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Table 1
Details on instruments taking part in the campaign.
| # | Telescope | Diameter (m) | CCD detector | N tr |
| Observatory | Size of matrix and field of view | |||
|
|
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| 1 | Ritchey-Chrétien-Coudé Telescope | 2.0 | Roper Scientific VersArray 1300B | 1 |
| National Astronomical Observatory Rozhen, Bulgaria | 1340 × 1300 pixels,  |
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| 2 | Ritchey-Chrétien Telescope | 1.5 | Roper Scientific VersArray 2048B | 4 |
| Sierra Nevada Observatory (OSN), Spain | 2048 × 2048 pixels,  |
|||
| 3 | Trebur 1-meter Telescope | 1.2 | SBIG STL-6303 | 3 |
| Michael Adrian Observatory, Trebur, Germany | 3072 × 2048 pixels,  |
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| 4 | Schmidt Teleskop Kamera (Mugrauer & Berthold 2010) | 0.9 | E2V CCD-42-40 | 3 |
| University Observatory Jena, Germany | 2048 × 2048 pixels,  |
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| 5 | Cassegrain Telescope | 0.6 | SBIG STL-1001 | 6 |
| Nicolaus Copernicus University, Poland | 1024 × 1024 pixels,  |
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| 6 | Cassegrain Telescope | 0.6 | SBIG STL-6303 | 1 |
| Volkssternwarte Kirchheim, Germany | 3072 × 2048 pixels,  |
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Notes. Diameter is the size of a telescope’s main mirror. Ntr is the total number of complete or partial transit light curves, acquired with the given instrument.
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