Tracking Advanced Planetary Systems (TAPAS) with HARPS-N - VII. Elder suns with low-mass companions

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Table 5

Summary of the activity analysis.

Star	OS_TNG	K		BIS		FWHM				S_HK		N_e

	[days]	[m s⁻¹]	[m s⁻¹]	r	p	r	p	r	p	r	p
HD 4760	934	718.30	1.10	0.56	0.09	−0.61	0.06	0.71	0.02	−0.16	0.66	10
HD 96992	1914	117.15	1.65	−0.24	0.25	0.10	0.63	0.30	0.15	0.09	0.69	24
BD+02 3313	1870	1153.10	1.54	−0.46	0.08	0.73	0.00	0.57	0.02	0.16	0.55	16
TYC 0434-04538-1	1721	442.23	4.53	0.50	0.04	0.27	0.29	0.59	0.01	−0.19	0.47	17

Notes. The OS_TNG is an observing period for TNG only, K denotes an amplitude of observed radial velocities defined as RV_max − RV_min, and is the average RV uncertainty. All linear correlation coefficients are calculated with reference to RV. The last column (N_e) provides the number of epochs.

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