J/A+A/703/A258ivo://CDS.VizieR/J/A+A/703/A258CDSUlmer-Moll S.Gill S.Brahm R.Claringbold A.Lendl M.Al Moulla K.,Anderson D.Battley M.Bayliss D.Bonfanti A.Bouchy F.Briceno C.,Bryant E.M.Burleigh M.R.Collins K.A.Deline A.Dumusque X.,Eberhardt J.Espinoza N.Falk B.Faria J.P.Fernandez Fernandez J.,Figueira P.Fridlund M.Furlan E.Goad M.R.Goeke R.F.Hagelberg J.,Hawthorn F.Helled R.Henning T.Hobson M.Howell S.B.,Jafariyazani M.Jenkins J.M.Jenkins J.S.Jones M.I.Jordan A.,Kendall A.Law N.Littlefield C.Mann A.W.McCormac J.Mordasini C.,Moyano M.Osborn H.Pezzotti C.Psaridi A.Quinn S.N.Rodel T.,Rodriguez J.E.Rojas F.Saha S.Schlecker M.Seager S.Sousa S.G.,Tala Pinto M.Trifonov T.Udry S.Vines J.I.Viviani G.Watson C.A.,Wheatley P.J.Wilson T.G.Winn J.N.Zhou G.Ziegler C.2026-03-02T06:25:50Z2025-11-24T09:31:27ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmultiple-starsdwarf-starsexoplanetsradial-velocityphotometryvisible-astronomyOnly a handful of transiting giant exoplanets with orbital periods longer than 100 days are known. These warm exoplanets are valuable objects as their radius and mass can be measured leading to an in-depth characterisation of the planet's properties. Thanks to low levels of stellar irradiation and large orbital distances, the atmospheric properties and orbital parameters of warm exoplanets remain relatively unaltered by their host star, giving new insights into planetary formation and evolution. We aim at extending the sample of warm giant exoplanets with precise radii and masses. Our goal is to identify suitable candidates in the Transiting Exoplanet Survey Satellite (TESS) data and perform follow-up observations with ground-based instruments. We use the Next Generation Transit Survey (NGTS) to detect additional transits of planetary candidates in order to pinpoint their orbital period. We also monitored the target with several high-resolution spectrographs to measure the planetary mass and eccentricity. We report the discovery of a 106-day period Jupiter-sized planet around the G-type star TOI-2449/NGTS-36. We jointly modelled the photometric and radial velocity data and find that the planet has a mass of 0.70M_{jup}_ and a radius of 1.002R_{jup}_. The planetary orbit has a semi-major axis of 0.449au and is slightly eccentric. We detect an additional 3-year signal in the radial velocity data likely due to the stellar magnetic cycle. Based on the planetary evolution models considered here, we find that TOI-2449 b/NGTS-36 b contains 11 Me of heavy elements and has a marginal planet-to-star metal enrichment of 3.3. Assuming a Jupiter-like Bond albedo, TOI-2449 b/NGTS-36 b has an equilibrium temperature of 400K and is a good target for understanding nitrogen chemistry in cooler atmospheres.2025A&A...703A.258Uhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/703/A258CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/703/A258https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/703/A258http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/703/A258https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/703/A258https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/703/A258http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/703/A258GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/703/A258/table1Radial velocities of TOI-2449recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBarycentric Julian datedtime.epochdoubleRVRadial velocitykm/sphys.veloc;pos.heliocentricdoublee_RVRadial velocity errorkm/sstat.errorfloatInstName of the instrument (CHIRON, CORALIE, FEROS or HARPS)meta.id;instrchar