Warm terrestrial planet with half the mass of Venus transiting a nearby star

O. D. S. Demangeon; M. R. Zapatero Osorio; Y. Alibert; S. C. C. Barros; V. Adibekyan; H. M. Tabernero; A. Antoniadis-Karnavas; J. D. Camacho; A. Suárez Mascareño; M. Oshagh; G. Micela; S. G. Sousa; C. Lovis; F. A. Pepe; R. Rebolo; S. Cristiani; N. C. Santos; R. Allart; C. Allende Prieto; D. Bossini; F. Bouchy; A. Cabral; M. Damasso; P. Di Marcantonio; V. D’Odorico; D. Ehrenreich; J. Faria; P. Figueira; R. Génova Santos; J. Haldemann; N. Hara; J. I. González Hernández; B. Lavie; J. Lillo-Box; G. Lo Curto; C. J. A. P. Martins; D. Mégevand; A. Mehner; P. Molaro; N. J. Nunes; E. Pallé; L. Pasquini; E. Poretti; A. Sozzetti; S. Udry

doi:10.1051/0004-6361/202140728

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Volume 653 (September 2021)

A&A, 653 (2021) A41

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Table A.4

Kinematics of L 98-59 A

U	15.42 ± 0.22 km s⁻¹
V	10.31 ± 1.06 km s⁻¹
W	− 2.59 ± 0.34 km s⁻¹
P(thick)	2 %
P(thin)	98 %
P(halo)	0 %
Group membership	Thin disk

Notes. U,V, W are the three velocity components in the solar reference frame. P(thin), P(thick), and P(halo) are the probability of L 98-59 A of belonging to the thin disk, the thick disk, and the galactic halo, respectively.

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