Cold Jupiters and small planets: Friends, foes, or indifferent? - A search for correlations with the largest exoplanet samples

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Volume 700 (August 2025)

A&A, 700 (2025) A126

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Table F.1

Occurrence rates of cold Jupiters in the CLS survey by using the selection criteria in BL24 (top) and this work (bottom).

	M_p = 0.3–13 M_Jup			M_p = 0.5–20 M_Jup
[Fe/H]	N_★ \| d	C	f_CJ [%]	N_★ \| d	C	f_CJ [%]
CLS radial velocity sample (BL24)
$\bar{[Fe/H]} = - 0.008 \pm 0.004$ $\overline {\left[ {{\rm{Fe/H}}} \right]} = - 0.008 \pm 0.004$	562 \| 51	0.981	${9.2}_{- 1.1}^{+ 1.9}$ $9.2_{ - 1.1}^{ + 1.9}$	562 \| 46	0.993	${8.2}_{- 1.0}^{+ 1.3}$ $8.2_{ - 1.0}^{ + 1.3}$
[Fe/H] < –0.1	135 \| 4	0.980	${3.0}_{- 0.9}^{+ 2.3}$ $3.0_{ - 0.9}^{ + 2.3}$	135 \| 4	0.993	${3.0}_{- 0.9}^{+ 2.3}$ $3.0_{ - 0.9}^{ + 2.3}$
–0.1 ≤ [Fe/H] ≤ + 0.1	201 \| 12	0.985	${6.1}_{- 1.3}^{+ 2.2}$ $6.1_{ - 1.3}^{ + 2.2}$	201 \| 11	0.994	${5.5}_{- 1.2}^{+ 2.1}$ $5.5_{ - 1.2}^{ + 2.1}$
[Fe/H] > + 0.1	226 \| 35	0.979	${15.8}_{- 2.1}^{+ 2.8}$ $15.8_{ - 2.1}^{ + 2.8}$	226 \| 31	0.992	${13.8}_{- 2.0}^{+ 2.6}$ $13.8_{ - 2.0}^{ + 2.6}$
CLS radial velocity sample (this work)
$\bar{[Fe/H]} = + 0.025 \pm 0.004$ $\overline {\left[ {{\rm{Fe/H}}} \right]} = + 0.025 \pm 0.004$	402 \| 50	0.987	${12.6}_{- 1.5}^{+ 1.8}$ $12.6_{ - 1.5}^{ + 1.8}$	402 \| 45	0.995	${11.2}_{- 1.4}^{+ 1.8}$ $11.2_{ - 1.4}^{ + 1.8}$
[Fe/H] < –0.1	95 \| 4	0.990	${4.2}_{- 1.2}^{+ 3.1}$ $4.2_{ - 1.2}^{ + 3.1}$	95 \| 4	0.996	${4.2}_{- 1.2}^{+ 3.1}$ $4.2_{ - 1.2}^{ + 3.1}$
–0.1 ≤ [Fe/H] ≤ + 0.1	149 \| 12	0.989	${8.1}_{- 1.7}^{+ 2.8}$ $8.1_{ - 1.7}^{ + 2.8}$	149 \| 11	0.996	${7.4}_{- 1.6}^{+ 2.7}$ $7.4_{ - 1.6}^{ + 2.7}$
[Fe/H] > + 0.1	158 \| 34	0.985	${21.8}_{- 1.7}^{+ 3.6}$ $21.8_{ - 1.7}^{ + 3.6}$	158 \| 30	0.994	${19.1}_{- 2.7}^{+ 3.5}$ $19.1_{ - 2.7}^{ + 3.5}$

Notes. Same columns as Table D.1.

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