Notes. (1) Has a close companion of similar brightness (Gaia DR2 2051819028221333120, looks redder), both can flare; (2) measured together with KIC 3245449, an RGB star, 0.7 mag brighter, with oscillations (e.g., Mosser et al. (2014)), the periodograms of both stars shows peaksaround 12–16 days, both could flare; (3) many faint stars around; (4) blended by the dwarf KIC 5093163 (McQuillan et al. 2014), the two rotational periods 2.799 (giant) and 0.402 (dwarf) are clearly seen in the Fourier spectrum, with a 2 mag difference in J (dwarf is fainter), both can flare; (5) blended by the oscillating KIC 5961985, 2 mag brighter (Vrard et al. 2018); (6) bright F-star around, not very near; (7) KIC 6869740 is close, 2 mag brighter, FIII-IV, and pulsates (P = 0.351441); (8) a fainter star very close; (9) 2 mag fainter star nearby, one uncertain flare; (10) Two distinct periods include one at 3.18 days with one sharp signal, and another around 13.5 d, where a number of signals are seen: characteristics typical of pulsation and differential rotation, respectively.