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 2.

Parameters of 20 simulated δ Sct stars.

ID	Z	log (L/L_⊙)	M (M_⊙)	R (R_⊙)	$\bar{ρ} ({\bar{ρ}}_{⊙})$ $\bar \rho\ (\bar \rho_{\odot})$	log g	T_eff (K)	v (km s⁻¹)	Δν (d⁻¹)	Age (Myr)
1	0.012	1.3	1.88	2.72	0.09	3.84	7401	94	39	958
2	0.010	1.13	1.70	2.33	0.13	3.93	7239	168	45	1125
3	0.014	0.88	1.56	1.65	0.35	4.20	7454	125	73	775
4	0.014	1.21	1.82	2.45	0.12	3.92	7401	34	45	989
5	0.016	1.39	2.02	2.96	0.08	3.80	7480	30	36	839
6	0.016	0.89	1.60	1.73	0.31	4.16	7314	204	67	630
7	0.018	0.87	1.58	1.71	0.32	4.17	7293	42	71	829
8	0.016	0.90	1.62	1.71	0.32	4.18	7436	207	524
9	0.020	1.18	1.86	2.62	0.10	3.87	7046	32	41	1002
10	0.020	1.37	2.06	2.93	0.08	3.82	7408	94	36	776
11	0.022	1.34	2.06	2.79	0.09	3.86	7483	164	38	711
12	0.020	1.16	1.84	2.55	0.11	3.89	7034	98	42	999
13	0.022	1.31	1.88	2.80	0.09	3.82	7337	92	37	1135
14	0.022	0.98	1.74	1.84	0.28	4.15	7483	206	63	424
15	0.026	1.45	2.16	3.36	0.06	3.72	7255	86	30	776
16	0.026	0.96	1.68	2.22	0.15	3.97	6722	36	51	1183
17	0.026	1.01	1.76	1.97	0.23	4.09	7349	122	60	664
18	0.028	1.39	1.98	3.05	0.07	3.77	7356	30	34	1010
19	0.030	1.41	2.02	3.33	0.05	3.70	7130	139	29	981
20	0.030	1.53	2.32	3.65	0.05	3.68	7301	140	27	624

Notes. From left to right: Identifier number (ID), metallicity (Z), luminosity (log(L/L_⊙)), mass (M/M_⊙), radius (R/R_⊙), mean density ( $\bar{ρ} / \bar{ρ_{⊙}}$ $\bar{\rho}/\bar{\rho_{\odot}}$ ), surface gravity (log g), effective temperature (T_eff), rotational velocity (v_rot), large frequency separation (Δν), and age.

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