We present the rest-frame UV and optical photometry and morphology of low-redshift broad-line quasar host galaxies from the Sloan Digital Sky Survey Reverberation Mapping project .
Our sample consists of 103 quasars at z < 0.8 , spanning a luminosity range of -25 \leq M _ { g } \leq - 17 mag .
We stack the multi-epoch images in the g and i bands taken by the Canada-France-Hawaii Telescope .
The combined g -band ( i -band ) images reach a 5 \sigma depth of 26.2 ( 25.2 ) mag , with a typical PSF size of 0 \farcs 7 ( 0 \farcs 6 ) .
Each quasar is decomposed into a PSF and a Sérsic profile , representing the central AGN and the host galaxy components , respectively .
The systematic errors of the measured host galaxy flux in the two bands are 0.23 and 0.18 mag .
The relative errors of the measured galaxy half-light radii ( R _ { e } ) are about 13 % .
We estimate the rest-frame u - and g -band flux of the host galaxies , and find that the AGN-to-galaxy flux ratios in the g band are between 0.9 to 4.4 ( 68.3 % confidence ) .
These galaxies have high stellar masses M _ { \ast } = 10 ^ { 10 } \sim 10 ^ { 11 } M _ { \odot } .
They have similar color with star-forming galaxies at similar redshifts , in consistent with AGN positive feedback in these quasars .
We find that the M _ { * } - M _ { \text { BH } } relation in our sample is shallower than the local M _ { \text { Bulge } } - M _ { \text { BH } } relation .
The Sérsic indices and the M _ { * } - R _ { e } relation indicate that the majority of the host galaxies are disk-like .