no code implementations • 8 Dec 2020 • Jonathan Freundlich, Nicolas F. Bouché, Thierry Contini, Emanuele Daddi, Johannes Zabl, Ilane Schroetter, Leindert Boogaard, Johan Richard
We further detect the dust continuum of three of the quasars and a strong emission line in one of them, which we identify as CO(4-3).
Astrophysics of Galaxies