Photometric objects Around Cosmic webs (PAC) delineated in a redshift survey. II. Morphology and color dependences of the stellar-halo mass relation at high mass

In this letter, we report a robust measurement of the morphology and color dependences of the stellar-halo mass relation (SHMR) at the high mass end ($10^{11.3}{\rm M_{\odot}} 6$) have the halo mass around 5.5 times larger than the disk galaxies ($n<2$). Similarly, using the rest-frame $u-r$ color, we find that red galaxies reside in halos $2.6$ times larger than those hosting blue galaxies.