A deeper look at the dust attenuation law of star-forming galaxies at high redshift

A deeper look at the dust attenuation law of star-forming galaxies at high redshift

A diverse range of dust attenuation laws is found in star-forming galaxies. In particular, Tress et al. (2018) studied the SHARDS survey to constrain the NUV bump strength (B) and the total-to-selective ratio (RV) of 1753 star-forming galaxies in the GOODS-N field at 1.5 

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2019-09, Vol.488 (2), p.2301-2311
Hauptverfasser: Tress, M, Ferreras, I, Pérez-González, P G, Bressan, A, Barro, G, Domínguez-Sánchez, H, Eliche-Moral, C
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Sprache:eng
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Zusammenfassung:A diverse range of dust attenuation laws is found in star-forming galaxies. In particular, Tress et al. (2018) studied the SHARDS survey to constrain the NUV bump strength (B) and the total-to-selective ratio (RV) of 1753 star-forming galaxies in the GOODS-N field at 1.5 
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stz1851