The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
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Peer-reviewed
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Abstract
The [CII] 158 micron line is one of the strongest IR emission lines, which
has been shown to trace the star-formation rate (SFR) of galaxies in the nearby
Universe and up to
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1432-0746
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European Research Council (695671)