Table 3
Photometric data sets for G 264–012 and Gl 393.
| Data set | Season | Filter | Δt | Nobs | Nnights | rms | Prot |
|---|---|---|---|---|---|---|---|
| (d) | (mmag) | (d) | |||||
| G 264–012 | |||||||
| MEarth-1 | 2008–2009 | RG715 | 211 | 225 | 19 | 5.9 | ... (a) |
| MEarth-2 | 2011 | I715−895 | 89 | 252 | 11 | 7.7 | ... (a) |
| MEarth-3 | 2011–2015 | RG715 | 1480 | 462 | 96 | 6.3 | ... (a) |
| ASAS-SN | 2015–2018 | V | 1316 | 222(b) | 222 | 17.0 | 92.8 ± 0.8 |
| T90/OSN V | 2019 | V | 265 | 1413 | 78 | 5.4 | 99.7 ± 1.0 |
| T90/OSN R | 2019 | R | 265 | 1389 | 78 | 5.3 | 107.5 ± 1.2 |
| TESS | 2019–2020 | T600−1000 | 244 | 50363 | 78 | 1.5 | ... (a) |
| Gl 393 | |||||||
| ASAS | 2001–2009 | V | 2969 | 358 | 358 | 14.0 | ... (a) |
| SuperWASP | 2008–2014 | R400−700 | 2321 | 74021 | 445 | 7.6 | ... (a) |
| Kepler/K2 | 2017 | K493−897 | 78 | 3393 | 78 | 0.6 | 34.0 ± 0.1 |
| LCOGT 1.0 m | 2020 | V | 72 | 181 | 38 | 7.9 | ... (a) |
| LCOGT 0.40 m | 2020 | V | 40 | 301 | 31 | 41.4 | ... (a) |
Notes. The table header shows the data set identifier, the season, the filter used, the time span (Δt) of the observations, the number of individualobservations (Nobs), the number of nights (Nnights), the rms of the residuals after removing the strongest signal in each data set, and the rotation period (Prot) estimation with formal error bars. (a)Since no significant signal is found, tabulated rms is determined on the original time series. (b) Observations binned to one data point per night.
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.