Table 1
Corrections to the 
values due to ISM absorption for the systems considered in the work of Fossati et al. (2015a).
| System |
Δ
|
|
log gp | σlog gp |
|
|
||||
| CoRoT-2 | 0.067 | −4.264 | 3.582 | 0.026 |
| HAT-P-1 | 0.046 | −4.938 | 2.874 | 0.020 |
| HAT-P-3 | 0.059 | −4.845 | 3.331 | 0.056 |
| HAT-P-4 | 0.045 | −5.037 | 3.019 | 0.041 |
| HAT-P-5 | 0.046 | −5.015 | 3.224 | 0.053 |
| HAT-P-12 | 0.069 | −5.035 | 2.753 | 0.030 |
| HAT-P-13 | 0.053 | −5.085 | 3.109 | 0.054 |
| HAT-P-16 | 0.056 | −4.806 | 3.796 | 0.043 |
| HAT-P-17 | 0.000 | −5.039 | 3.110 | 0.028 |
| HAT-P-27 | 0.061 | −4.724 | 3.169 | 0.057 |
| HAT-P-31 | 0.045 | −5.267 | 3.673 | 0.139 |
| HAT-P-44 | 0.054 | −5.193 | 2.773 | 0.070 |
| HD 149026 | 0.000 | −5.030 | 3.233 | 0.449 |
| HD 189733 | 0.000 | −4.501 | 3.338 | 0.056 |
| HD 209458 | 0.000 | −4.970 | 2.968 | 0.015 |
| TrES-1 | 0.063 | −4.675 | 3.194 | 0.038 |
| TrES-2 | 0.054 | −4.895 | 3.342 | 0.025 |
| TrES-3 | 0.064 | −4.485 | 3.444 | 0.058 |
| WASP-2 | 0.060 | −4.994 | 3.256 | 0.034 |
| WASP-4 | 0.054 | −4.811 | 3.197 | 0.024 |
| WASP-5 | 0.055 | −4.665 | 3.472 | 0.045 |
| WASP-11 | 0.067 | −4.756 | 3.019 | 0.037 |
| WASP-13 | 0.049 | −5.214 | 2.810 | 0.055 |
| WASP-16 | 0.050 | −5.050 | 3.320 | 0.063 |
| WASP-19 | 0.064 | −4.596 | 3.152 | 0.021 |
| WASP-22 | 0.050 | −4.850 | 3.036 | 0.030 |
| WASP-23 | 0.066 | −4.614 | 3.368 | 0.061 |
| WASP-26 | 0.049 | −4.931 | 3.194 | 0.049 |
| WASP-41 | 0.064 | −4.606 | 3.193 | 0.056 |
| WASP-42 | 0.062 | −4.838 | 3.026 | 0.052 |
| WASP-48 | 0.046 | −5.089 | 2.946 | 0.054 |
| WASP-50 | 0.062 | −4.608 | 3.441 | 0.028 |
| WASP-70 | 0.044 | −5.186 | 3.366 | 0.098 |
| WASP-84 | 0.000 | −4.430 | 3.287 | 0.026 |
| WASP-117 | 0.046 | −4.904 | 2.815 | 0.057 |
| XO-1 | 0.051 | −4.907 | 3.202 | 0.043 |
| XO-2 | 0.061 | −4.927 | 3.210 | 0.029 |
Notes. Columns two and three list the correction to the values and the corrected values, respectively. Columns four and five give the planets’ surface gravity (in cgs) and relative uncertainty, as given by Fossati et al. (2015a).
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