Tracking Advanced Planetary Systems (TAPAS) with HARPS-N - VI. HD 238914 and TYC 3318-01333-1: two more Li-rich giants with planets

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Table 5

Data on S_HK activity.

Star	S_HK	σ	r_RV	p	r_S∕N	p	No
BD+02 3497	0.17	0.02	-0.37	0.15	0.42	0.09	17
BD+48 740	0.17	0.03	-0.33	0.23	0.54	0.04	15
HD 181368	0.15	0.02	-0.02	0.92	-0.63	0.01	18
HD 188214	0.17	0.02	0.17	0.58	-0.29	0.34	13
HD 238914	0.11	0.01	-0.04	0.90	0.35	0.21	14
TYC 0684-00553-1	0.09	0.02	-0.12	0.67	0.07	0.79	16
TYC 3105-00152-1	0.13	0.03	0.05	0.84	-0.32	0.14	22
TYC 3263-02180-1	0.12	0.00	-0.11	0.65	0.00	0.99	19
TYC 3300-00133-1	0.16	0.03	-0.41	0.28	0.38	0.32	9
TYC 3318-01333-1	0.10	0.03	-0.25	0.39	-0.04	0.88	14
TYC 3663-01966-1	0.10	0.01	-0.56	0.08	0.47	0.15	11
TYC 3930-00681-1	0.21	0.03	-0.89	0.00	-0.33	0.32	11

Notes. The r_RV and r_S∕N are the Pearson correlation coefficients between RV and SHK, and between S/N and SHK, respectively. p is the significance level for the two-tailed test.

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