MASSIVE: A Bayesian analysis of giant planet populations around low-mass stars

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Volume 596 (December 2016)

A&A, 596 (2016) A83

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Table 1

Giant planets and brown dwarfs imaged around self-luminous young M-dwarfs (source: http://exoplanet.eu).

Name^ref	SpT	d	Age	Comp. mass	Sep.
		(pc)	(Myr)	(M_Jup)	(AU)

Planetary-mass companions

2M 0103(AB) b⁽¹⁾	M5,5 + M6	47.2 ± 3.1	30	13.0 ± 1.0	84.0
GU Psc b⁽²⁾	M3	48.0 ± 5.0	100 ± 30	11.0 ± 2.0	2000 ± 200
J0219-3925 B⁽³⁾	M6	39.4 ± 2.6	30−40	12−15	156 ± 10
FW Tau b⁽⁴⁾	M4	145.0 ± 15.0		10.0 ± 4.0	330 ± 30
DH Tau b⁽⁵⁾	M0,5	~140	1.0 ± 0.9		330
2M 044144 b⁽⁶⁾	M8,5	140.0	1.0	7.5 ± 2.5	15.0 ± 0.6
CHXR 73 b⁽⁷⁾	M3,25	~1.6	2		200
2M1207 b⁽⁸⁾	M8	52.4 ± 1.1	8 ± 3		46.0 ± 5.0
VHS 1256-1257 B⁽⁹⁾	M7.5	12.7 ± 1.0	150−300		102 ± 9
Ross 458(AB) c⁽¹⁰⁾	M2	114.0 ± 2.0	475 ± 325	8.5 ± 2.5	1168.0
ROXs 42B b⁽¹¹⁾	M0	135.0	2 ± 1	10.0 ± 4.0	140.0 ± 10.0

Brown dwarfs

1RXS J034231.8+121622 B⁽¹²⁾	M4V	23.9 ± 1.1	60−300	35 ± 8	19.8 ± 0.9
FU Tau b⁽¹³⁾	M7,25	140.0	1.0	15.0	800
CD-35 2722 b⁽¹⁴⁾	M1V	21.3 ± 1.4	100 ± 50	31.0 ± 8.0	67.0 ± 4.0
GJ 3629 B⁽¹²⁾	M3V	22 ± 3		46 ± 6	6.5 ± 0.5
2MASS J15594729+4403595 B⁽¹²⁾	M2	33 ± 4	120	43 ± 9	187 ± 23
UScoCTIO 108 b⁽¹⁵⁾	M7	145.0 ± 2.0	11 ± 2		670.0
GSC 6214-210 b⁽¹⁶⁾	M1	145.0 ± 14.0	11 ± 2	17.0 ± 3.0	320.0
Oph 11 b⁽¹⁷⁾	M9	145.0 ± 20.0	11 ± 2	21.0 ± 3.0	243 ± 55.0
1RXS J235133.3+312720 B⁽¹²⁾	M2	50 ± 10	120	32.0 ± 6.0	120 ± 20

Reference.

⁽¹⁾

Delorme et al. (2013);

⁽²⁾

Naud et al. (2014);

⁽³⁾

Artigau et al. (2015);

⁽⁴⁾

Kraus et al. (2014a);

⁽⁵⁾

Itoh et al. (2005);

⁽⁶⁾

Todorov et al. (2010);

⁽⁷⁾

Luhman et al. (2006);

⁽⁸⁾

Chauvin et al. (2004);

⁽⁹⁾

Gauza et al. (2015);

⁽¹⁰⁾

Burgasser et al. (2010);

⁽¹¹⁾

Currie et al. (2014);

⁽¹²⁾

Bowler et al. (2015);

⁽¹³⁾

Luhman et al. (2009);

⁽¹⁴⁾

Wahhaj et al. (2011);

⁽¹⁵⁾

Béjar et al. (2009);

⁽¹⁶⁾

Ireland et al. (2011);

⁽¹⁷⁾

Allers et al. (2006).

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