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Table 1
Properties of the GPC and the Pan-Planets survey.
| GPC specifications | |
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| Telescope | 1.8 m Pan-STARRS1 |
| Camera FOV | 7 sq. deg. |
| Filters | g ′ , r ′ , i ′ , z ′ , y ′ |
| Camera Properties | 8 × 8 CCDs 11 |
| CCD Properties | 8 × 8 cells with –600 × 600 pixels |
| Pixel scale | 0.258 arcsec/pixel |
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| Pan-Planets characteristics | |
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| Observation period | May 2010 – Sep. 2012 |
| Observation time | 165 h |
| Survey FOV | 42 sq. deg. |
| Survey area | 301.7° > RA > 293.7° |
| 21° > Dec > 13° | |
| Exposure time | 15 or 30 s |
| seeing-dependent | |
| Median FWHM | 1.07 arcsec |
| Photometric band | i ′ |
| #target stars | –4 × 106 |
| Target brightness | 13.5 mag ≤ i′ ≤ 18 mag |
| M dwarf targets | –60 000 |
| White dwarf targets | –4000 |
| Observation time per night | 1 or 3 h |
| Photometric precision | 5–15 mmag |
Notes. The GPC camera has a circular layout, i.e. the corners of the detector do not get illuminated.
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