Table A.1
TESS observations used in this study.
| Cycle | Sector | Camera | CCD | from – to | Ndata | PNR (ppm min−1) | Ntr |
|---|---|---|---|---|---|---|---|
| 2 | 14 | 1 | 1 | 2019 Jul 18-2019 Aug 14 | 18424 | 826 | 0 |
| 2 | 15 | 1 | 2 | 2019 Aug 15-2019 Sep 10 | 17749 | 883 | 1 |
| 4 | 41 | 1 | 1 | 2021 Jul 23-2021 Aug 20 | 18322 | 644 | 2 |
| 4 | 55 | 2 | 2 | 2022 Aug 05 – 2022 Sep 01 | 18882 | 633 | 1 |
| 6 | 75 | 4 | 3 | 2024 Jan 30 – 2024 Feb 26 | 19474 | 631 | 1 |
| 6 | 81 | 2 | 1 | 2024 Jul 15 – 2024 Aug 10 | 16048 | 578 | 2 |
| 6 | 82 | 2 | 2 | 2024 Aug 10-2024 Sep 05 | 18138 | 578 | 1 |
Notes. Cycle is a predefined period during which TESS observes different regions of the sky: the southern ecliptic hemisphere in odd-numbered cycles and the northern ecliptic hemisphere in even-numbered cycles. Camera and CCD specify a sensor used. Ndata is the number of useful measurements in a final light curve. PNR is the photometric noise rate in parts per million (ppm) of the normalised flux per minute of exposure (see Fulton et al. 2011), calculated for OOT data points. Ntr is the number of transits qualified for this study.
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.