Open Access
Table 1
Input parameters used in this work for algorithms 1 and 2, and a nonexhaustive list of additional examples that can be used.
| Input parameter | Examples selected in this work for illustration | Other examples |
|---|---|---|
| Periodogram P | Lomb–Scargle periodogram (Sects. 4–6), Generalized Lomb–Scargle (Sect. 5.5) | Other periodograms’ variants: e.g., Ferraz-Mello (1981), Cumming et al. (1999), Cumming (2004), Reegen (2007); Bourguignon et al. (2007), Baluev (2013a,b), Jenkins et al. (2014); Tuomi et al. (2014), Gregory (2016), Hara et al. (2017; 2022) |
| Detection test T | Max test TM (Eq. (6)), Test of the  largest value, TC (Eq. (9)) |
Any detection test (see e.g., in Sulis et al. 2017a,b): e.g., Higher Criticism (Donoho & Jin 2004), Berk-Jones (Berk & Jones 1979) |
| Noise models ℳd | Gaussian process (Eq. (10)), Linear activity proxy with polynomials (Eq. (14)), Linear activity proxy (Eq. (16)) | Any relevant model for d: e.g., models for long term instrumental trends, stellar magnetic activity, binary trends |
| Noise models ℳn | AR process (Eq. (8)) Harvey function (Eq. (13)) | Any relevant model for n: e.g., models for meridional circulation, stellar granulation, supergranulation, or instrumental noise |
| Ancillary time series c | log  (Sects. 5 and 6) |
Any activity proxy for d: e.g., S-index (Wilson 1968), FF′ (Aigrain et al. 2012), bisector (Queloz et al. 2001) |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.