Table 3: Minimum planet radius for F0V, G0V, K0V, and M0V stars in unit of Earth radius, corresponding to the empirical detection curve estimated by the blind test, which possibly overestimates the minimal radius of the detected planets at the longest periods. The star radii are from Allen (2000), i.e. 1.5, 1.1, 0.85, and 0.6 solar radius, respectively.
Period F0V G0V K0V M0V

50-day 5.6 4.0 3.2 2.2

10-day 3.75 2.75 2.1 1.5

3-day 2.8 2.0 1.6 1.1

**Table 3:** Minimum planet radius for F0V, G0V, K0V, and M0V stars in unit of Earth radius, corresponding to the empirical detection curve estimated by the blind test, which possibly overestimates the minimal radius of the detected planets at the longest periods. The star radii are from Allen (2000), i.e. 1.5, 1.1, 0.85, and 0.6 solar radius, respectively.
Period	F0V	G0V	K0V	M0V
50-day	5.6	4.0	3.2	2.2
10-day	3.75	2.75	2.1	1.5
3-day	2.8	2.0	1.6	1.1

Source LaTeX | All tables | In the text

	1 Introduction
	2 Generating simulated light curves
	3 Blind search for transit events
	4 Comparison and analysis
	5 Conclusion and prospects
	References