The International Deep Planet Survey - II. The frequency of directly imaged giant exoplanets with stellar mass

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Volume 594 (October 2016)

A&A, 594 (2016) A63

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Table 10

Frequencies of stars harboring at least one giant planet in given intervals of masses and semimajor axes derived from our work and from previous publications.

Stellar type	Frequency (in %)			Separation	Planet mass	Mass&SMA	Reference
		95% certitude		(AU)	(M_J)	distribution
	Mode	Min.	Max.

BA	1.90	0.50	10.05	59−460	4−14	uniform law	This work
BA	2.05	0.50	11.05	59−460	4−14	power law	This work
BA	−	−	20	59−460	> 4		Nielsen et al. (2013) ^a

BA	2.70	0.65	14.30	25−940	4−14	uniform law	This work
BA	2.75	0.70	14.70	25−940	4−14	power law	This work
BA	−	−	50	25−940	> 4		Nielsen et al. (2013) ^a

FGK	1.20	0.30	6.60	25−856	4−14	uniform law	This work
FGK	1.10	0.30	6.05	25−856	4−14	power law	This work
F2-K7	−	−	20	25−856	> 4		Nielsen & Close (2010) ^a

M	−	−	8.30	9−207	4−14	uniform law	This work
M	−	−	8.60	9−207	4−14	power law	This work
M0-M5	−	−	20	9−207	> 4		Nielsen & Close (2010) ^a

M	−	−	9.15	10−200	1−13	uniform law	This work
M	−	−	11.85	10−200	1−13	power law	This work
M	−	−	11	10−200	1−13		Bowler et al. (2015)

GKM	1.30	0.35	7.00	30−900	5−14	uniform law	This work
GKM	1.05	0.30	5.85	30−900	5−14	power law	This work
GKM	−	−	2	≥ 30	≥ 5		Kasper et al. (2007) ^a

FGKM	−	−	3.30	10−500	0.5−13	uniform law	This work
FGKM	−	−	6.25	10−500	0.5−13	power law	This work
FGKM	−	−	57	10−500	0.5−13		Lafrenière et al. (2007a)

FGKM	−	−	2.75	25−340	0.5−13	uniform law	This work
FGKM	−	−	5.20	25−340	0.5−13	power law	This work
FGKM	−	−	17	25−340	0.5−13		Lafrenière et al. (2007a)

FGKM	−	−	2.40	50−230	0.5−13	uniform law	This work
FGKM	−	−	4.50	50−230	0.5−13	power law	This work
FGKM	−	−	10	50−230	0.5−13		Lafrenière et al. (2007a)

FGKM	0.60	0.15	3.25	100−300	5−14	uniform law	This work
FGKM	0.60	0.15	3.30	100−300	5−14	power law	This work
FGKM	−	−	15	100−300	> 5		Chauvin et al. (2015) ^a

FGKM	0.50	0.15	2.80	50−300	10−14	uniform law	This work
FGKM	0.50	0.15	2.75	50−300	10−14	power law	This work
FGKM	−	−	10	50−300	>10		Chauvin et al. (2015) ^a

BAFGKM	0.45	0.15	2.60	40−150	1−14	uniform law	This work
BAFGKM	0.75	0.20	4.10	40−150	1−14	power law	This work
BAFGKM	−	−	10	40−150	> 1		Chauvin et al. (2010) ^a

BAFGKM	0.45	0.15	2.55	10−150	1−20	uniform law	This work
BAFGKM	0.85	0.25	4.70	10−150	1−20	power law	This work
BAFGKM	−	−	6	10−150	1−20		Biller et al. (2013)

BAFGKM	0.35	0.10	1.95	10−100	5−70	uniform law	This work
BAFGKM	0.45	0.15	2.45	10−100	5−70	power law	This work
BAFGKM	1.70	0.52	4.90	10−100	5−70		Brandt et al. (2014)

Notes. Credible intervals are given for confidence levels of 95%.

^(a)

The authors do not provide all the upper limits.

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