Known transiters:

CoRoT-1 b
CoRoT-2 b
CoRoT-3 b
CoRoT-4 b
CoRoT-5 b
CoRoT-6 b
CoRoT-7 b
GJ1214 b
GJ436 b
HAT-P-1 b
HAT-P-10/WASP-11 b
HAT-P-11 b
HAT-P-12 b
HAT-P-13 b
HAT-P-2 b
HAT-P-3 b
HAT-P-4 b
HAT-P-5 b
HAT-P-6 b
HAT-P-7 b
HAT-P-8 b
HAT-P-9 b
HD149026 b
HD17156 b
HD189733 b
HD209458 b
HD80606 b
Kepler-4 b
Kepler-5 b
Kepler-6 b
Kepler-7 b
Kepler-8 b
LUPUS-TR3 b
OGLE-TR-10 b
OGLE-TR-111 b
OGLE-TR-113 b
OGLE-TR-132 b
OGLE-TR-182 b
OGLE-TR-211 b
OGLE-TR-56 b
OGLE-TR-L9 b
TrES-1 b
TrES-2 b
TrES-3 b
TrES-4 b
WASP-1 b
WASP-10 b
WASP-12 b
WASP-13 b
WASP-14 b
WASP-15 b
WASP-16 b
WASP-17 b
WASP-18 b
WASP-19 b
WASP-2 b
WASP-3 b
WASP-4 b
WASP-5 b
WASP-6 b
WASP-7 b
XO-1 b
XO-2 b
XO-3 b
XO-4 b
XO-5 b

What's new:

2010-02-22 : According to latest transit observation, CoRoT-1 b orbital period was refined to P = 1.508969 d (original Porb was 1.5089557 days).

2009-12-28 : AV CMi - eclipsing binary with transiting exoplanet?
A. Liakos and P. Niarchos has found periodic transit-like features in light curve of ecplipsing binary AV CMi (EA, Porb = 2.277751 d). The third object is orbiting one of the binary component on inner orbit with period P' = 0.5192237 days. Published orbital elements for transits are

Tmid = HJD 2454521.36315 + 0.5192237d * E


Transit duration is 3.3 hours (200 minutes) and the depth is about 2.6% (0.028 mag).

Apparent magnitude of AV CMi is about 11.5 mag and EB amplitude is 0.3 mag.


We have prepared predictions of the probably transit for observers here.


Results of preliminary study published by Liakos and Niarchos leads to a conclusion, that the third object must be a brown dwarf or hot jupiter exoplanet.


For more information see: A. Liakos, P. Niarchos, Preliminary results for the triple system AV CMi