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The ALPINE-ALMA [CII] survey - Dust attenuation properties and obscured star formation at z ∼ 4.4–5.8
We present dust attenuation properties of spectroscopically confirmed star forming galaxies on the main sequence at a redshift of ∼4.4 − 5.8. Our analyses are based on the far infrared continuum observations of 118 galaxies at rest-frame 158 μ m obtained with the Atacama Large Millimeter Array (ALMA) Large Program …