Table C.1
Photometric observations used for the light curve analysis in the present study.
| ID | TESS | TESS | Source(*) | No. of Points | Spots | Detrending | |
|---|---|---|---|---|---|---|---|
| Sector | Cadence (s) | total | used | (mag) | |||
| CG Scl | 02 | 120 | SPOC | 18300 | 1898 | 0.017 | yes |
| 29 | 600 | QLP | 3572 | 299 | 0.027 | yes | |
| 69 | 200 | FFI | 9273 | 907 | 0.019 | yes | |
| HD 27476 | 30 | 120 | SPOC | 18567 | 1994 | 0.003 | no |
| 32 | 120 | SPOC | 17977 | 2264 | 0.003 | no | |
| AW Col | 06 | 120 | SPOC | 14691 | 1004 | 0.005 | yes |
| 33 | 120 | SPOC | 12955 | 1188 | 0.005 | yes | |
| TYC 6511-1799-1 | 06 | 120 | SPOC | 14691 | 2575 | – | no |
| BD+17 1832 | 44 | 600 | TESS-SPOC | 3260 | 574 | <0.002 | yes |
| 72 | 200 | FFI | 9267 | 1639 | 0.003 | yes | |
| TYC 266-718-1 | 45 | 600 | FFI | 3397 | 251 | <0.002 | yes |
| HD 149946 | 39 | 600 | FFI | 3864 | 412 | 0.004 | yes |
| VZ PsA | 01 | 120 | SPOC | 18279 | 1137 | <0.003 | no |
| 28 | 120 | SPOC | 17285 | 2409 | <0.003 | no | |
| HD 219869 | 42 | 120 | SPOC | 17367 | 2117 | <0.003 | yes |
| 70 | 200 | FFI | 10716 | 1520 | 0.004 | yes | |
| Kepler K2 | K2 | Source | N. of Points | Spots | Detrending | ||
| Campaign | cadence (s) | total | used | (mag) | |||
| BD+17 1832 | 05 | 1800 | EVEREST | 3320 | 552 | 0.003 | no |
| 18 | 1800 | EVEREST | 2138 | 338 | 0.002 | no | |
| TYC 266-718-1 | 01 | 1800 | EVEREST | 3202 | 459 | <0.001 | yes |
| HD 149946 | 02 | 1800 | EVEREST | 3355 | 440 | <0.001 | yes |
| HD 159246 | 11a | 1800 | EVEREST | 943 | 459 | – | yes |
| 11b | 1800 | EVEREST | 1988 | 968 | – | yes | |
| HD 219869 | 12 | 1800 | EVEREST | 3379 | 516 | 0.005 | yes |
Notes. (*)Source: SPOC - the TESS Science Processing Operations Center (Jenkins et al. 2016), TESS-SPOC - the TESS Science Processing Operations Center Full-Frame Images products (Caldwell et al. 2020), QLP – MIT’s Quick Look Pipeline Full-Frame Images (Huang et al. 2020), FFI – lightcurve from Full-Frame Images processed by the lightkurve python package (Lightkurve Collaboration 2018), EVEREST – EPIC Variability Extraction and Removal for Exoplanet Science Targets (Luger et al. 2016).
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