Context. Dust attenuation in galaxies is poorly known, especially at high redshift. And yet the amount of dust attenuation is a key parameter to deduce accurate star formation rates from ultraviolet (UV) rest-frame measurements. The wavelength dependence of the dust attenuation is also of fundamental importance to interpret the observed spectral energy distributions (SEDs) and to derive photometric redshifts or physical properties of galaxies.
No takes yet. Share an insight, caveat, or question.
A 2012 study studied this question.
Synapse has enriched 4 closely related papers on similar clinical questions. Consider them for comparative context: