Toward the true number of flaring giant stars in the Kepler field - Are their flaring specialities associated with their being giant stars?

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Table B.3

Available LAMOST results.

KIC No.	T_eff [K]	T_eff [K]	log g	[Fe/H]	Remark^(a)	KIC No.	T_eff [K]	T_eff [K]	logg	[Fe/H]	Remark^(a)
	TICv8	LAMOST					TICv8	LAMOST
1573138	4838	5182	3.93	0.07	V? EM	8776850	5172	5140	4.53	0.12	ABS
1872340	5454	5454	3.80	0.34	ABS			5185	4.55	0.11	ABS
2585397	4975	5218	2.98	0.18	ABS			5179	4.58	0.09	ABS
2852961	4797	4747	2.22	−0.31	ABS	8780458	4430	4427	4.47	0.13	W ABS
4157933	5567	–	–	–	ABS	8894773	4845	4845	4.37	−0.23	filled in
4180534	4496	4496	4.32	0.20	filled in	8915957^(b)	4910	7001	4.25	0.39	H ABS
4263801	5206	5211	3.80	0.12	ABS			6972	4.28	0.42	H ABS
4750889	5092	–	–	–	ABS	8951096	4879	4827	2.71	−0.54	ABS
5281818	5900	5900	3.57	0.10	S ABS	9093349	5130	4971	3.87	0.17	filled in
5296446	5611	5616	3.50	0.10	ABS	9116222	5526	5526	3.69	−0.20	ABS
5808398	4710	4536	3.00	0.20	ABS	9237305	5107	5220	3.94	0.33	ABS
6192231	4777	5398	4.07	0.32	ABS	9419002	5322	5388	3.45	0.04	S ABS
6219880	5965	5972	4.42	0.12	ABS	9716554	5120	5257	3.35	−0.36	S ABS
7363468	5230	5237	3.09	0.05	ABS	9752982	4923	5191	4.73	0.09	ABS
		5225	3.09	0.07	ABS	10603977	4933	4933	3.80	0.09	filled in
7433177	4442	5031	3.37	0.09	W ABS	10646009	4493	4505	3.10	−0.12	EM
7676676	4774	4774	3.72	0.24	EM	10666510	4790	4784	3.68	−0.35	W ABS
		4920	3.82	0.35	ABS			4797	3.75	−0.33	filled in
7740188	4419	4741	3.57	0.24	filled in	11135986	4830	–	–	–	EM
		4812	3.61	−0.21	W ABS	11407895	5732	5796	3.43	−0.01	S ABS
7848068	5072	5072	3.80	0.20	ABS	11515713	5589	5589	3.88	0.18	ABS
7869590	4370	4420	2.57	0.09	filled in?	11551404	4703	5046	3.77	−0.08	W ABS
		4392	2.58	0.19	ABS			5181	3.95	0.01	filled in
8022670	4573	4623	3.13	0.27	S EM	11554998	4301	4386	2.42	−0.25	W ABS
		4525	3.04	0.35	S EM			4431	2.46	−0.22	W ABS
		4366	2.96	0.41	S EM			4422	2.51	−0.25	W ABS
8231401	4833	–	–	–	ABS	11753121	5335	5335	4.65	0.16	ABS
8517303	4547	–	–	–	ABS			5437	4.66	0.17	ABS
8749284	5089	5089	3.25	0.18	H EM?	11962994	4604	4604	2.69	0.01	ABS
8774912	4585	–	–	–	EM

Notes. ^(a) ABS = absorption, EM=emission, V = variable, H = huge, S = strong, W = weak; ^(b) this should be an identification problem because the LAMOST spectra indicate a main-sequence F-star. For KIC 7433177, 7869590, 8022670, 8749284, 10666510, and 11551404 Frasca et al. (2016) lists Hα and Ca II infrared triplet equivalent widths.

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