Table 2.

Average values and standard deviations for the terrestrial planet multiplicity and planet mass (Mp), semimajor axis (ap), eccentricity (e), and inclination (i) after |$7 \, \rm Myr$| of integration time for all models. These statistics only consider bodies with a mass larger or equal to 0.1 M. We also list the binary separation and eccentricity, and the SPH fit for the initial surface density profiles of each model for reference. Models that include the subscript JS include Jupiter and Saturn, and the model that includes the subscript X begins with a truncated disc that only includes bodies at or exterior to the critical stability limit for an eccentric binary, |$a_{\rm c}=3.6 \, a_{\rm b}$|⁠.

Model|$a_{\rm b}/ \rm au$|ebSurface densityNo. of planetsMp (M)|$a_{\rm p}/ \rm au$|ei°
SHFitCH5.8 ± 0.760.81 ± 0.602.59 ± 1.200.06 ± 0.051.70 ± 1.53
CH0.50.0FitCH5.1 ± 1.280.89 ± 0.582.76 ± 0.880.04 ± 0.030.96 ± 0.66
EH0.50.8FitEH3.4 ± 1.031.22 ± 0.673.21 ± 0.790.06 ± 0.042.63 ± 2.27
S1FitC14.8 ± 0.750.99 ± 0.732.98 ± 0.950.04 ± 0.041.49 ± 1.46
C11.00.0FitC12.9 ± 0.891.35 ± 0.723.45 ± 0.680.05 ± 0.031.35 ± 0.94
E11.00.8FitE11.5 ± 0.570.30 ± 0.164.10 ± 0.340.05 ± 0.031.44 ± 1.25
|$\rm CH_{\rm JS}$|0.50.0FitCH2.4 ± 0.911.35 ± 1.032.26 ± 0.440.05 ± 0.041.49 ± 1.10
|$\rm EH_{\rm JS}$|0.50.8FitEH1.4 ± 0.691.43 ± 0.742.62 ± 0.300.06 ± 0.053.16 ± 3.01
|$\rm C1_{\rm JS}$|1.00.0FitC11.4 ± 0.610.76 ± 0.452.85 ± 0.310.06 ± 0.021.10 ± 0.66
|$\rm E1_{\rm JS}$|1.00.8FitE10.0
E1X1.00.8FitE11.4 ± 0.480.29 ± 0.134.17 ± 0.310.05 ± 0.032.10 ± 1.42
Model|$a_{\rm b}/ \rm au$|ebSurface densityNo. of planetsMp (M)|$a_{\rm p}/ \rm au$|ei°
SHFitCH5.8 ± 0.760.81 ± 0.602.59 ± 1.200.06 ± 0.051.70 ± 1.53
CH0.50.0FitCH5.1 ± 1.280.89 ± 0.582.76 ± 0.880.04 ± 0.030.96 ± 0.66
EH0.50.8FitEH3.4 ± 1.031.22 ± 0.673.21 ± 0.790.06 ± 0.042.63 ± 2.27
S1FitC14.8 ± 0.750.99 ± 0.732.98 ± 0.950.04 ± 0.041.49 ± 1.46
C11.00.0FitC12.9 ± 0.891.35 ± 0.723.45 ± 0.680.05 ± 0.031.35 ± 0.94
E11.00.8FitE11.5 ± 0.570.30 ± 0.164.10 ± 0.340.05 ± 0.031.44 ± 1.25
|$\rm CH_{\rm JS}$|0.50.0FitCH2.4 ± 0.911.35 ± 1.032.26 ± 0.440.05 ± 0.041.49 ± 1.10
|$\rm EH_{\rm JS}$|0.50.8FitEH1.4 ± 0.691.43 ± 0.742.62 ± 0.300.06 ± 0.053.16 ± 3.01
|$\rm C1_{\rm JS}$|1.00.0FitC11.4 ± 0.610.76 ± 0.452.85 ± 0.310.06 ± 0.021.10 ± 0.66
|$\rm E1_{\rm JS}$|1.00.8FitE10.0
E1X1.00.8FitE11.4 ± 0.480.29 ± 0.134.17 ± 0.310.05 ± 0.032.10 ± 1.42
Table 2.

