On detecting the large separation in the autocorrelation of stellar oscillation times series

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Table 4:

Kepler performance.
			90-day run					4-year run
Stellar	Type	B-V	$m_{{\rm V}}$ magnitude					$m_{{\rm V}}$ magnitude
type as			9	10	11	12	13	9	10	11	12	1 3
HD 181907	G8III	1.09	23	23	23	23	22	379	378	377	373	364
HD 49385	G0IV	0.51	167	53	14	3.6	0.9	2709	864	233	58	14
HD 49933	F5V	0.35	44	11	2.9	0.7	0.2	715	188	46	11	2.7
HD 181420	F2V	0.40	36	10	2.5	0.6	0.1	598	161	40	9.8	2.3
HD 181906	F8V	0.43	27	6.9	1.7	0.4	0.1	446	111	27	6.5	1.5
HD 175726	G0V	0.53	3.3	0.8	0.2	0.0	0.0	54	13	3.3	0.8	0.2

Maximum amplitude $\mathcal{A}_{{\rm max}}$ for Kepler performance on CoRoT-like targets with varying magnitudes.

Source LaTeX | All tables | In the text

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