Radial velocity homogeneous analysis of M dwarfs observed with HARPS - I. Exoplanet detection and candidates

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Table 3

Sinusoidal model.

Star		Period (d)	K(m s⁻¹)	Ref.
GJ 179*	b	2288	22.10	Howard et al. (2010)
GJ 317	b	762	76.24	Johnson et al. (2007)
GJ 676A*	b	1056	166.47	Forveille et al. (2011)
GJ 832	b	3687	17.91	Bailey et al. (2008)
GJ 849*	b	1924	29.90	Butler et al. (2006)
GJ 3307		3539	970.41	This paper
GJ 4001		2672	571.92	This paper
GJ 4254*		1453	4595.92	This paper
GJ 4303		1267	47.92	This paper
GJ 9425*	c	1800	31.02	Moutou et al. (2011)
	b	700		Moutou et al. (2011)
GJ 9482*	b	6700	75.52	Segransan et al. (2011)
GJ 9588*		620	540.65	This paper

Notes. Targets dominated by a sinusoidal function. The last column gives the companion discovery reference, including the five in this work. Targets flagged with an asterisk correspond to those dominated by a linear trend in addition to the sinusoidal function.

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