Table A.1
Observational setup and weather conditions for all acquired data.
| Star | V (a) | K(b) | Observation date | Mode (c) | NDITH × NDIT × DIT (d) | ⟨ω⟩(e) | ⟨X⟩(f) | ⟨τ0⟩(g) |
|---|---|---|---|---|---|---|---|---|
| (mag) | (mag) | (yyyy-mm-dd) | (1 × 1 × s) | (′′) | (ms) | |||
| HAT-P-41 | 11.36 | 9.73 | 2016-10-24 | P | 26 × 4 × 4 | 1.53 | 1.24 | 5.70 |
| HAT-P-57 | 10.47 | 9.43 | 2016-10-09 | P | 16 × 4 × 4 | 0.61 | 1.52 | 7.61 |
| HAT-P-57 | 10.47 | 9.43 | 2017-05-15 | F | 16 × 4 × 4 | 0.92 | 1.22 | 2.94 |
| K2-02 | 10.19 | 8.03 | 2017-05-15 | F | 16 × 4 × 4 | 0.99 | 1.50 | 2.77 |
| K2-24 | 11.28 | 9.18 | 2017-06-23 | F | 16 × 4 × 4 | 2.13 | 1.58 | 1.60 |
| K2-38 | 11.39 | 9.47 | 2017-03-06 | P | 16 × 4 × 4 | 0.56 | 1.01 | 7.38 |
| K2-39 | 10.83 | 8.52 | 2017-05-15 | F | 16 × 4 × 4 | 1.13 | 1.21 | 2.47 |
| K2-99 | 11.15 | 9.72 | 2017-08-28 | F | 16 × 4 × 4 | 0.66 | 1.83 | 3.17 |
| KELT-10 | 10.70 | 9.34 | 2017-05-15 | F | 16 × 4 × 4 | 0.96 | 1.09 | 3.14 |
| WASP-2 | 11.98 | 9.63 | 2017-05-15 | F | 16 × 4 × 4 | 1.04 | 1.27 | 2.38 |
| WASP-7 | 9.48 | 8.40 | 2016-10-06 | P | 16 × 4 × 4 | 0.69 | 1.17 | 4.90 |
| WASP-8 | 9.77 | 8.09 | 2016-10-06 | P | 16 × 4 × 4 | 0.69 | 1.03 | 4.82 |
| WASP-16 | 11.31 | 9.59 | 2017-03-06 | P | 16 × 4 × 4 | 0.52 | 1.07 | 9.41 |
| WASP-20 | 10.79 | 9.39 | 2016-10-06 | P | 16 × 4 × 4 | 0.94 | 1.02 | 3.20 |
| WASP-21 | 11.59 | 9.98 | 2016-10-24 | P | 16 × 4 × 4 | 0.94 | 1.42 | 2.84 |
| WASP-29 | 11.21 | 8.78 | 2016-10-09 | P | 16 × 4 × 4 | 0.46 | 1.04 | 11.84 |
| WASP-30 | 11.46 | 10.20 | 2017-05-15 | F | 16 × 4 × 4 | 1.05 | 1.37 | 3.12 |
| WASP-54 | 10.42 | 9.04 | 2017-03-05 | P | 16 × 4 × 4 | 0.57 | 1.23 | 5.81 |
| WASP-68 | 10.68 | 8.95 | 2017-06-29 | F | 16 × 4 × 4 | 1.41 | 1.01 | 1.78 |
| WASP-69 | 9.87 | 7.46 | 2016-10-06 | P | 12 × 4 × 4 | 0.69 | 1.08 | 4.90 |
| WASP-70 | 10.79 | 9.58 | 2017-05-15 | F | 16 × 4 × 4 | 1.28 | 1.07 | 2.49 |
| WASP-71 | 10.56 | 9.32 | 2016-11-08 | P | 16 × 4 × 4 | 0.76 | 1.63 | 9.40 |
| WASP-72 | 10.87 | 9.62 | 2017-07-06 | F | 16 × 4 × 4 | 0.95 | 1.22 | 3.41 |
| WASP-73 | 10.48 | 9.03 | 2016-10-09 | P | 26 × 4 × 4 | 0.56 | 1.20 | 7.79 |
| WASP-74 | 9.76 | 8.22 | 2017-06-22 | F | 16 × 4 × 4 | 1.07 | 1.10 | 2.23 |
| WASP-76 | 9.53 | 8.24 | 2016-11-07 | P | 16 × 4 × 4 | 0.81 | 1.76 | 9.40 |
