Extrasolar planet population synthesis - II. Statistical comparison with observations

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Volume 501 / No 3 (July III 2009)

A&A, 501 3 (2009) 1161-1184

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Table 1:

Basic results of the population synthesis.
Feature	Value
Duration of synthetic survey ( $\tau _{RV,{\rm MC}}$ ) [yr]	10
RV-precision of synthetic survey ( $\epsilon _{\rm RV,MC}$ ) [m/s]	10
Nb. of initial conditions ( $N_{\rm init}$ )	70 000
Nb. of calculated synthetic planets ( $N_{\rm synt}$ )	50 204
Nb. of initial conditions without calculations ( $N_{\rm nocalc}$ )	19 796
Nb. of detectable synthetic planets ( $N_{\rm obssynt}$ )	6075
Nb. of synth. planets migrating to $a_{\rm touch}$ ( $N_{\rm hot}$ )	1386
Synth. detection probability w/o $N_{\rm hot}$ (P) [%]	8.7
Synth. detection probability w. $N_{\rm hot}$ ( $P_{\rm whot}$ ) [%]	10.7
Nb. of actual planets in obs. comp. sample ( $N_{\rm obsreal}$ )	32
Nb. of KS bootstrap samples ( $N_{\rm samp}$ )	180
Significance KS $a-M \sin i$ ( $S_{\rm a-M}$ ) [%]	87.7
Significance KS $M \sin i$ ( $S_{\rm M}$ ) [%]	95.6
Significance KS a ( $S_{\rm a}$ ) [%]	63.9
Significance KS [Fe/H] ( $S_{\rm [Fe/H]}$ ) [%]	21.7

Source LaTeX | All tables | In the text

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