Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since $z\sim 0.7$

S. K. Leslie, M. T. Sargent, E. Schinnerer +6

Disk galaxies at intermediate redshift ($z\sim 0.7$) have been found in previous work to display more optically thick behaviour than their local counterparts in the rest-frame B-ban…