Rotation and magnetic activity of the Hertzsprung-gap giant 31 Comae

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Table 4:

Best-fit periods in days from the MOST observations, the four APT T6 data sets, and the STELLA radial velocities.
Dataset	CLEAN	L-S	PDM	DFT	$\delta f_{\rm R}$
MOST 2007	...	3.377	6.87	6.97	0.091
APT b 1996	3.54	7.16	7.04	6.97	0.007
APT y 1996	3.56	3.56	6.94	6.96	0.007
APT v 2002	8.31	...	3.47	7.04	0.062
APT y 2002	12.2	...	3.45	6.96	0.061
STELLA 2007/8	6.73	6.76	6.80	6.75	0.008

Notes. The methods applied are CLEAN, L-S=Lomb Scargle, PDM=Phase Dispersion Method, DFT=Discrete Fourier Transform. The last column lists the Rayleigh frequency resolution, $\delta f_{\rm R}$ , defined as the inverse total time covered by the respective time series.

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