Table 1
Overview about new transit observations of HAT-P-12b.
| Date | Telescope | Filter | texp (s) | Cadence (s) | Ndata | rms (mmag) | β | Airmass |
|
|
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| 2011 Mar. 9 | Asiago | R | 10 | 12.1 | 1117 | 2.00 | 1.12 | 1.00–1.20 |
| 2011 Apr. 7 | STELLA | r ′ | 40 | 78 | 205 | 1.92 | 1.64 | 1.03–1.91 |
| 2011 Apr. 23 | STELLA | r ′ | 40 | 78 | 85 | 1.45 | 1.00 | 1.07–1.28 |
| 2011 May 9 | STELLA | r ′ | 40 | 78 | 204 | 1.26 | 1.02 | 1.03–1.59 |
| 2011 May 25 | STELLA | r ′ | 40 | 78 | 204 | 1.83 | 1.00 | 1.08–2.77 |
| 2011 Jun. 7 | STELLA | r ′ | 40 | 78 | 205 | 1.14 | 1.00 | 1.03–1.61 |
| 2011 Jun. 23 | STELLA | r ′ | 40 | 78 | 203 | 2.03 | 1.06 | 1.07–2.76 |
| 2012 Feb. 6 | STELLA | V | 30 | 145 | 133 | 4.10 | 1.08 | 1.03–1.90 |
| 2012 Mar. 19 | Asiago | R | 10 | 12.1 | 930 | 2.11 | 1.11 | 1.03–1.42 |
| 2012 May 3 | STELLA | V | 40 | 186 | 92 | 2.04 | 1.03 | 1.03–1.36 |
| 2012 May 6 | STELLA | V | 40 | 186 | 107 | 2.77 | 1.05 | 1.03–2.02 |
| 2012 Jun. 4 | STELLA | V | 40 | 128 | 129 | 3.88 | 1.00 | 1.03–2.12 |
| 2013 Apr. 5 | LBT | U spec | 90 | 125 | 66 | 1.57 | 1.18 | 1.02–1.28 |
| 2013 Apr. 5 | LBT | F972N20 | 90 | 117 | 63 | 0.98 | 1.00 | 1.02–1.28 |
| 2014 Feb. 27 | STELLA | g ′ | 80 | 104 | 140 | 1.69 | 1.00 | 1.07–2.17 |
| 2014 Mar. 15 | STELLA | g ′ | 80 | 104 | 136 | 1.34 | 1.45 | 1.03–1.28 |
| 2014 Mar. 15 | NOT | B | 60 | 103 | 139 | 1.52 | 1.00 | 1.04–1.34 |
| 2014 Mar. 15 | WHT | u ′ | 23 | 23 | 676 | 7.16 | 1.36 | 1.03–1.38 |
| 2014 Mar. 15 | WHT | g ′ | 5.7 | 5.7 | 2717 | 1.69 | 1.96 | 1.03–1.38 |
| 2014 Mar. 15 | WHT | r ′ | 5.7 | 5.7 | 2717 | 1.27 | 2.00 | 1.03–1.38 |
| 2014 May 15 | OAdM | I | 120 | 136 | 40 | 1.44 | 1.76 | 1.20–1.51 |
| 2014 May 28 | STELLA | i ′ | 45 | 72 | 240 | 1.55 | 1.00 | 1.04–1.56 |
| 2014 May 28 | TNG | u ′ | 40 | 49 | 308 | 5.44 | 1.22 | 1.03–1.32 |
Notes. The columns give the observing date, the used telescope, the chosen filter, the exposure time, the observing cadence, the number of observed individual data points, the dispersion of the data points as root-mean-square (rms) of the observations after subtracting a transit model and a detrending function, the β factor (see Sect. 4), and the airmass range of the observation.
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