Table 6
First 10 TEPs ordered by the Roche-filling factor f(Roche).
| Star | f(Roche) | T 0 | P[d] | Age[Gyr] | Sp | V |
|
|
||||||
| WASP-12 | 0.613 | 3650 | 1.09 | 1.7 | G0 | 11.7 |
| WASP-19 | 0.590 | 2900 | 0.79 | 0.6 | G8V | 12.3 |
| WASP-4 | 0.425 | 2640 | 1.34 | 5.2 | G8 | 12.6 |
| CoRoT-1 | 0.424 | 2680 | 1.51 | 7.2 | G0V | 13.6 |
| OGLE-56 | 0.414 | 3180 | 1.21 | 2.0 | G | 16.6 |
| WASP-33 | 0.354 | 3800 | 1.22 | 0.1 | A5 | 8.3 |
| WASP-17 | 0.333 | 2340 | 3.74 | 3.0 | F4 | 11.6 |
| TrES-3 | 0.329 | 2340 | 1.31 | 0.3 | G | 12.4 |
| TrES-4 | 0.292 | 2500 | 3.55 | 2.9 | F | 11.6 |
| OGLE-132 | 0.288 | 2800 | 1.69 | 1.0 | F | 16.8 |
| HD 209458 | 0.229 | 2050 | 3.53 | 4.0 | G0V | 7.7 |
Notes.f(Roche) values are taken from Budaj (2011), ages and spectral types are from http://exoplanet.eu/, 
is the equilibrium temperature at the substellar point (assuming circular orbit – see Cowan & Agol 2011). The ages listed for WASP-4, CoRoT-1 and for TrES-3 are from Gillon et al. (2009a,b) and from Sozzetti et al. (2009), respectively. For OGLE-132 we took an age 1.0 Gyr as the average of the values given in Guillot et al. (2006).
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