The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo
  Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
  We present the clustering properties of low-$z$ $(z\leq1.4)$ galaxies
selected by the Hyper Suprime-Cam Subaru Strategic Program Wide layer over
$145$ deg$^{2}$. The wide-field and multi-wavelength observation yields
$5,064,770$ galaxies at $0.3\leq z\leq1.4$ with photometric redshifts and
physical properties. This enables the accurate measurement of angular
correlation functions and subsequent halo occupation distribution (HOD)
analysis allows the connection between baryonic properties and dark halo
properties. The fraction of less-massive satellite galaxies at $z\lesssim1$ is
found to be almost constant at $\sim20\%$, but it gradually decreases beyond
$M_{\star} \sim 10^{10.4}h^{-2}M_{\odot}$. However, the abundance of satellite
galaxies at $z>1$ is quite small even for less-massive galaxies due to the
rarity of massive centrals at high-$z$. This decreasing trend is connected to
the small satellite fraction of Lyman break galaxies at $z>3$. The
stellar-to-halo mass ratios at $0.3\leq z\leq1.4$ are almost consistent with
the predictions obtained using the latest empirical model; however, we identify
small excesses from the theoretical model at the massive end. The pivot halo
mass is found to be unchanged at $10^{11.9-12.1}h^{-1}M_{\odot}$ at $0.3\leq
z\leq1.4$, and we systematically show that $10^{12}h^{-1}M_{\odot}$ is a
universal pivot halo mass up to $z\sim5$ that is derived using only the
clustering/HOD analyses. Nevertheless, halo masses with peaked instantaneous
baryon conversion efficiencies are much smaller than the pivot halo mass
regardless of a redshift, and the most efficient stellar-mass assembly is
thought to be in progress in $10^{11.0-11.5}h^{-1}M_{\odot}$ dark haloes.
