Asteroseismology of 35 Kepler and TESS δ Scuti stars near the red edge of the instability strip - The limitations of δ Scuti stars for dating open clusters

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Table A.1.

Parameters of the Kepler sample of δ Sct stars.

KIC	G $_{mag}^{(1)}$ $_{mag}^{(1)}$	log (L/L_⊙)⁽¹⁾	M (M_⊙)⁽¹⁾	R (R_⊙)⁽¹⁾	$\bar{ρ} ({\bar{ρ}}_{⊙})$ $\bar \rho\ (\bar \rho_{\odot})$	log g⁽¹⁾	T_eff (K)⁽¹⁾	v ⋅ sin i (km s⁻¹)	[Fe/H]⁽¹⁾	Spectral type
3219256	8.279	0.97 ± 0.021	1.53 ± 0.25	1.81 ± 0.09	0.258 ± 0.081	4.11 ± 0.08	7500 ± 150	96⁴	-0.02	F0IV⁽²⁾
3760002	10.632	1.13 ± 0.040	1.63 ± 0.25	2.32 ± 0.19	0.131 ± 0.052	3.92 ± 0.10	7255 ± 253	-	-0.12	F1V⁽²⁾
3942911	10.837	1.04 ± 0.022	1.58 ± 0.25	1.95 ± 0.14	0.213 ± 0.080	4.06 ± 0.09	7532 ± 263	93⁴	0.03	F0V⁽²⁾
5428254	10.506	1.02 ± 0.026	1.58 ± 0.25	1.87 ± 0.15	0.242 ± 0.096	4.09 ± 0.10	7612 ± 266	96⁴	0.13	-
5474427	11.443	1.33 ± 0.034	1.80 ± 0.25	2.96 ± 0.21	0.069 ± 0.024	3.75 ± 0.09	7213 ± 220	< 120⁽²⁾	-0.07	F0V⁽²⁾
5774557	11.056	1.30 ± 0.019	1.78 ± 0.25	2.82 ± 0.20	0.079 ± 0.028	3.79 ± 0.09	7274 ± 254	96⁴	-0.07	F0IV⁽²⁾
7106205	11.514	1.24 ± 0.018	1.72 ± 0.25	2.90 ± 0.14	0.071 ± 0.020	3.74 ± 0.08	6900 ± 138	< 120²	0.30	F1V⁽²⁾
7217483	10.702	1.31 ± 0.037	1.78 ± 0.25	2.92 ± 0.24	0.071 ± 0.028	3.76 ± 0.10	7165 ± 250	150²	-0.10	F0IV⁽²⁾
7548479	8.347	0.91 ± 0.024	1.49 ± 0.25	1.68 ± 0.08	0.314 ± 0.098	4.17 ± 0.09	7500 ± 150	10⁵	0.01	A4V⁽⁶⁾
8103917	11.561	1.17 ± 0.020	1.68 ± 0.25	2.38 ± 0.17	0.125 ± 0.045	3.91 ± 0.09	7355 ± 257	-	0.05	Am⁽²⁾
8446738	11.089	0.95 ± 0.034	1.50 ± 0.25	1.82 ± 0.15	0.249 ± 0.103	4.09 ± 0.10	7370 ± 257	-	-0.20	A7III⁽²⁾
8827821	11.160	1.00 ± 0.026	1.56 ± 0.25	1.83 ± 0.14	0.255 ± 0.099	4.11 ± 0.10	7610 ± 266	-	-0.01	A8IV-V⁽³⁾
9489590	10.906	1.13 ± 0.040	1.64 ± 0.25	2.23 ± 0.20	0.148 ± 0.062	3.95 ± 0.10	7383 ± 258	-	0.03	A9III⁽²⁾
9762713	11.206	1.35 ± 0.017	1.82 ± 0.25	3.05 ± 0.19	0.064 ± 0.021	3.73 ± 0.08	7188 ± 210	-	0.17	-
10549371	9.469	1.18 ± 0.020	1.67 ± 0.25	2.49 ± 0.08	0.108 ± 0.027	3.87 ± 0.07	7201 ± 80	71³	0.07	F2II⁽²⁾
10686752	11.311	0.90 ± 0.044	1.49 ± 0.25	1.66 ± 0.15	0.326 ± 0.143	4.17 ± 0.11	7497 ± 262	-	-0.12	A9V⁽²⁾
11183539	10.769	1.00 ± 0.018	1.57 ± 0.25	1.79 ± 0.13	0.274 ± 0.103	4.13 ± 0.09	7693 ± 269	96⁴	-0.07	-
12647070	10.684	1.09 ± 0.023	1.62 ± 0.25	2.07 ± 0.16	0.183 ± 0.071	4.01 ± 0.09	7498 ± 262	-	-0.19	-

Notes. From left to right: KIC identifier, apparent magnitude in the Gaia G Band (G_mag), luminosity (log(L/L_⊙)), mass(M/M_⊙), radius (R/R_⊙), density ( $\bar{ρ} / \bar{ρ_{⊙}}$ $\bar{\rho}/\bar{\rho_{\odot}}$ ), surface gravity (log g), effective temperature (T_eff), projected velocity (v ⋅ sin i), metallicity ([Fe/H]) and spectral type. ⁽¹⁾Murphy et al. (2019), ⁽²⁾Frasca et al. (2016), ⁽³⁾Niemczura et al. (2015), ⁽⁴⁾Jönsson et al. (2020), ⁽⁵⁾Gebran et al. (2016), ⁽⁶⁾Balona et al. (2015).

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