Planet formation by nucleated-instability: comparison with the two first CoRoT runs

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Table 2:

Characteristics of the four cases considered, and statistics of results.
Case	1	2	3	4
target selection	I	N-I	N-I	N-I
$f_{\rm I}$	0.001	0.001	0.01	0.1
# of transits	158	601	831	2513
# of detectable transits	30	29	39	146
# of confirmable transits	28	12	18	58
# of detected transits	20	7	7	37

I is for ``ideal'' target selection, and N-I is for ``non-ideal'' target selection. Detectable transits are transits producing a signal-to-noise ratio greater than the threshold, confirmable transits are planets whose radial velocity motion can be detected, and detected transits correspond to detectable transit that can be confirmed by radial velocity follow-up, and with a period lower than DT/2.

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