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

    14 Citations (Scopus)

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    Physics