Erratum: 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? (A&A (2021) 646 (A68) DOI: 10.1051/0004-6361/201936460)

被引：0

作者：

Schreiber, C. ^{[1
]}

Glazebrook, K. ^{[2
]}

Papovich, C. ^{[3
]}

Diáz-Santos, T. ^{[4
,16
,17
]}

Verma, A. ^{[1
]}

Elbaz, D. ^{[5
]}

Kacprzak, G.G. ^{[2
]}

Nanayakkara, T. ^{[6
]}

Oesch, P. ^{[7
]}

Pannella, M. ^{[8
]}

Spitler, L. ^{[9
,10
]}

Straatman, C. ^{[11
]}

Tran, K.-V. ^{[12
,13
]}

Wang, T. ^{[14
,15
]}

机构：

[1] Astrophysics, Department of Physics, Keble Road, Oxford,OX13RH, United Kingdom

[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 AandM University, College Station,TX,77843, United States

[4] Núcleo de Astronomiá, Facultad de Ingenieriá 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, Gif-sur-Yvette,91191, France

[6] Leiden Observatory, Leiden University, Leiden,2300 RA, Netherlands

[7] Department of Astronomy, University of Geneva, 51 Ch. des Maillettes, Versoix,1290, Switzerland

[8] Faculty of Physics, Ludwig-Maximilians Universität, Scheinerstr. 1, Munich,81679, Germany

[9] Research Centre for Astronomy Astrophysics and Astrophotonics, Macquarie University, Sydney,NSW,2109, Australia

[10] Department of Physics and Astronomy, Macquarie University, Sydney,NSW,2109, Australia

[11] Max-Planck Institut für Astronomie, Königstuhl 17, Heidelberg,69117, 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, 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, China

[17] Institute of Astrophysics, Foundation for Research and Technology-Hellas (FORTH), Heraklion,70013, Greece

来源：

Astronomy and Astrophysics | 2021年 / 650卷

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共 3 条

[1] 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? (vol 646, A68, 2021)
Schreiber, C.
Glazebrook, K.
Papovich, C.
Diaz-Santos, T.
Verma, A.
Elbaz, D.
Kacprzak, G. G.
Nanayakkara, T.
Oesch, P.
Pannella, M.
Spitler, L.
Straatman, C.
Tran, K. -V.
Wang, T.
ASTRONOMY & ASTROPHYSICS, 2021, 650
[2] 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
Schreiber, C.
Glazebrook, K.
Papovich, C.
Diaz-Santos, T.
Verma, A.
Elbaz, D.
Kacprzak, G. G.
Nanayakkara, T.
Oesch, P.
Pannella, M.
Spitler, L.
Straatman, C.
Tran, K-, V
Wang, T.
ASTRONOMY & ASTROPHYSICS, 2021, 646
[3] Erratum: SEEDisCS: I. Molecular gas in galaxy clusters and their large-scale structure: The case of CL1411.1-1148 at z ∼0.5 (A&A (2021) 647 (A156) (2021), https://doi.org/10.1051/0004-6361/202038904)
Spérone-Longin, D. (damien.sperone-longin@epfl.ch), 1600, EDP Sciences (648):

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