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Table 3

Results of the individual analyses of the four WASP-43 b and two HAT-P-20 b transit light curves.

Instr./Tel. a/R Rp/R ip [°] T14 [day] TC [BJD2 400 000] u

WASP-43

AFOSC@1.82 m 4.896 ± 0.084 0.1590 ± 0.0017 82.27 ± 0.29 0.0512 ± 0.0010 55 891.67847 ± 0.00018 0.66 ± 0.13
CAMELOT@IAC80 4.989 ± 0.070 0.1594 ± 0.0016 82.12 ± 0.21 0.04943 ± 0.00073 56 398.47228 ± 0.00016 0.511 ± 0.075
DFOSC@Danish 1.5 m 5.039 ± 0.052 0.15538 ± 0.00086 82.03 ± 0.19 0.04792 ± 0.00036 56 402.539119 ± 0.000088 0.484 ± 0.057
CCD Camera@APT2 0.8 m 4.737 ± 0.090 0.1702 ± 0.0021 81.36 ± 0.48 0.05156 ± 0.00030 57 339.66239 ± 0.00011 0.54 ± 0.11

HAT-P-20

CAMELOT@IAC80 10.74 ± 0.44 0.1534 ± 0.0034 86.32 ± 0.40 0.0796 ± 0.0016 55 943.52369 ± 0.00025 0.51 ± 0.12
CCD Camera@CA 1.23 m 11.48 ± 0.33 0.1542 ± 0.0027 87.00 ± 0.26 0.0791 ± 0.00048 56 955.634275 ± 0.000055 0.675 ± 0.068

Notes. The columns report the following parameters: a/R is the ratio between the semi-major orbital axis and the stellar radius; Rp/R is the planet to star radii ratio; i [°] is the orbital inclination angle; b is the transit impact parameter; T14 is the transit duration; TC is the epoch of mid-transit; u is the coefficient of the linear limb-darkening law according to Eq. (1) in Claret & Bloemen (2011).

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