Inflection point in the power spectrum of stellar brightness variations - III. Facular versus spot dominance on stars with known rotation periods

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Volume 642 (October 2020)

A&A, 642 (2020) A225

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Table 2

GPS outcome values.

	(1)				(2)	(3)			(4)
KIC	P_HFIP	σ P_HFIP	α	σ α	P_rot GPS	P_rot GLS	P_rot ACF	log g	[Fe/H]	Var	T_eff
	(d)	(d)			(d)	(d)	(d)			(ppm)	(K)
10070928	3.78	0.108	0.173	0.0050	19.894	22.132	21.747	4.594	−0.46	4688	5706
10080186	3.67	0.131	0.207	0.0074	19.315	18.239	17.747	4.547	−0.10	7472	5749
10080239	2.96	0.084	0.184	0.0052	15.578	16.577	16.131	4.547	−0.14	7174	5792
10083970	3.08	0.097	0.188	0.0059	16.210	16.308	16.374	4.559	−0.20	11 418	5745
10089777	3.65	0.066	0.188	0.0034	19.210	19.437	19.381	4.541	0.07	3752	5713
10091612	2.90	0.078	0.130	0.0035	15.263	–	22.214	4.550	−0.18	1760	5804
10125510	3.78	0.180	0.161	0.0076	19.894	–	23.427	4.372	−0.64	0608	5838
10129857	4.69	0.235	0.162	0.0081	24.684	–	28.859	4.536	−0.06	1488	5757
10136417	4.46	0.276	0.169	0.0105	23.473	27.541	26.288	4.303	0.16	2690	5849
10140949	4.12	0.127	0.182	0.0056	21.684	–	22.636	4.501	0.02	1999	5874
10146308	3.69	0.191	0.174	0.0090	19.421	–	21.193	4.591	−0.52	3340	5804
10064358	3.82	0.078	0.231	0.0047	20.105	16.526	16.533	4.486	−0.22	2526	5772

Notes. This table contains an example of the GPS outputs, the compared rotation period values from GLS & ACF, and stellar parameters for 12 randomly selected objects from samples A and B. (1) GPS outcome: in Col. 2, the P_HFIP is given, in Col. 3, its 2-sigma uncertainty, σ P_HFIP, defined from individual inflection points for each Kepler observing quarter. In Cols. 4 and 5, values of α-factor and its 2-sigma uncertainty are reported, respectively. P_rot GPS values in Col. 6, as result of applying Eq. (1) using the factor α = 0.19. (2) Col. 7 shows the P_rot reported by Reinhold & Gizon (2015). (3) P_rot and variability values reported by McQuillan et al. (2014) in Col. 8. (4) Cols. 10, 11 and 12 show the log g, [Fe/H] and T_eff, respectively,taken from Huber et al. (2014). A complete table for the 1047 objects is available at the CDS.

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