Analysis of putative exoplanetary signatures found in light curves of two sdBV stars observed by Kepler

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Table 3

KIC 10001893: frequency amplitude modulation for the k₁ = 52.682 μHz frequency, prewhitened from LC aperture var data.

Data	(μHz)			Distance to central (μHz)		Amplitudes (ppm)			Differences of side lobe distances from central

	Left	Central freq.	Right	Left	Right	Left	Central	Right
LC	k₁	77.5306 (f₂)	102.3475 (f₁₂)	24.8484	24.8168	22	86	21	0.032
	k₁	114.6705(f₁₈)	176.6796(f₄₄)	61.9883	62.0091	22	29	25	0.021
SC	k₁	114.6710 (f₁₈)	176.6694 (f₄₄)	61.9888	61.9984	22	34	34	0.010

Notes. Only pulsating frequencies with amplitudes greater than 20 ppm and matching right-side lobe amplitudes comparable to k₁ are shown.

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