Evolved stars and the origin of abundance trends in planet hosts

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Table 5

Same as Table 2 but for a sample of 34 solar analogs (T_eff = 5777 ± 200 K, log g = 4.44 ± 0.20 dex, [Fe/H] = 0.00 ± 0.20 dex).


	All elements				Only refractory
	MC		CA		MC		CA
Parameter	SR	ZS	SR	p	SR	ZS	SR	p


[Fe/H]	0.07 ± 0.18	0.18 ± 0.44	0.06	0.72	−0.38 ± 0.15	−0.96 ± 0.43	−0.48	~10^-3
log g	0.32 ± 0.15	0.79 ± 0.40	0.44	0.01	−0.02 ± 0.17	−0.05 ± 0.42	0.04	0.81
M _⋆	0.13 ± 0.17	0.32 ± 0.42	0.13	0.47	−0.18 ± 0.18	−0.45 ± 0.44	−0.22	0.20
Age	−0.22 ± 0.16	−0.53 ± 0.40	−0.29	0.10	0.08 ± 0.18	0.20 ± 0.43	0.06	0.72
R _⋆	−0.16 ± 0.18	−0.38 ± 0.43	−0.20	0.26	0.11 ± 0.18	0.26 ± 0.43	0.09	0.62
d _galact	−0.04 ± 0.18	−0.10 ± 0.43	−0.05	0.77	−0.13 ± 0.18	−0.33 ± 0.46	−0.15	0.39

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