TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS

E. Martioli (1) , G. Hébrard (1) , P. Fouqué (2) , É. Artigau (3) , J.-F. Donati (2) , C. Cadieux (3) , S. Bellotti (2) , A. Lecavelier Des Etangs (1) , R. Doyon (3) , J.-D. Do Nascimento (4) , L. Arnold (5) , A. Carmona (6) , N. J. Cook (3) , P. Cortes-Zuleta (7) , L. de Almeida (4) , X. Delfosse (8) , C. P. Folsom (2) , P.-C. König (1) , C. Moutou (2) , M. Ould-Elhkim (2) , P. Petit (2) , K. G. Stassun (9) , A. A. Vidotto (10) , T. Vandal (3) , B. Benneke (11) , I. Boisse (1) , X. Bonfils (8) , P. Boyd (12) , C. Brasseur (13) , D. Charbonneau (14) , R. Cloutier (15) , K. Collins (16) , P. Cristofari , I. Crossfield (17) , R. F. Díaz (18) , M. Fausnaugh (19) , P. Figueira (20) , T. Forveille (8) , E. Furlan (21) , E. Girardin (22) , C. L. Gnilka (21) , J. Gomes da Silva (23) , P.-G. Gu (24) , P. Guerra (25) , S. B. Howell (26) , G. A. J. Hussain (27) , J. M. Jenkins (26) , F. Kiefer (1) , D. W. Latham (14) , R. A. Matson (28) , E. C. Matthews (29) , J. Morin (30) , R. Naves (25) , G. Ricker (19) , S. Seager (19) , M. Takami (31) , J. D. Twicken (26) , A. Vanderburg (19) , R. Vanderspek (19) , J. Winn (32)

1 IAP - Institut d'Astrophysique de Paris
2 IRAP - Institut de recherche en astrophysique et planétologie
3 UdeM - Université de Montréal
4 UFRN - Universidade Federal do Rio Grande do Norte [Natal]
5 CFHT - Canada-France-Hawaii Telescope Corporation
6 UGA - Université Grenoble Alpes
7 LAM - Laboratoire d'Astrophysique de Marseille
8 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble
9 Vanderbilt University [Nashville]
10 Universiteit Leiden = Leiden University
11 Département de Physique [Montréal]
12 UBC - University of British Columbia
13 STSci - Space Telescope Science Institute
14 CfA - Harvard-Smithsonian Center for Astrophysics
15 UQAR - Université du Québec à Rimouski
16 SETI Institute
17 University of Kansas [Kansas City]
18 International Center for Advanced Studies (ICAS) and ICIFI (CONICET)
19 MIT - Massachusetts Institute of Technology
20 ESO - European Southern Observatory
21 NExScI - NASA ExoPlanet Science Institute
22 Grand Pra Observatory
23 Universidade do Porto = University of Porto
24 Institute of Astronomy and Astrophysics, Academia Sinica, Taipei
25 Observatori Astronòmic Albanyà
26 ARC - NASA Ames Research Center
27 ESTEC - European Space Research and Technology Centre
28 U.S. Naval Observatory
29 ObsGE - Observatoire Astronomique de l'Université de Genève
30 LUPM - Laboratoire Univers et Particules de Montpellier
31 ASIAA - Academia Sinica Institute of Astronomy and Astrophysics
32 Peyton Hall

We report the detection and characterization of the transiting sub-Neptune TOI-1759 b, using photometric time series from the Transiting Exoplanet Survey Satellite (TESS) and near-infrared spectropolarimetric data from the Spectro-Polarimètre Infra Rouge (SPIRou) on the Canada-France-Hawaii Telescope. TOI-1759 b orbits a moderately active M0V star with an orbital period of 18.849975 ± 0.000006 days, and we measured a planetary radius and mass of 3.06 ± 0.22 R⊕ and 6.8 ± 2.0 M⊕. Radial velocities were extracted from the SPIRou spectra using both the cross-correlation function and the line-by-line methods, optimizing the velocity measurements in the near-infrared domain. We analyzed the broadband spectral energy distribution of the star and the high-resolution SPIRou spectra to constrain the stellar parameters and thus improve the accuracy of the derived planet parameters. A least squares deconvolution analysis of the SPIRou Stokes V polarized spectra detects Zeeman signatures in TOI-1759. We modeled the rotational modulation of the magnetic stellar activity using a Gaussian process regression with a quasi-periodic covariance function and find a rotation period of 35.65−0.15+0.17 days. We reconstructed the large-scale surface magnetic field of the star using Zeeman-Doppler imaging, which gives a predominantly poloidal field with a mean strength of 18 ± 4 G. Finally, we performed a joint Bayesian Markov chain Monte Carlo analysis of the TESS photometry and SPIRou radial velocities to optimally constrain the system parameters. At 0.1176 ± 0.0013 au from the star, the planet receives 6.4 times the bolometric flux incident on Earth, and its equilibrium temperature is estimated at 433 ± 14 K. TOI-1759 b is a likely gas-dominated sub-Neptune with an expected high rate of photoevaporation. Therefore, it is an interesting target to search for neutral hydrogen escape, which may provide important constraints on the planetary formation mechanisms responsible for the observed sub-Neptune radius desert.

Mots clés: planetary systems; stars: individual: TOI-1759; techniques: photometric; techniques: radial velocities; stars: magnetic field; planetary systems; planetary systems; planetary systems

Domaines: Astrophysique [astro-ph]

E. Martioli, G. Hébrard, P. Fouqué, É. Artigau, J.-F. Donati, et al.. TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS. Astronomy and Astrophysics - A&A, 2022, 660, pp.A86. ⟨10.1051/0004-6361/202142540⟩. ⟨hal-03647782⟩