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Spatially Resolved Observations of the Ultraviolet Attenuation Curve

Published onMay 31, 2019
Spatially Resolved Observations of the Ultraviolet Attenuation Curve
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Abstract

UV attenuation curves are used to correct rest-frame UV galaxy fluxes, and they encode information about dust-star geometry and dust grain properties. Spatially resolved measurements of the UV attenuation curve in the local universe will enable better constraints on corrections, dust geometry, and dust grains across all redshifts.

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