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

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Table B.4

Identified signals as rotation signatures

Star	FAP	P(d)	P_E (d)	P_P (d)	Method	Reference
GJ 87	0.004	53.15	72.6	53.05	Hα	Mignon et al. (2023)

GJ 205	0.0	27.2	21.1	20.	Ph	Hébrard et al. (2016)
				33.4	Ph	Suárez Mascareño et al. (2016)
				35	Hα, Ca	Mignon et al. (2023)

GJ 229	0.0	27.60	25.3	27.3	Ph	Suárez Mascareño et al. (2016)
				27.6	Hα, NaD, Ca	Mignon et al. (2023)
	0.007	26.51		26.3	Ca	Mignon et al. (2023)

GJ 358	0.0	24.96	21.2	25.4	Ph	Hébrard et al. (2016)

GJ 388	0.0	2.23	-	2.23	VR	Morin et al. (2008)

GJ 393	0.0	38.5	44.6	37.2	Ca	Mignon et al. (2023)
	0.0	33.7

GJ 406	0.0	2.69	-		Ph	Díez Alonso et al. (2019)

GJ 447	0.0	61.9	100	123	VR	Bonfils et al. (2018a)
				111	Hα	Mignon et al. (2023)

GJ 479	0.0	23.10	28.7	24	Ph	Hébrard et al. (2016)
				22.5	Ch	Suárez Mascareño et al. (2015)
	0.01	11.27

GJ 514	0.0	31.4	33.9		Ch	Suárez Mascareño et al. (2015)
	0.0	32.4		34.0	Ca, NaD	Mignon et al. (2023)
	0.0	15.15		15.1	Hα, NaD, Ca	Mignon et al. (2023)

GJ 536	0.0	43.9	32.6	43.1	Ph	Suárez Mascareño et al. (2016)
				39.	Hα, Ca	Mignon et al. (2023)
				49.	NaD	Mignon et al. (2023)

GJ 551	0.0	114	28.4		Ca, NaD, Hα	Mignon et al. (2023)
	0.0	44.6		83		Kiraga & Stepien (2007)

GJ 581	0.0	67	114	127	Ca, NaD, Hα	Mignon et al. (2023)

GJ 628	0.0	48.3	92.6	93	VR	Astudillo-Defru et al. (2017b)
	0.0	186

GJ 667C	0.0	90.9	73	90	VR	Robertson & Mahadevan (2014)
	0.001	38.9
	0.003	82.4

GJ 674	0.0	36.68	33.3	33.9	Ch	Suárez Mascareño et al. (2015)
	0.007	35.62			Ph	Suárez Mascareño et al. (2016)
				35.2	Hα, Ca	Mignon et al. (2023)
	0.009	16.9

GJ 740	0.002	17.58	23.4			Toledo-Padrön et al. (2021)
				18.2	Ca	Mignon et al. (2023)
				37.2	Hα	Mignon et al. (2023)

GJ 832	0.005	36.73	50	35.8	Ca	Mignon et al. (2023)
				35.4	Hα	Mignon et al. (2023)

GJ 849	0.0	35.8	58	39.2	Ch	Suárez Mascareño et al. (2015)
				39.2	Hα, Ca	Mignon et al. (2023)

GJ 880	0.001	40.17	25.8	37.5	Ch	Suárez Mascareño et al. (2015)
				37	Hα, NaD, Ca	Mignon et al. (2023)

GJ 1132	0.0	62.6	63	125	VR	Bonfils et al. (2018a)

GJ 3148	0.0	11.14	16.2		-	-
	0.0	5.67			-	-

GJ 4303	0.002	17.63	15.5	17.5	Hα, NaD, Ca	Mignon et al. (2023)

Notes. The three periods are i) the period found in the frequency analysis of the RV time series (P), ii) the estimation of the rotation period obtained by the relation with the mean activity level of Astudillo-Defru et al. (2017a) (P_E), and iii) the period found in the literature (P_P). The 0.0 FAP value corresponds to a value under the 10⁻³ threshold.

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