An updated dust-to-star geometry: dust attenuation does not depend on inclination in 1.3 ≤ z ≤ 2.6 star-forming galaxies from MOSDEF

Lorenz, B.; Kriek, M.T.; Shapley, A.E.; Reddy, N.A.; Sanders, R.L.; Barro, G.; ... ; Weisz, D.R. (2023)

Article / Letter to editor

• Galaxy properties
• Galaxy evolution
• High-redshift galaxies
• Star formation
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• 594
• 734
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• Astrophysics - Astrophysics of Galaxies

• All authors: Lorenz, B.; Kriek, M.T.; Shapley, A.E.; Reddy, N.A.; Sanders, R.L.; Barro, G.; Coil, A.L.; Mobasher, B.; Price, S.H.; Runco, J.N.; Shivaei, I.; Siana, B.; Weisz, D.R.
• Date: 2023
• Journal: The Astrophysical Journal
• Volume: 951
• Issue: 1
• DOI: doi:10.3847/1538-4357/accdd1
• Link: https://ui.adsabs.harvard.edu/abs/2023ApJ...951...29L