Average values and standard deviations for the terrestrial planet multiplicity and planet mass (Mp), semimajor axis (ap), eccentricity (e), and inclination (i) after |$7 \, \rm Myr$| of integration time for all models. These statistics only consider bodies with a mass larger or equal to 0.1 M. We also list the binary separation and eccentricity, and the SPH fit for the initial surface density profiles of each model for reference. Models that include the subscript JS include Jupiter and Saturn, and the model that includes the subscript X begins with a truncated disc that only includes bodies at or exterior to the critical stability limit for an eccentric binary, |$a_{\rm c}=3.6 \, a_{\rm b}$|⁠.

Model|$a_{\rm b}/ \rm au$|ebSurface densityNo. of planetsMp (M)|$a_{\rm p}/ \rm au$|ei°
SHFitCH5.8 ± 0.760.81 ± 0.602.59 ± 1.200.06 ± 0.051.70 ± 1.53
CH0.50.0FitCH5.1 ± 1.280.89 ± 0.582.76 ± 0.880.04 ± 0.030.96 ± 0.66
EH0.50.8FitEH3.4 ± 1.031.22 ± 0.673.21 ± 0.790.06 ± 0.042.63 ± 2.27
S1FitC14.8 ± 0.750.99 ± 0.732.98 ± 0.950.04 ± 0.041.49 ± 1.46
C11.00.0FitC12.9 ± 0.891.35 ± 0.723.45 ± 0.680.05 ± 0.031.35 ± 0.94
E11.00.8FitE11.5 ± 0.570.30 ± 0.164.10 ± 0.340.05 ± 0.031.44 ± 1.25
|$\rm CH_{\rm JS}$|0.50.0FitCH2.4 ± 0.911.35 ± 1.032.26 ± 0.440.05 ± 0.041.49 ± 1.10
|$\rm EH_{\rm JS}$|0.50.8FitEH1.4 ± 0.691.43 ± 0.742.62 ± 0.300.06 ± 0.053.16 ± 3.01
|$\rm C1_{\rm JS}$|1.00.0FitC11.4 ± 0.610.76 ± 0.452.85 ± 0.310.06 ± 0.021.10 ± 0.66
|$\rm E1_{\rm JS}$|1.00.8FitE10.0
E1X1.00.8FitE11.4 ± 0.480.29 ± 0.134.17 ± 0.310.05 ± 0.032.10 ± 1.42
Model|$a_{\rm b}/ \rm au$|ebSurface densityNo. of planetsMp (M)|$a_{\rm p}/ \rm au$|ei°
SHFitCH5.8 ± 0.760.81 ± 0.602.59 ± 1.200.06 ± 0.051.70 ± 1.53
CH0.50.0FitCH5.1 ± 1.280.89 ± 0.582.76 ± 0.880.04 ± 0.030.96 ± 0.66
EH0.50.8FitEH3.4 ± 1.031.22 ± 0.673.21 ± 0.790.06 ± 0.042.63 ± 2.27
S1FitC14.8 ± 0.750.99 ± 0.732.98 ± 0.950.04 ± 0.041.49 ± 1.46
C11.00.0FitC12.9 ± 0.891.35 ± 0.723.45 ± 0.680.05 ± 0.031.35 ± 0.94
E11.00.8FitE11.5 ± 0.570.30 ± 0.164.10 ± 0.340.05 ± 0.031.44 ± 1.25
|$\rm CH_{\rm JS}$|0.50.0FitCH2.4 ± 0.911.35 ± 1.032.26 ± 0.440.05 ± 0.041.49 ± 1.10
|$\rm EH_{\rm JS}$|0.50.8FitEH1.4 ± 0.691.43 ± 0.742.62 ± 0.300.06 ± 0.053.16 ± 3.01
|$\rm C1_{\rm JS}$|1.00.0FitC11.4 ± 0.610.76 ± 0.452.85 ± 0.310.06 ± 0.021.10 ± 0.66
|$\rm E1_{\rm JS}$|1.00.8FitE10.0
E1X1.00.8FitE11.4 ± 0.480.29 ± 0.134.17 ± 0.310.05 ± 0.032.10 ± 1.42
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