Table A.4
Statistical tests outputted by our custom-built pipeline.
| Planet | λ (μm) | Vary ld 3σ | Bad pix % | Cut time (min) | Photon noise % | MCMC acceptance fraction |
|---|---|---|---|---|---|---|
| HAT-P-32 b | 3.6 | 0.804 | 0.306 | 0.0 | 1.31 | 0.384 |
| HAT-P-32 b | 4.5 | 0.603 | 0.056 | 0.0 | 1.32 | 0.383 |
| XO-1 b | 3.6 | 0.442 | 0.113 | 10.0 | 1.31 | 0.384 |
| XO-1 b | 4.5 | 0.194 | 0.061 | 10.0 | 1.23 | 0.385 |
| HAT-P-1 b | 3.6 | 0.018 | 0.270 | 10.0 | 1.47 | 0.386 |
| HAT-P-1 b | 4.5 | 0.035 | 0.052 | 10.0 | 1.34 | 0.385 |
| WASP-17 b | 3.6 | 0.198 | 0.309 | 50.0 | 1.41 | 0.385 |
| WASP-17 b | 4.5 | 0.106 | 0.058 | 30.0 | 1.37 | 0.386 |
| WASP-39 b | 3.6 | 1.188 | 0.294 | 20.0 | 1.39 | 0.382 |
| WASP-39 b | 4.5 | 0.416 | 0.062 | 0.0 | 1.32 | 0.381 |
| HAT-P-12 b | 3.6 | 0.387 | 0.289 | 10.0 | 1.35 | 0.382 |
| HAT-P-12 b | 4.5 | 0.273 | 0.062 | 10.0 | 1.34 | 0.383 |
| HAT-P-18 b | 3.6 | 0.382 | 0.243 | 20.0 | 1.47 | 0.382 |
| HAT-P-18 b | 4.5 | 0.183 | 0.067 | 0.0 | 1.34 | 0.385 |
| TrES2 b | 3.6 | 0.332 | 0.275 | 10.0 | 1.33 | 0.383 |
| TrES2 b | 4.5 | 0.193 | 0.069 | 5.0 | 1.26 | 0.385 |
| WASP-4 b | 3.6 | 1.424 | 0.295 | 10.0 | 1.53 | 0.384 |
| WASP-4 b | 4.5 | 0.771 | 0.049 | 30.0 | 1.48 | 0.385 |
| XO-2 b | 3.6 | 0.156 | 0.250 | 30.0 | 1.27 | 0.385 |
| XO-2 b | 4.5 | 0.052 | 0.048 | 20.0 | 1.24 | 0.383 |
| GJ3470 b | 3.6 | 0.523 | 0.007 | 5.0 | 1.22 | 0.382 |
| GJ3470 b | 4.5 | 0.246 | 0.006 | 5.0 | 1.28 | 0.383 |
| WASP-21 b | 3.6 | 0.029 | 0.242 | 40.0 | 1.39 | 0.383 |
| WASP-21 b | 4.5 | 0.020 | 0.070 | 10.0 | 1.32 | 0.383 |
| WASP-31 b | 3.6 | 0.034 | 0.317 | 30.0 | 1.46 | 0.383 |
| WASP-31 b | 4.5 | 0.037 | 0.055 | 10.0 | 1.43 | 0.383 |
| WASP-1 b | 3.6 | 0.742 | 0.331 | 10.0 | 1.43 | 0.384 |
| WASP-1 b | 4.5 | 0.490 | 0.055 | 40.0 | 1.39 | 0.387 |
| HAT-P-26 b | 3.6 | 1.501 | 0.265 | 10.0 | 1.35 | 0.384 |
| HAT-P-26 b | 4.5 | 0.689 | 0.069 | 10.0 | 1.29 | 0.383 |
| WASP-107 b | 3.6 | 9.628 | 0.010 | 95.0 | 1.30 | 0.384 |
| WASP-107 b | 4.5 | 4.939 | 0.048 | 15.0 | 1.26 | 0.385 |
| WASP-13 b | 3.6 | 0.319 | 0.263 | 55.0 | 1.25 | 0.383 |
| WASP-13 b | 4.5 | 0.137 | 0.060 | 10.0 | 1.26 | 0.384 |
| WASP-121 b | 3.6 | 0.585 | 0.248 | 45.0 | 1.13 | 0.384 |
| WASP-121 b | 4.5 | 0.343 | 0.070 | 30.0 | 1.08 | 0.382 |
| WASP-69 b | 3.6 | 0.078 | 0.008 | 30.0 | 1.25 | 0.383 |
| WASP-69 b | 4.5 | 0.057 | 0.009 | 25.0 | 1.21 | 0.382 |
| WASP-67 b | 3.6 | 0.548 | 0.193 | 45.0 | 1.33 | 0.385 |
| WASP-67 b | 4.5 | 0.196 | 0.075 | 30.0 | 1.24 | 0.385 |
| HATS-7 b | 3.6 | 0.039 | 0.240 | 35.0 | 1.38 | 0.386 |
| HATS-7 b | 4.5 | 0.017 | 0.056 | 30.0 | 1.40 | 0.385 |
