Solar-like oscillations and magnetic activity of the slow rotator EK Eridani

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Table 2:

Results from different methods of period analysis of the long-term photometry.
Method	$P_{\rm phot}$ [d]	$\sigma$ [d]
Period04	308.99	-
DFT	308.76	3.36
CLEAN	308.77	4.00
Lomb-Scargle	308.91	2.04
Lafler-Kinman	308.57	3.19
MSL	310.12	5.05
PDM	309.81	7.39
Adopted value	308.8	2.5

Notes. The period has been found by a Gaussian fit to the peak, except for Period04 which uses a sinusoidal fit. The $\sigma$ is the error on the fitted peak position.

Source LaTeX | All tables | In the text

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