Probing star formation and ISM properties using galaxy disk inclination - II. Testing typical FUV attenuation corrections out to z ~ 0.7S. K. Leslie, E. Schinnerer, B. Groves, M. T. Sargent, G. Zamorani, P. Lang and E. VardoulakiA&A, 616 (2018) A157DOI: https://doi.org/10.1051/0004-6361/201833114
