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Table 1.

Summary information for the RC stars selected in each field.

Field (l, b) AV σR/R tobs N N
Kepler (76, 13) 0.22 0.018 4 yr 1729 1560

K2 0.28 0.038 80 d 2230 1227
C1 (264, 58) 0.15 0.034 48 47
C2 (354, 18) 0.89 0.04 157 9
C3 (51, −52) 0.16 0.038 126 118
C4 (172, −26) 0.85 0.037 482 38
C5 (209, 31) 0.14 0.039 291 271
C6 (321, 50) 0.18 0.036 170 159
C7 (14, −15) 0.45 0.038 145 77
C8 (129, −57) 0.15 0.04 112 104
C10 (291, 58) 0.09 0.042 43 37
C11 (1.3, 7.2) 1.23 0.035 83 0
C12 (77, −60) 0.14 0.037 112 107
C13 (180, −15) 1.24 0.037 183 0
C14 (241, 53) 0.11 0.037 88 83
C15 (347, 28) 0.74 0.031 4 0
C16 (209, 35) 0.13 0.037 102 95
C17 (319, 54) 0.13 0.042 73 71
C18 (209, 31) 0.14 0.045 11 11

TESS-SCVZ (276, −30) 0.24 0.035 1 yr 731 635

Notes. Galactic coordinates, mean extinction (in mag), mean relative uncertainty on radius, duration of observations, and number of stars before and after applying the cuts summarised in Sect. 4 (AV ≤ 0.5 mag and RUWE < 1.4). In terms of ecliptic latitude, Kepler is at +65°, K2 at around 0°, and TESS at −90°.

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