Probing star formation and ISM properties using galaxy disk inclination - III. Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
, , , , , , and
A&A, 662 (2022) A26
Published online: 06 June 2022
DOI: 10.1051/0004-6361/202142452