| Target type . | c* . | |${\mu _{\mathrm{B}}}^{\dagger }$| . | |${\sigma _{\mathrm{B}}}^{\ddagger }$| . | |$f_{\mathrm{G}}$| § . | |${\mu _{\mathrm{G}}}^{\dagger }$| . | |${\sigma _{\mathrm{G}}}^{\ddagger }$| . | |$f_{\mathrm{R}}$| § . | |${\mu _{\mathrm{R}}}^{\dagger }$| . | |${\sigma _{\mathrm{R}}}^{\ddagger }$| . |
|---|---|---|---|---|---|---|---|---|---|
| AGN‖ | 0.304 ± 0.016 | 0.70 ± 0.02 | 0.17 ± 0.03 | 0.36 ± 0.13 | 1.25 ± 0.16 | 0.41 ± 0.13 | 0.16 ± 0.03 | 2.21 ± 0.03 | 0.17 ± 0.02 |
| AGN♯ | 0.304 ± 0.014 | 0.70 | 0.17 | 0.36 ± 0.03 | 1.25 | 0.41 | 0.16 ± 0.01 | 2.21 | 0.17 |
| AGN–LG pair♯ | 0.506 ± 0.049 | 0.70 | 0.17 | 0.33 ± 0.06 | 1.25 | 0.41 | 0.21 ± 0.03 | 2.21 | 0.17 |
| blue galaxy♯ | 0.093 ± 0.013 | 0.70 | 0.17 | 0.29 ± 0.08 | 1.25 | 0.41 | 0.17 ± 0.04 | 2.21 | 0.17 |
| Target type . | c* . | |${\mu _{\mathrm{B}}}^{\dagger }$| . | |${\sigma _{\mathrm{B}}}^{\ddagger }$| . | |$f_{\mathrm{G}}$| § . | |${\mu _{\mathrm{G}}}^{\dagger }$| . | |${\sigma _{\mathrm{G}}}^{\ddagger }$| . | |$f_{\mathrm{R}}$| § . | |${\mu _{\mathrm{R}}}^{\dagger }$| . | |${\sigma _{\mathrm{R}}}^{\ddagger }$| . |
|---|---|---|---|---|---|---|---|---|---|
| AGN‖ | 0.304 ± 0.016 | 0.70 ± 0.02 | 0.17 ± 0.03 | 0.36 ± 0.13 | 1.25 ± 0.16 | 0.41 ± 0.13 | 0.16 ± 0.03 | 2.21 ± 0.03 | 0.17 ± 0.02 |
| AGN♯ | 0.304 ± 0.014 | 0.70 | 0.17 | 0.36 ± 0.03 | 1.25 | 0.41 | 0.16 ± 0.01 | 2.21 | 0.17 |
| AGN–LG pair♯ | 0.506 ± 0.049 | 0.70 | 0.17 | 0.33 ± 0.06 | 1.25 | 0.41 | 0.21 ± 0.03 | 2.21 | 0.17 |
| blue galaxy♯ | 0.093 ± 0.013 | 0.70 | 0.17 | 0.29 ± 0.08 | 1.25 | 0.41 | 0.17 ± 0.04 | 2.21 | 0.17 |
* Scaling factor of the Gaussian distribution for each galaxy component.
† Mean of the D distribution for each component.
‡ Standard deviation of the D distribution for each component.
§ Fraction of green or red galaxy component.
‖ Fitting was applied by making all nine parameters free.
♯ Fitting was applied by fixing the mean and standard deviation parameters to the values obtained for the nine-parameter fitting to the data of the whole AGN sample.
| Target type . | c* . | |${\mu _{\mathrm{B}}}^{\dagger }$| . | |${\sigma _{\mathrm{B}}}^{\ddagger }$| . | |$f_{\mathrm{G}}$| § . | |${\mu _{\mathrm{G}}}^{\dagger }$| . | |${\sigma _{\mathrm{G}}}^{\ddagger }$| . | |$f_{\mathrm{R}}$| § . | |${\mu _{\mathrm{R}}}^{\dagger }$| . | |${\sigma _{\mathrm{R}}}^{\ddagger }$| . |
|---|---|---|---|---|---|---|---|---|---|
| AGN‖ | 0.304 ± 0.016 | 0.70 ± 0.02 | 0.17 ± 0.03 | 0.36 ± 0.13 | 1.25 ± 0.16 | 0.41 ± 0.13 | 0.16 ± 0.03 | 2.21 ± 0.03 | 0.17 ± 0.02 |
| AGN♯ | 0.304 ± 0.014 | 0.70 | 0.17 | 0.36 ± 0.03 | 1.25 | 0.41 | 0.16 ± 0.01 | 2.21 | 0.17 |
| AGN–LG pair♯ | 0.506 ± 0.049 | 0.70 | 0.17 | 0.33 ± 0.06 | 1.25 | 0.41 | 0.21 ± 0.03 | 2.21 | 0.17 |
| blue galaxy♯ | 0.093 ± 0.013 | 0.70 | 0.17 | 0.29 ± 0.08 | 1.25 | 0.41 | 0.17 ± 0.04 | 2.21 | 0.17 |
| Target type . | c* . | |${\mu _{\mathrm{B}}}^{\dagger }$| . | |${\sigma _{\mathrm{B}}}^{\ddagger }$| . | |$f_{\mathrm{G}}$| § . | |${\mu _{\mathrm{G}}}^{\dagger }$| . | |${\sigma _{\mathrm{G}}}^{\ddagger }$| . | |$f_{\mathrm{R}}$| § . | |${\mu _{\mathrm{R}}}^{\dagger }$| . | |${\sigma _{\mathrm{R}}}^{\ddagger }$| . |
|---|---|---|---|---|---|---|---|---|---|
| AGN‖ | 0.304 ± 0.016 | 0.70 ± 0.02 | 0.17 ± 0.03 | 0.36 ± 0.13 | 1.25 ± 0.16 | 0.41 ± 0.13 | 0.16 ± 0.03 | 2.21 ± 0.03 | 0.17 ± 0.02 |
| AGN♯ | 0.304 ± 0.014 | 0.70 | 0.17 | 0.36 ± 0.03 | 1.25 | 0.41 | 0.16 ± 0.01 | 2.21 | 0.17 |
| AGN–LG pair♯ | 0.506 ± 0.049 | 0.70 | 0.17 | 0.33 ± 0.06 | 1.25 | 0.41 | 0.21 ± 0.03 | 2.21 | 0.17 |
| blue galaxy♯ | 0.093 ± 0.013 | 0.70 | 0.17 | 0.29 ± 0.08 | 1.25 | 0.41 | 0.17 ± 0.04 | 2.21 | 0.17 |
* Scaling factor of the Gaussian distribution for each galaxy component.
† Mean of the D distribution for each component.
‡ Standard deviation of the D distribution for each component.
§ Fraction of green or red galaxy component.
‖ Fitting was applied by making all nine parameters free.
♯ Fitting was applied by fixing the mean and standard deviation parameters to the values obtained for the nine-parameter fitting to the data of the whole AGN sample.
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