos, T.; Verma, A.; Elbaz, D.; Kacprzak, G.G.; Nanayakkara, W.T.T.; Oesch, P.; Pannella, M.; Spitler, L.; Straatman, C.; Tran, K.V.; Wang, T.
• Date: 2021
• Title of host publication: Astronomy and Astrophysics
• Volume: 650
• Pages: C2
• DOI: doi:10.1051/0004-6361/201936460e
• Link: https://ui.adsabs.harvard.edu/abs/2021A&A...650C...2S