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Table 1

Our high signal-to-noise target sample ordered by increasing Teff.

Kepler ID δ/N Teff /K log g Name N transit

5794240 11.5 3948 4.72 Kepler-45b 23
10748390 45.6 4766 4.59 HAT-P-11b 18
11391018 15.1 4787 4.58 7
5357901 10.7 5087 4.59 68
8845026 15.6 5490 4.49 1
9595827 11.3 5504 4.54 BOKS-1b 22
6849046 8.9 5541 4.32 63
9410930 8.9 5585 4.49 Kepler-41b 141
9651668 15.7 5722 4.55 86
8359498 12.2 5731 4.45 97
7023960 15.6 5768 4.50 6
11359879 13.6 5786 4.42 Kepler-15b 70
10619192 17.3 5787 4.45 Kepler-17b 154
11446443 60.6 5814 4.38 TrES-2b 167
12019440 8.8 5826 4.49 74
10874614 17.2 5826 4.42 Kepler-6b 133
7877496 9.4 5912 4.44 153
5780885 15.7 5934 4.04 Kepler-7b 70
9631995 13.6 5972 4.41 47
11804465 22.0 6011 4.23 Kepler-12b 82
6922244 9.9 6025 4.11 Kepler-8b 120
9818381 9.3 6082 4.37 Kepler-43b 114
10019708 6.9 6214 4.41 75
10666592 40.4 6264 3.79 HAT-P-7b 206
8191672 10.7 6297 3.99 Kepler-5b 121
9941662 41.7 8848 3.94 Kepler-13b 92

Notes. Teff and log (g) are taken from the Kepler planetary candidates list. δ/N is our mean SNR for the transit signal calculated in Sect. 2.3 and Ntransit gives the number of transits used for our modeling.

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