Research Article
The Low-Mass End of the / Relation in Quasars
Table 3
Results from the imaging analysis. (1) Quasar name. (2) Redshift. (3) Apparent observed -band magnitude of the nucleus. (4) Apparent observed -band magnitude of the host galaxy. (5) Apparent central surface brightness, as extrapolated from the host galaxy model. (6) Chi-square ratio between the best fit using a pure PSF and the best fit using a galaxy+quasar model. (7) Effective radius of the host galaxy. (8) Ellipticity of the host galaxy model. (9) Sersic index of the host galaxy model. (10) Rest-frame -observed color correction. (11) Resulting absolute rest-frame -band magnitude of the host galaxy. (12) Adopted mass-to-light ratio. (13) Stellar mass of the host galaxy. (14) BH-to-host galaxy mass ratio.
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