| WASP-80 | 11.87 | 8.35 | 2017-06-22 | F | 16 × 4 × 4 | 1.25 | 1.08 | 2.56 |
| WASP-87 | 10.74 | 9.60 | 2017-04-02 | F | 16 × 4 × 4 | 1.74 | 1.19 | 1.54 |
| WASP-88 | 11.39 | 10.32 | 2017-05-15 | F | 16 × 4 × 4 | 0.93 | 1.14 | 2.90 |
| WASP-94 | 10.06 | 8.87 | 2016-10-09 | P | 16 × 4 × 4 | 0.54 | 1.01 | 9.59 |
| WASP-95 | 10.09 | 8.56 | 2016-10-21 | P | 16 × 4 × 4 | 0.84 | 1.25 | 2.78 |
| WASP-97 | 10.58 | 9.03 | 2016-10-09 | P | 16 × 4 × 4 | 0.47 | 1.17 | 11.72 |
| WASP-99 | 9.48 | 8.09 | 2017-07-06 | F | 16 × 4 × 4 | 0.78 | 1.23 | 3.32 |
| WASP-108 | 11.22 | 9.80 | 2017-03-05 | P | 16 × 4 × 4 | 0.81 | 1.10 | 6.20 |
| WASP-109 | 11.44 | 10.20 | 2017-07-23 | F | 12 × 4 × 4 | 1.41 | 1.62 | 2.65 |
| WASP-111 | 10.26 | 9.00 | 2017-05-15 | F | 16 × 4 × 4 | 1.26 | 1.11 | 2.24 |
| WASP-117 | 10.15 | 8.78 | 2016-10-21 | P | 16 × 4 × 4 | 0.78 | 1.14 | 3.37 |
| WASP-118 | 11.02 | 9.79 | 2017-07-06 | F | 16 × 4 × 4 | 1.12 | 1.23 | 3.41 |
| WASP-120 | 10.96 | 9.88 | 2016-12-20 | P | 9 × 4 × 4 | 0.86 | 1.07 | 7.61 |
| WASP-121 | 10.52 | 9.37 | 2016-12-25 | P | 16 × 4 × 4 | 1.39 | 1.04 | 2.51 |
| WASP-122 | 11.00 | 9.42 | 2016-12-25 | P | 16 × 4 × 4 | 1.41 | 1.07 | 2.26 |
| WASP-123 | 11.03 | 9.36 | 2016-10-22 | P | 16 × 4 × 4 | 0.89 | 1.17 | 2.20 |
| WASP-130 | 11.11 | 9.46 | 2017-03-11 | P | 16 × 4 × 4 | 0.42 | 1.20 | 11.18 |
| WASP-131 | 10.08 | 8.57 | 2017-07-05 | F | 16 × 4 × 4 | 1.01 | 1.66 | 2.77 |
| WASP-136 | 9.98 | 8.81 | 2016-10-25 | P | 16 × 4 × 4 | 1.45 | 1.26 | 5.70 |
| WASP-137 | 10.89 | 9.46 | 2016-10-26 | P | 6 × 4 × 4 | 0.58 | 1.49 | 8.47 |
Notes. (a) V -band apparent magnitudes are from a range of sources and are those reported in TEPCat (Southworth 2011). (b) K-band system magnitudes from 2MASS (Cutri et al. 2012). (c)Observation mode is either pupil (P) or field (F) stabilised. (d)NDITH denotes the number of dithering positions, NDIT describes the number of integrations per dithering position, and DIT is the detector integration time for each individual exposure. (e) ⟨ω⟩ denotes the average seeing conditions during the observation. (f)⟨X⟩ denotes the average airmass during the observation. (g)⟨τ0⟩ denotes the average coherence time during the observation.
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