| WASP-29 b | 3.6 | 1.719 | 0.274 | 70.0 | 1.35 | 0.384 |
| WASP-29 b | 4.5 | 0.822 | 0.054 | 10.0 | 1.22 | 0.381 |
| HAT-P-41 b | 3.6 | 0.403 | 0.221 | 30.0 | 1.31 | 0.382 |
| HAT-P-41 b | 4.5 | 0.201 | 0.061 | 150.0 | 1.27 | 0.384 |
| WASP-101 b | 3.6 | 0.231 | 0.261 | 30.0 | 1.33 | 0.385 |
| WASP-101 b | 4.5 | 0.140 | 0.064 | 30.0 | 1.21 | 0.384 |
| WASP-131 b | 3.6 | 0.027 | 0.304 | 30.0 | 1.26 | 0.383 |
| WASP-131 b | 4.5 | 0.033 | 0.068 | 35.0 | 1.25 | 0.383 |
| WASP-36 b | 3.6 | 0.001 | 0.320 | 110.0 | 1.49 | 0.384 |
| WASP-36 b | 4.5 | 0.003 | 0.075 | 40.0 | 1.42 | 0.383 |
| WASP-63 b | 3.6 | 0.298 | 0.307 | 60.0 | 1.30 | 0.385 |
| WASP-63 b | 4.5 | 0.107 | 0.058 | 10.0 | 1.23 | 0.384 |
| WASP-79 b | 3.6 | 0.169 | 0.291 | 35.0 | 1.45 | 0.385 |
| WASP-79 b | 4.5 | 0.158 | 0.062 | 10.0 | 1.22 | 0.385 |
| WASP-94 Ab | 3.6 | 0.591 | 0.268 | 105.0 | 1.35 | 0.384 |
| WASP-94 Ab | 4.5 | 0.348 | 0.065 | 30.0 | 1.21 | 0.385 |
| WASP-74 b | 3.6 | 0.894 | 0.008 | 90.0 | 1.26 | 0.384 |
| WASP-74 b | 4.5 | 0.560 | 0.007 | 70.0 | 1.24 | 0.384 |
| WASP-62 b | 3.6 | 0.373 | 0.255 | 85.0 | 1.47 | 0.384 |
| WASP-62 b | 4.5 | 0.239 | 0.064 | 40.0 | 1.21 | 0.384 |
| KELT-7 b | 3.6 | 0.248 | 0.009 | 60.0 | 1.29 | 0.384 |
| KELT-7 b | 4.5 | 0.182 | 0.007 | 50.0 | 1.21 | 0.382 |
| Kepler-45 b | 3.6 | 0.022 | 0.277 | 30.0 | 1.50 | 0.383 |
| Kepler-45 b | 3.6 | 0.021 | 0.280 | 10.0 | 1.55 | 0.384 |
| Kepler-45 b | 3.6 | 0.026 | 0.269 | 40.0 | 1.71 | 0.384 |
| Kepler-45 b | 3.6 | 0.024 | 0.265 | 20.0 | 1.78 | 0.384 |
| Kepler-45 b | 4.5 | 0.005 | 0.047 | 20.0 | 1.44 | 0.384 |
| Kepler-45 b | 4.5 | 0.006 | 0.065 | 20.0 | 1.51 | 0.383 |
| Kepler-45 b | 4.5 | 0.008 | 0.059 | 20.0 | 1.41 | 0.383 |
| Kepler-45 b | 4.5 | 0.005 | 0.052 | 20.0 | 1.46 | 0.385 |
Notes. We measure the strength of the dependence on the chosen limb-darkening parameters by varying them within 3σ of their error for 500 iterations. For each iteration we perform a least-squares fit and measure the variation on the measured Rp /Rs as a function of the final calculated error on Rp /Rs. ‘Bad pix’ is the number of bad pixels corrected at the beginning of the analysis. Cut time (min) is the number of minutes cut from the beginning of each observation; this value is chosen such that we keep as much baseline as possible while minimizing the chi2 of the differentpossible baselines. Photon noise is the percentage above pure statistical noise we have for each light curve; typical values for Spitzer are 30–60% above photon noise.
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