Table 1
Overview of the new observations of transits of HAT-P-12b during 2016 and 2017.
| Date | Telescope | Filter | texp (s) | Ndata | rms (mag) | β |
|---|---|---|---|---|---|---|
| 07 May 2016 | STELLA | g′ | 80 | 163 | 0.0016 | 1.00 |
| 18 Mar 2017 | 1.23 m Calar Alto | B | 150 | 97 | 0.0016 | 1.22 |
| 21 Mar 2017 | STELLA | g′ | 80 | 108 | 0.0016 | 1.15 |
| 02 May 2017 | STELLA | g′ | 80 | 149 | 0.0015 | 1.34 |
| 05 May 2017 | STELLA | g′ | 80 | 130 | 0.0017 | 1.48 |
| 18 May 2017 | 2.2 m Calar Alto | B | 60 | 161 | 0.0022 | 1.15 |
| 18 May 2017 | TNG | B | 40 | 257 | 0.0008 | 1.15 |
| 18 May 2017 | 1.23 m Calar Alto | B | 120 | 170 | 0.0019 | 1.30 |
| 03 June 2017 | STELLA | g′ | 80 | 150 | 0.0017 | 1.25 |
| 05 July 2017 | ARC | B | 45 | 210 | 0.0017 | 1.00 |
Notes. The columns present the observational date, the telescope, and the associated filter that was used for each observation. Furthermore, the exposure time in seconds texp, the individual data points of each transit Ndata, and the scatter of the data points as root-mean-square (rms) of the light curve residuals. The β factor is shown in the last column.
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