The SOPHIE search for northern extrasolar planets XI. Three new companions and an orbit update: Giant planets in the habitable zone

R. F. Diaz , J. Rey (1) , O. Demangeon (2, 3) , G. Hébrard (4) , I. Boisse (5) , L. Arnold , N. Astudillo-Defru , J. -L. Beuzit (6) , X. Bonfils (6) , S. Borgniet (6) , F. Bouchy (7, 4) , V. Bourrier , B. Courcol , M. Deleuil (5) , X. Delfosse (6) , D. Ehrenreich (6) , T. Forveille (6) , A. -M. Lagrange (6) , M. Mayor (8) , C. Moutou (9, 5) , F. Pepe (8) , D. Queloz (8) , A. Santerne (10) , N. C. Santos (10, 11) , J. Sahlmann , D. Segransan (8) , S. Udry (8) , P. A. Wilson

1 DRCP - Département RadioChimie et Procédés
2 UP11 - Université Paris-Sud - Paris 11
3 IAS - Institut d'astrophysique spatiale
4 IAP - Institut d'Astrophysique de Paris
5 LAM - Laboratoire d'Astrophysique de Marseille
6 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble
7 OHP - Observatoire de Haute-Provence
8 ObsGE - Observatoire Astronomique de l'Université de Genève
9 CFHT - Canada-France-Hawaii Telescope Corporation
10 CAUP - Centro de Astrofísica da Universidade do Porto
11 DFA/FCUP - Departamento de Física e Astronomia [Porto]

We report the discovery of three new substellar companions to solar-type stars, HD191806, HD214823, and HD221585, based on radial velocity measurements obtained at the Haute-Provence Observatory. Data from the SOPHIE spectrograph are combined with observations acquired with its predecessor, ELODIE, to detect and characterise the orbital parameters of three new gaseous giant and brown dwarf candidates. Additionally, we combine SOPHIE data with velocities obtained at the Lick Observatory to improve the parameters of an already known giant planet companion, HD16175 b. Thanks to the use of different instruments, the data sets of all four targets span more than ten years. Zero-point off sets between instruments are dealt with using Bayesian priors to incorporate the information we possess on the SOPHIE/ELODIE off set based on previous studies. The reported companions have orbital periods between three and five years and minimum masses between 1.6 M-Jup and 19 M-Jup. Additionally, we find that the star HD191806 is experiencing a secular acceleration of over 11 m s(-1) per year, potentially due to an additional stellar or substellar companion. A search for the astrometric signature of these companions was carried out using HIPPARCOS data. No orbit was detected, but a significant upper limit to the companion mass can be set for HD221585, whose companion must be substellar. With the exception of HD191806 b, the companions are located within the habitable zone of their host star. Therefore, satellites orbiting these objects could be a propitious place for life to develop.

Domaines: Astrophysique [astro-ph]

R. F. Diaz, J. Rey, O. Demangeon, G. Hébrard, I. Boisse, et al.. The SOPHIE search for northern extrasolar planets XI. Three new companions and an orbit update: Giant planets in the habitable zone. Astronomy and Astrophysics - A&A, 2016, 591, ⟨10.1051/0004-6361/201628331⟩. ⟨hal-01440712⟩