Notes. The parameters r_⋆ and r_p are the fractional stellar and planetary radius, respectively. The quantities in bracketsdenote the uncertainty in the final digit of the preceding number. ^(a) The photometric parameters of HAT-P-3 were estimated from the light curves presented in this work (Fig. 1), incorporating results from Southworth (2012) (see text). ^(b) The photometric parameters of HAT-P-12 were estimated from the light curves presented in this work, see Fig. 2. ^(c) The photometric parameters of HAT-P-22 were estimated from the light curves taken from various works (Bakos et al. 2011; Baştürk et al. 2015; Hinse et al. 2015; Turner et al. 2016), see Fig. 3. ^(d) The photometric parameters of WASP-39 were estimated from the light curves taken from different works (Faedi et al. 2011; Ricci et al. 2015; Maciejewski et al. 2016), see Fig. 4. ^(e) The photometric parameters of WASP-60 were estimated from the light curve presented in this work and the one from Turner et al. (2017), see Fig. 5.