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The ALPINE-ALMA [C <scp>ii</scp>] survey: Investigation of 10 galaxies at <i>z</i> ∼ 4.5 with [O <scp>ii</scp>] and [C <scp>ii</scp>] line emission − ISM properties and [O <scp>ii</scp>]−SFR relation
We present $10$ main-sequence ALPINE galaxies (log($M/M_{\odot}$) = 9.2-11.1 and ${\rm SFR}=23-190\,{\rm M_{\odot}\,yr^{-1}}$) at $z\sim4.5$ with optical [OII] measurements from Keck/MOSFIRE spectroscopy and Subaru/MOIRCS narrow-band imaging. This is the largest such multi-wavelength sample at these redshifts, combining various measurements in the ultra-violet, optical, and far-infrared including [CII]$_{158{\rm \mu m}}$ line …