Open Access

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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