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Table 1
Techniques to deal with stellar signals used by the different teams, as well as planetary and stellar parameters reported.
| Team | Techniques | Prot | P | K | T0 | ecc | ω | |
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| 1 | Torino | Bayesian framework with Gaussian process to account for red noise | Yes | Yes | Yes | Yes | Sometimes | Sometimes |
| 2 | Oxford | Bayesian framework with Gaussian process to account for red noise | No | Yes | Yes | Yes | Yes | Yes |
| 3 | M. Tuomi | Bayesian framework with Moving Average to account for red noise | Yes | Yes | Yes | No | No | No |
| 4 | P. Gregory | Bayesian framework with apodized Keplerians to account for red noise | No | Yes | Yes | Yes | Yes | Yes |
| 5 | Geneva | Bayesian framework with white noise | No | Yes | Yes | No | No | No |
| 6 | A. Hatzes | Pre-whitening | Yes | Yes | Yes | No | No | No |
| 7 | Brera | Filtering in frequency space | No | Yes | Yes | Yes | Yes | Yes |
| 8 | IMCCE | Compressed sensing and filtering in frequency space (preliminary results) | Yes | Yes | Yes | No | No | No |
Notes. Prot corresponds to the stellar rotation period, P, KT0, ecc and ω to the planetary period, semi-amplitude, transit time, eccentricity and argument of periastron, respectively.
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