A possible signature of terrestrial planet formation in the chemical composition of solar analogs

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Table 6:

Spearman correlation coefficient $r_{\rm S}$ , percent probability of correlation occurring by chance ( $P_{\rm S}$ ), and significance of the [X/Fe] vs. FIP or $T_{\rm C}$ slope for the $T_{\rm C}>900$ K data points of the samples shown in Fig. 6.
Sample	$r_{\rm S}$	$P_{\rm S}$	slope $/\sigma$	$r_{\rm S}$	$P_{\rm S}$	Slope $/\sigma$
	(vs. FIP)			(vs. $T_{\rm C}$ )
R03	-0.397	10.0	-2.1	0.380	13.5	1.6
A04	-0.616	3.8	-2.9	0.626	2.8	2.6
T07	+0.024	58.7	+0.1	0.386	25.1	1.2
N09	-0.093	61.9	-0.3	0.576	7.9	2.0
G10	+0.111	60.7	+0.6	0.063	63.9	1.0
BFO	-0.154	55.5	-0.5	0.322	36.3	0.9
R09	-0.222	46.2	-1.0	0.588	5.1	2.9
M09	-0.370	17.4	-1.0	0.682	0.6	2.6

Source LaTeX | All tables | In the text

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