All Tables

• Table 1: The characteristics of the transits that were inserted in the light curves: the star radius R (in solar radius units), the stellar limb darkening coefficient (LD), the planet radius r, the orbital period in days, the system inclination in degrees, the semi-major axis a, the star magnitude, the final standard deviation of the light curve in percents, and some comments. The detection flag shows a series of + and - signs, corresponding to each team, respectively, from 1 to 5; + means a positive detection (for Team 1 in position 1, etc.), - means that the event is missed.
• Table 2: Table of contaminating events introduced into the light curves: magnitude, event type ("BEB'' stands for background eclipsing binaries, "GrB'' stands for grazing binaries), period and relative flux (contribution of the background star to the total flux), and the standard deviation of the final light curve. Detection flag: detection and correct identification (+), wrong identification (i), no detection (-), for each team from 1 to 5. References: UTM (Deeg, 1999, UTM), Nightfall (Wichmann, 1998, W98), (Mandel & Agol, 2002, MA), AAVSO (American Association of Variable Star Observers), Andreasen (1988) (A88).
• 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.