Table 1
Summary of follow-up transit photometry obtained for WASP-103.
| Night | Telescope | Filter | N | T exp | Baseline function |
| (s) | |||||
|
|
|||||
| 2013 Jun. 15–16 | TRAPPIST | BB | 802 | 7 | p(t1 + f1) + o |
| 2013 Jun. 28–29 | Euler | Gunn-r′ | 103 | 120 | p(t1 + f1 + b2 + xy1) |
| 2013 Jul. 11–12 | Euler | Gunn-r′ | 105 | 80 | p(t1 + b1) |
| 2013 Jul. 23–24 | TRAPPIST | BB | 941 | 9 | p(t2) + o |
| 2013 Aug. 4–5 | TRAPPIST | BB | 935 | 10 | p(t2) + o |
Notes. N = number of measurements. Texp = exposure time. BB = blue-blocking filter. The baseline functions are the analytical functions used to model the photometric baseline of each light curve (see G13). o denotes an offset fixed at the time of the meridian flip, and p(αβ) a β-order polynomial function of time (α = t), full width at half maximum (α = f), background (α = b), or stellar position on the detector (α = xy).
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