Table 1
The selected sample of targets for the TASTE project, and their parameters.
Name | Mp/MJ | Rp/RJ | P (d) | Dur (min) | i (°) | RA | Dec | V | Depth | TTV2:1 (s) | TTVm (s) | V-TDVm (s) | T-TDVm (s) |
|
|||||||||||||
WASP-11 | 0.46 | 1.05 | 3.72 | 159 | 88.50 | 030929 | +304025 | 11.9 | 0.018 | 485 | 4.13 | 8.17 | 0.06 |
HAT-P-9 | 0.78 | 1.40 | 3.92 | 206 | 86.50 | 072040 | +370826 | 12.3 | 0.012 | 302 | 2.67 | 6.43 | 0.18 |
XO-5 | 1.08 | 1.09 | 4.19 | 193 | 86.80 | 074652 | +390541 | 12.1 | 0.011 | 234 | 2.59 | 5.51 | 0.17 |
XO-2 | 0.57 | 0.97 | 2.62 | 162 | 88.58 | 074807 | +501333 | 11.2 | 0.011 | 276 | 2.38 | 6.81 | 0.02 |
HAT-P-13 | 0.85 | 1.28 | 2.92 | 194 | 83.40 | 083932 | +472107 | 10.6 | 0.007 | 206 | 1.89 | 5.80 | 0.35 |
HAT-P-3 | 0.60 | 0.89 | 2.90 | 123 | 87.24 | 134423 | +480143 | 11.9 | 0.012 | 291 | 2.60 | 5.10 | 0.12 |
HAT-P-12 | 0.21 | 0.96 | 3.21 | 140 | 90.00 | 135734 | +432937 | 12.8 | 0.020 | 906 | 6.22 | 12.54 | 0.00 |
HAT-P-14 | 2.23 | 1.15 | 4.63 | 131 | 83.50 | 172028 | +381432 | 9.98 | 0.006 | 125 | 1.52 | 1.99 | 1.23 |
HAT-P-5 | 1.06 | 1.26 | 2.79 | 175 | 86.75 | 181737 | +363718 | 12.0 | 0.012 | 158 | 1.59 | 4.61 | 0.08 |
WASP-3 | 1.76 | 1.31 | 1.85 | 137 | 85.06 | 183432 | +353942 | 10.6 | 0.011 | 63 | 0.74 | 2.52 | 0.05 |
HAT-P-1 | 0.52 | 1.23 | 4.47 | 160 | 86.28 | 225747 | +384030 | 10.4 | 0.013 | 511 | 4.10 | 6.77 | 0.41 |
HAT-P-6 | 1.06 | 1.33 | 3.85 | 203 | 85.51 | 233906 | +422758 | 10.5 | 0.009 | 219 | 2.13 | 5.16 | 0.22 |
Notes. The first ten columns give the name of the target, the planet mass Mp and radius Rp (both in jovian units), the orbital period P (in days), the transit duration (in minutes), the orbital inclination i (in degrees), the 2000.0 RA and DEC, the V magnitude of the host star, the transit depth (in flux). In the last four columns, we reported the expected TTV & TDV effects in seconds caused by a 1 M⊕ exoplanet in a 2:1 resonant external orbit (TTV2:1) and to a 1 M⊕ exomoon at one third of the Hill radius (TTVm and the V- and TIP- components of the TDVm).
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