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Table A.1

Atmospheric parameters Teff (from SDSS-based temperature scale, see Sect. 2.2, with a total uncertainty of 69 K for all stars that are not marked by an apex), [Fe/H] from ASPCAP where available, and corrected stellar masses for NGC 6791 following Sharma et al. (2016).

KIC ID T eff [Fe/H] Mass log g State
(K) (M) (dex)

2297384a 4504 0.38 ± 0.02 1.06 ± 0.04 2.37 ± 0.02 RC
2297825a 4479 0.31 ± 0.02 0.95 ± 0.05 2.37 ± 0.02 RC
2435987 4427 0.28 ± 0.02 1.09 ± 0.03 2.46 ± 0.01 RGB
2436097 4402 1.11 ± 0.03 2.51 ± 0.02 RGB
2436417 4460 0.31 ± 0.02 1.04 ± 0.04 2.32 ± 0.02 RC
2436458 4350 1.05 ± 0.03 2.45 ± 0.01 RGB
2436676 4573 0.97 ± 0.03 3.01 ± 0.01 RGB
2436732 4503 1.10 ± 0.03 2.37 ± 0.02 RC
2436818 4610 1.04 ± 0.03 2.87 ± 0.01 RGB
2437103 4503 0.83 ± 0.03 2.35 ± 0.02 RC
2437240 4459 1.15 ± 0.03 2.55 ± 0.01 RGB
2437270a 4499 1.26 ± 0.05 2.73 ± 0.02 RGB
2437325 4484 1.04 ± 0.03 2.86 ± 0.01 RGB
2437353 4520 0.30 ± 0.02 1.10 ± 0.03 2.39 ± 0.01 RC
2437564 4467 0.32 ± 0.02 1.12 ± 0.03 2.39 ± 0.02 RC
2437589a 4508 1.44 ± 0.06 2.55 ± 0.02 RGB
2437804 4439 0.35 ± 0.03 1.02 ± 0.03 2.31 ± 0.02 RC
2437933 4534 1.11 ± 0.03 2.92 ± 0.01 RGB
2437957 4556 1.03 ± 0.03 2.86 ± 0.01 RGB
2437972a 4543 1.09 ± 0.04 2.82 ± 0.02 RGB
2437976 4478 1.05 ± 0.03 2.84 ± 0.01 RGB
2437987 4517 1.13 ± 0.05 2.38 ± 0.02 RC
2438038a 4450 1.09 ± 0.04 2.68 ± 0.02 RGB
2438051 4524 0.30 ± 0.02 1.14 ± 0.07 2.37 ± 0.03 RC
2438333 4473 0.32 ± 0.02 1.08 ± 0.03 2.67 ± 0.01 RGB
2569055 4479 0.32 ± 0.02 1.09 ± 0.04 2.38 ± 0.02 RC
2569945 4507 0.33 ± 0.02 0.97 ± 0.04 2.37 ± 0.02 RC
2570094a 4485 1.16 ± 0.04 2.72 ± 0.02 RGB
2570244 4515 1.09 ± 0.03 2.91 ± 0.01 RGB
2570384 4519 0.32 ± 0.02 0.81 ± 0.05 2.65 ± 0.03 RGB

Notes. Surface gravities, log g, and corresponding 1σ uncertainties, are also provided using stellar radii computed according to Sharma et al. (2016). The evolutionary state specifies whether a star is RC or RGB, as classified by Corsaro et al. (2012, 2017).

(a)

The source for temperature is the (VK) color (Hekker et al. 2011), with an adopted uncertainty of 110 K. See Sect. 2.2 for more details.

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