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Table 1

Predicted companion population around WDs for different model assumptions.

1000 planets simulation af ef MWD tWD ttot fsurv fWD
(AU) (M) (Gyr) (Gyr)
Villaver (Baseline) 11.33.2+4.8Mathematical equation: $11.3_{-3.2}^{+4.8}$ 0.150.11+0.20Mathematical equation: $0.15_{-0.11}^{+0.20}$ 0.610.04+0.06Mathematical equation: $0.61_{-0.04}^{+0.06}$ 2.912.19+2.22Mathematical equation: $2.91_{-2.19}^{+2.22}$ 5.962.41+2.41Mathematical equation: $5.96_{-2.41}^{+2.41}$ 262/1000 1.3%
Rasio (Baseline) 11.02.7+3.8Mathematical equation: $11.0_{-2.7}^{+3.8}$ 0.110.07+0.19Mathematical equation: $0.11_{-0.07}^{+0.19}$ 0.600.03+0.05Mathematical equation: $0.60_{-0.03}^{+0.05}$ 3.102.40+2.51Mathematical equation: $3.10_{-2.40}^{+2.51}$ 6.582.27+2.02Mathematical equation: $6.58_{-2.27}^{+2.02}$ 123/1000 0.6%
No Tidal Forces 9.63.4+4.5Mathematical equation: $9.6_{-3.4}^{+4.5}$ 0.180.11+0.18Mathematical equation: $0.18_{-0.11}^{+0.18}$ 0.610.04+0.05Mathematical equation: $0.61_{-0.04}^{+0.05}$ 2.671.97+2.46Mathematical equation: $2.67_{-1.97}^{+2.46}$ 5.482.26+2.51Mathematical equation: $5.48_{-2.26}^{+2.51}$ 652/1000 3.2%
Villaver (Pbreak=1500 days) 15.45.5+6.9Mathematical equation: $15.4_{-5.5}^{+6.9}$ 0.190.12+0.25Mathematical equation: $0.19_{-0.12}^{+0.25}$ 0.610.04+0.05Mathematical equation: $0.61_{-0.04}^{+0.05}$ 2.661.96+2.45Mathematical equation: $2.66_{-1.96}^{+2.45}$ 5.532.37+2.48Mathematical equation: $5.53_{-2.37}^{+2.48}$ 573/1000 2.8%
Rasio (Pbreak=1500 days) 17.06.4+5.9Mathematical equation: $17.0_{-6.4}^{+5.9}$ 0.170.12+0.24Mathematical equation: $0.17_{-0.12}^{+0.24}$ 0.610.04+0.05Mathematical equation: $0.61_{-0.04}^{+0.05}$ 2.772.07+2.35Mathematical equation: $2.77_{-2.07}^{+2.35}$ 5.752.20+2.43Mathematical equation: $5.75_{-2.20}^{+2.43}$ 386/1000 1.9%
Villaver (e=0) 11.33.4+4.2Mathematical equation: $11.3_{-3.4}^{+4.2}$ 0.00 0.610.04+0.05Mathematical equation: $0.61_{-0.04}^{+0.05}$ 2.802.07+2.45Mathematical equation: $2.80_{-2.07}^{+2.45}$ 5.832.45+2.39Mathematical equation: $5.83_{-2.45}^{+2.39}$ 343/1000 1.7%
Rasio (e=0) 11.42.8+3.9Mathematical equation: $11.4_{-2.8}^{+3.9}$ 0.00 0.600.03+0.05Mathematical equation: $0.60_{-0.03}^{+0.05}$ 2.922.29+2.21Mathematical equation: $2.92_{-2.29}^{+2.21}$ 6.172.39+2.22Mathematical equation: $6.17_{-2.39}^{+2.22}$ 170/1000 0.8%
Villaver (ηB = 0.7) 11.64.4+5.8Mathematical equation: $11.6_{-4.4}^{+5.8}$ 0.190.12+0.23Mathematical equation: $0.19_{-0.12}^{+0.23}$ 0.620.04+0.05Mathematical equation: $0.62_{-0.04}^{+0.05}$ 2.701.98+2.44Mathematical equation: $2.70_{-1.98}^{+2.44}$ 5.362.33+2.60Mathematical equation: $5.36_{-2.33}^{+2.60}$ 579/1000 2.9%
Rasio (ηB = 0.7) 12.94.3+5.3Mathematical equation: $12.9_{-4.3}^{+5.3}$ 0.180.12+0.26Mathematical equation: $0.18_{-0.12}^{+0.26}$ 0.620.04+0.05Mathematical equation: $0.62_{-0.04}^{+0.05}$ 2.822.09+2.32Mathematical equation: $2.82_{-2.09}^{+2.32}$ 5.342.20+2.62Mathematical equation: $5.34_{-2.20}^{+2.62}$ 405/1000 2.0%

Notes. We tested the impact of the assumed mass-loss efficiency for stars on the AGB, the assumed strength of tidal forces, the adopted eccentricity and planet-mass distribution, as well as the age-metallicity relation assumed for the WD progenitor stars. Each entry shows the median value with the 16th and 84th percentiles. Columns correspond to final semimajor axis, final eccentricity, WD mass, WD age, total system age, survival rate, and predicted fraction of WDs hosting substellar companions, normalized to the total sample of 20 315 WDs.

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