Frequency dependence of p-mode frequency shifts induced by magnetic activity in Kepler solar-like stars

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Table 2

Detection percentage p(λ₁ ) to have the selection criterion λ₁ fulfilled, based on simulations of linearly varying frequency shifts.

	(μHz)

δν^max (μHz)	0.09	0.16	0.25	0.35	0.61	0.70
0.0	23	19	19	19	12	6
0.1	85	51	29	20	11	3
0.2	84	40	32	20	16	5
0.3	97	76	40	31	18	3
0.4	100	88	53	43	19	14
0.5	100	95	74	51	24	8
0.6	100	100	84	57	32	10
0.7	100	99	87	71	26	11
0.8	100	100	97	75	50	13

Notes. The mean error depends on the different simulated levels of noise, σ₀ : Hz corresponds to 5σ₀ ; Hz to 10σ₀ ; Hz to 15σ₀ ; Hz to 20σ₀ ; Hz to 25σ₀ ; and Hz to 30σ₀. The parameter δν^max is the maximum linear frequency shift introduced in the associated simulation.

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