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In this paper, we report a robust measurement of the morphology, color andgalaxy size dependences of the stellar-halo mass relation (SHMR) at the highmass end ($10^{11.3}{\rm M_{\odot}}<M_{\star}<10^{11.7}{\rm M_{\odot}}$) atredshift $z_s\sim0.6$ (Throughout the paper, we use $z_s$ for redshift, $z$ forthe z-band magnitude.). Applying our method, Photometric objects Around Cosmicwebs (PAC), developed in a previous work to CMASS and HSC-SSP observations, wemeasure the excess surface density ($\bar{n}_2w_p(r_p)$) of satellites aroundmassive central galaxies with different morphologies indicated by S\'ersicindex $n$. We find that more compact (larger $n$) central galaxies aresurrounded by more satellites. With the abundance matching method, we estimatehalo mass for the central galaxies, and find that halo mass is increasedmonotonically with $n$, solid evidence for a morphology dependence of SHMR.Specifically, our results show that the most compact galaxies ($n>6$) have thehalo mass around 5.5 times larger than the disk galaxies ($n<2$). Similarly,using the effective radius $R_e$ and the rest-frame $u-r$ color, we find thatred (large) galaxies reside in halos that are in average $2.6$ ($2.3$) timesmore massive than those hosting blue (small) galaxies.

astrophysical journal/the astrophysical journal

Photometric Objects Around Cosmic Webs (PAC) Delineated in a  Spectroscopic survey. II. Morphology, Color and Size Dependences of the  Stellar-halo Mass Relation for Massive Galaxies