Table 2.
Photometric and spectroscopic observations used in the analysis of HR 7495.
| Instrument | Year | Method | Time Span | Observing | Quarters/ | Contemporaneous |
|---|---|---|---|---|---|---|
| [days] | Epochs | Sectors | ||||
| Kepler | 2009–2013 | Photometry | 1459.5 | Q1-Q17 | 17 Quarters | No |
| TESS | 2019 | Photometry | 54 | Sectors 14, 15 | 2 Sectors | No |
| TESS | 2021 | Photometry | 54 | Sectors 40, 41 | 2 Sectors | No |
| TESS | 2022 | Photometry | 27 | Sector 55 | 1 Sector | Yes |
| TESS | 2024 | Photometry | 54 | Sectors 75, 76 | 2 Sectors | No |
| FIES@NOT | 2022 | Spectroscopy (RV) | – | 10 epochs | – | Yes |
| ESPaDOnS@CFHT | 2023 | Spectropolarimetry | – | 3 epochs | – | No |
Notes. The data include different instruments and observing runs from Kepler, TESS, FIES at NOT, and ESPaDOnS at CFHT. Time spans are provided in days, and observing epochs are indicated where applicable. The “Contemporaneous” column marks datasets taken during overlapping time periods. We distinguish between the different years of TESS data because the datasets were analysed independently to avoid alias peaks introduced by the large gaps.
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.