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arXiv · 1709.06102

Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field

R. J. McLure·J. S. Dunlop·F. Cullen·N. Bourne·P. N. Best·S. Khochfar·R. A. A. Bowler·A. D. Biggs·J. E. Geach·D. Scott·M. J. Michalowski·W. Rujopakarn·E. van Kampen·A. Kirkpatrick·A. Pope
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Abstract

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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R. J. McLure, J. S. Dunlop, F. Cullen, N. Bourne, P. N. Best, S. Khochfar, R. A. A. Bowler, A. D. Biggs, J. E. Geach, D. Scott, M. J. Michalowski, W. Rujopakarn, E. van Kampen, A. Kirkpatrick, A. Pope. 2018-02-23. Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field. https://doi.org/10.1093/mnras%2Fsty522

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