Table A.3
Results of the rotation and flare search and contamination analysis for all stars. Gaps in each LC were subtracted from the observation length (cf. Sect. 4.4).
| contamination factor | ||||||||
|---|---|---|---|---|---|---|---|---|
| TIC ID | observation sectors | obs. duration [d] | mean [%] | min [%] | max [%] | Prot | ||
| [d] | Nflares,tot [d]−1 | vflares,thresh [d]−1 | ||||||
| 38759628 | 1-13 | 302.32 | 0.6 | 0.5 | 0.7 | – | 5 | 0.003 |
| 55745883 | 1-6;8-13 | 278.64 | 2.5 | 0.0 | 5.2 | – | – | – |
| 140635646 | 1-9;11-13 | 281.35 | 0.4 | 0.1 | 0.5 | – | – | – |
| 140998116 | 1-13 | 304.2 | 3.8 | 0.2 | 9.6 | – | – | – |
Notes. (a)“∞” is set when the target is outside the mask. These stars have been excluded from the analysis. (**)denotes CPM pairs. There are 18 targets with a maximum contamination > 10%, meaning the flux in the aperture mask coming from objects other than the target makes for more than 10% of the target’s flux in at least one observation sector. Ten of these 18 stars are part of CPM pairs where contamination is mainly caused by the companions listed in Table A.2.
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