Dust attenuation in 2 < z < 3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field
2018
We present the results of a new study of the relationship between infrared excess (IRX), UV spectral slope (beta) and stellar mass at redshifts 2 = 9.75, both the IRX-beta and IRX-mass relations are well described by a Calzetti-like attenuation law.
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