ALMA reveals the molecular gas properties of five star-forming galaxies across the main sequence at 3 < z < 3.5

Author(s):: Cassata, P.; Liu, D.; Groves, B.; Schinnerer, E.; Ibar, E.; Sargent, M.; Karim, A.; Talia, M.; Fèvre, O.L.; Tasca, L.; Lemaux, B.C.; Leite Ribeiro, B.R. (0000-0002-4844-0414); Fiore, S.; Romano, M.; Mancini, C.; Morselli, L.; Rodighiero, G.; Rodríguez-Muñoz, L.; Enia, A.; Smolcic, V.

Published: 2020
Publication type: Article / Letter to editor

Date issued: 2020-03-06
Language: English
Is part of: The Astrophysical Journal (2020), Vol. 891, no. 1, p. 83
hdl: 1887/3134402
doi: 10.3847/1538-4357/ab7452
URL: https://ui.adsabs.harvard.edu/abs/2020ApJ...891...83C