Radial velocity homogeneous analysis of M dwarfs observed with HARPS - II. Detection limits and planetary occurrence statistics

Home

All issues

Volume 700 (August 2025)

A&A, 700 (2025) A146

Full HTML

Open Access

Table A.4

Comparison of occurrence rates

Planetary Mass range [M_⊕]	Ref	1 - 10 d	10 - 100 d	100 - 1000 d	1000 - 10000 d
100 - 1000	S21	< 3	$4_{- 2}^{+ 3}$ $\rm 4^{+3}_{-2}$	$5_{- 3}^{+ 4}$ $\rm 5^{+4}_{-3}$	−
	M24	< 0.5	$1_{- 0.3}^{+ 1}$ $\rm 1^{+1}_{-0.3}$	$1_{- 0.3}^{+ 1.5}$ $\rm 1^{+1.5}_{-0.3}$	$3_{- 1}^{+ 2}$ $\rm 3^{+2}_{-1}$
	B13	< 1	$2_{- 1}^{+ 3}$ $\rm 2^{+3}_{-1}$	< 1	$4_{- 1}^{+ 5}$ $\rm 4^{+5}_{-1}$
10 - 100	S21	$3_{- 2}^{+ 3}$ $\rm 3^{+3}_{-2}$	$10_{- 4}^{+ 5}$ $\rm 10^{+5}_{-4}$	$14_{- 7}^{+ 10}$ $\rm 14^{+10}_{-7}$	−
	M24	$3_{- 1}^{+ 2}$ $\rm 3^{+2}_{-1}$	$3_{- 1}^{+ 3}$ $\rm 3^{+3}_{-1}$	$13_{- 3}^{+ 7}$ $\rm 13^{+7}_{-3}$	< 3
	B13	$3_{- 1}^{+ 4}$ $\rm 3^{+4}_{-1}$	< 2	< 4	< 12
1 - 10	S21	$59_{- 17}^{+ 20}$ $\rm 59^{+20}_{-17}$	$97_{- 33}^{+ 42}$ $\rm 97^{+42}_{-33}$	−	−
	M24	$89_{- 15}^{+ 18}$ $\rm 89^{+18}_{-15}$	$90_{- 18}^{+ 21}$ $\rm 90^{+21}_{-18}$	$6_{- 2}^{+ 5}$ $\rm 6^{+5}_{-2}$	−
	B13	$36_{- 10}^{+ 25}$ $\rm 36^{+25}_{-10}$	$52_{- 16}^{+ 50}$ $\rm 52^{+50}_{-16}$	−	−

Notes. Planetary occurrences rates in percent from this work (M24), from Sabotta et al. (2021) (S21) and from Bonfils et al. (2013a) (B13).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.