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The ALPINE-ALMA [C ii] survey: Little to no evolution in the [C ii]-SFR relation over the last 13 Gyr
The [C II] 158 μ m 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 z ∼ 2. Whether this is also the case at higher redshift and in the …