J/A+A/636/L6        HD 158259 SOPHIE radial velocities             (Hara+, 2020)

The SOPHIE search for northern extrasolar planets. XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain. Hara N.C., Bouchy F., Stalport M., Boisse I., Rodrigues J., Delisle J.-B., Santerne A., Henry G.W., Arnold L., Astudillo-Defru N., Borgniet S., Bonfils X., Bourrier V., Brugger B., Courcol B., Dalal S., Deleuil M., Delfosse X., Demangeon O., Diaz R.F., Dumusque X., Forveille T., Hebrard G., Hobson M.J., Kiefer F., Lopez T., Mignon L., Mousis O., Moutou C., Pepe F., Rey J., Santos N.C., Segransan D., Udry S., Wilson P.A. <Astron. Astrophys., 636, L6 (2020)> =2020A&A...636L...6H 2020A&A...636L...6H (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Stars, G-type ; Exoplanets ; Radial velocities ; Photometry Keywords: planets and satellites: detection - planets and satellites: dynamical evolution and stability - planets and satellites: fundamental parameters - planets and satellites: formation - methods: statistical - techniques: radial velocities Abstract: Since 2011, the SOPHIE spectrograph has been used to search for Neptunes and super-Earths in the northern hemisphere. As part of this observational program, 290 radial velocity measurements of the 6.4 V magnitude star HD 158259 were obtained. Additionally, TESS photometric measurements of this target are available. We present an analysis of the SOPHIE data and compare our results with the output of the TESS pipeline. The radial velocity data, ancillary spectroscopic indices, and ground-based photometric measurements were analyzed with classical and l1 periodograms. The stellar activity was modeled as a correlated Gaussian noise and its impact on the planet detection was measured with a new technique. The SOPHIE data support the detection of five planets, each with msini~=6M, orbiting HD 158259 in 3.4, 5.2, 7.9, 12, and 17.4 days. Though a planetary origin is strongly favored, the 17.4 d signal is classified as a planet candidate due to a slightly lower statistical significance and to its proximity to the expected stellar rotation period. The data also present low frequency variations, most likely originating from a magnetic cycle and instrument systematics. Furthermore, the TESS pipeline reports a significant signal at 2.17 days corresponding to a planet of radius ~=1.2R. A compatible signal is seen in the radial velocities, which confirms the detection of an additional planet and yields a ~=2M mass estimate. We find a system of five planets and a strong candidate near a 3:2 mean motion resonance chain orbiting HD 158259. The planets are found to be outside of the two and three body resonances. Description: Radial velocities of HD 158259 from SOPHIE spectrograph. Objects: ------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------- 17 25 24.06 +52 47 26.5 HD 158259 = TOI-1462 ------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file hd158259.dat 89 290 HD 158259 SOPHIE OHP observations -------------------------------------------------------------------------------- See also: J/A+A/505/853 : HD16760 radial velocity curve (Bouchy+, 2009) J/A+A/513/A69 : HD9446 radial velocity curve (Hebrard+, 2010) J/A+A/523/A88 : A Jupiter-mass companion around HD 109246 (Boisse+, 2010) J/A+A/538/A113 : RV of eight stars (Diaz+ 2012) J/A+A/545/A55 : RV of 5 stars (Boisse+, 2012) J/A+A/563/A22 : RV of 3 new hot Jupiters (Moutou+, 2014) J/A+A/585/A46 : RV of 5 stars (Bouchy+, 2016) J/A+A/588/A144 : RV of 15 targets (Wilson+, 2016) J/A+A/588/A145 : RV of 8 stars with giant planets (Hebrard+, 2016) J/A+A/601/A9 : HD17674, HD29021, and HD42012 radial velocities (Rey+, 2017) J/A+A/618/A103 : Gl617A and Gl96 radial velocity curves (Hobson+, 2018) J/A+A/625/A17 : SOPHIE data of Gliese 411 (Diaz+, 2019) Byte-by-byte Description of file: hd158259.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.4 d RJD Reduced Julian date (JD-2400000) 12- 18 F7.4 km/s RV Radial velocity 20- 25 F6.4 km/s e_RV Radial velocity photon plus instrument error 27- 32 F6.4 km/s FWHM Full width half maximum of the CCF 34- 40 F7.4 --- Cont Contrast of the CCF 42- 48 F7.4 km/s BisSpan Bisector slope span of the CCF 50- 55 F6.4 km/s noise Photon noise 57- 62 F6.2 --- sn10 Signal to noise ratio on echelle order 10 64- 69 F6.2 --- sn50 Signal to noise ratio on echelle order 50 71- 76 F6.2 --- sn60 Signal to noise ratio on echelle order 60 78- 84 A7 --- RHK log R'HK 86- 89 F4.2 --- e_RHK Error on log R'HK -------------------------------------------------------------------------------- Acknowledgements: Nathan Hara, Nathan.Hara(at)unige.ch Francois Bouchy, francois.bouchy(at)unige.ch [University of Geneva, Switzerland] Isabelle Boisse, Isabelle.boisse(at)lam.r Alexandre Santerne, Alexandre. Santerne(at)lam.r [Laboratoire d'astrophysique de Marseille, France] References: Bouchy et al., Paper I 2009A&A...505..853B 2009A&A...505..853B, Cat. J/A+A/505/853 Hebrard et al., Paper II 2010A&A...513A..69H 2010A&A...513A..69H, Cat. J/A+A/513/A69 Boisse et al., Paper III 2010A&A...523A..88B 2010A&A...523A..88B, Cat. J/A+A/535/A88 Diaz et al., Paper IV 2012A&A...538A.113D 2012A&A...538A.113D, Cat. J/A+A/538/A113 Boisse et al., Paper V 2012A&A...545A..55B 2012A&A...545A..55B, Cat. J/A+A/545/A55 Moutou et al., Paper VI 2014A&A...563A..22M 2014A&A...563A..22M, Cat. J/A+A/563/A22 Courcol et al., Paper VII 2015A&A...581A..38C 2015A&A...581A..38C Bouchy et al., Paper VIII 2016A&A...585A..46B 2016A&A...585A..46B, Cat. J/A+A/585/A46 Wilson et al., Paper IX 2016A&A...588A.144W 2016A&A...588A.144W, Cat. J/A+A/588/A144 Hebrard et al., Paper X 2016A&A...588A.145H 2016A&A...588A.145H, Cat. J/A+A/588/A145 Diaz et al., Paper XI 2016A&A...591A.146D 2016A&A...591A.146D Rey et al., Paper XII 2017A&A...601A...9R 2017A&A...601A...9R, Cat. J/A+A/601/A9 Hobson et al., Paper XIII 2018A&A...618A.103H 2018A&A...618A.103H, Cat. J/A+A/618/A03 Diaz et al., Paper XIV 2019A&A...625A..17D 2019A&A...625A..17D, Cat. J/A+A/625/A17 Hobson et al., Paper XV 2019A&A...625A..18H 2019A&A...625A..18H
(End) Patricia Vannier [CDS] 08-Feb-2021
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