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 3:

Constraints on the ``Hot'' planets from Fischer & Valenti (2005) and results from the synthetic population.
Feature	0.1 AU	0.01 AU	Obs. const. (FV05)
Nb. of detectable synth. planets with the FV05 bias outside feeding limit	3382		-
Detection probability with FV05 bias excluding ``Hot'' planets ( $P_{\rm FV}$ ) [%]	4.8		$4.5\pm0.7$
Nb. of ``Hot'' synth. planets detectable with the FV05 bias	259	407	-
Detection probability with FV05 bias including ``Hot'' planets ( $P_{\rm FV,whot}$ ) [%]	5.2	5.4	$\geq$ $5.5\pm0.8$
Fraction of ''Hot'' detectable planets of all FV05 detectable planets ( $F_{\rm FV}$ ) [%]	7.1	10.7	$\geq$ $19 \pm 6$

The two columns 0.1 and 0.01 AU represent the results if such final semimajor
axes for the synthetic ``Hot'' planets are assumed.

Source LaTeX | All tables | In the text

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