Close-up view of a luminous star-forming galaxy at z = 2.95

Author(s):
Berta, S.; Young, A.J.; Cox, P.; Neri, R.; Jones, B.M.; Baker, A.J.; Omont, A.; Dunne, L.; Carnero Rosell, A.; Marchetti, L.; Negrello, M.; Yang, C.; Riechers, D.A.; Dannerbauer, H.; Perez-Fournon, I.; Werf, P.P. van der (0000-0002-4389-832x); Bakx, T.; Ivison, R.J.; Beelen, A.; Buat, V.; Cooray, A.; Cortzen, I.; Dye, S.; Eales, S.; Gavazzi, R.; Harris, A.I.; Herrera, C.N.; Hughes, D.; Jin, S.; Krips, M.; Lagache, G.; Lehnert, M.; Messias, H.; Serjeant, S.; Stanley, F.; Urquhart, S.; Vlahakis, C.; Weiß, A.
Published
2021
Publication type
Article / Letter to editor
Galaxies: high-redshiftGalaxies: ISMGalaxies: star formationGravitational lensing: strongSubmillimeter: galaxiesRadio lines: ISMAstrophysics - cosmology and nongalactic astrophysics
Date issued
2021
Language
English
Is part of
Astronomy & Astrophysics (2021), Vol. 646, p. 1-33
hdl
1887/3263685
doi
10.1051/0004-6361/202039743
URL
https://ui.adsabs.harvard.edu/abs/2021A&A...646A.122B