Probing star formation and ISM properties using galaxy disk inclination I. Evolution in disk opacity since z ∼ 0.7

S. K. Leslie^*, M. T. Sargent, E. Schinnerer, B. Groves, A. Van Der Wel, G. Zamorani, Y. Fudamoto, P. Lang, V. Smolčić

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review