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Bozhilov, V.; Antonova, D.; Hobson, M.J.; Brahm, R.; Jordan, A.; Henning, T.; Eberhardt, J.; Rojas, F.I.; Batygin, K.; Torres-Miranda, P.; Stassun, K.G.; Millholland, S.C.; Stoeva, D.; Minev, M.; Espinoza, N.; Ricker, G.R.; Latham, D.W.; Dragomir, D.; Kunimoto, M.; Jenkins, J.M.; Ting, E.B.; Seager, S.; Winn, J.N.; Villasenor, J.N.; Bouma, LG.; Medina, J.; Trifonov, T. |
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A 2:1 Mean-motion Resonance Super-Jovian Pair Revealed by TESS, FEROS, and HARPS |
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2023 |
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Astrophysical Journal Letters |
Abbreviated Journal |
Astrophys. J. Lett. |
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946 |
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2 |
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L36 |
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GIANT PLANETS; ECCENTRICITY; EVOLUTION; EXOPLANET; ORIGIN; MASS |
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We report the discovery of a super-Jovian 2:1 mean-motion resonance (MMR) pair around the G-type star TIC 279401253, whose dynamical architecture is a prospective benchmark for planet formation and orbital evolution analysis. The system was discovered thanks to a single-transit event recorded by the Transiting Exoplanet Survey Satellite mission, which pointed to a Jupiter-sized companion with poorly constrained orbital parameters. We began ground-based precise radial velocity (RV) monitoring with HARPS and FEROS within the Warm gIaNts with tEss survey to constrain the transiting body's period, mass, and eccentricity. The RV measurements revealed not one but two massive planets with periods of 76.80(-0.06)(+0.06) and 155.3(-0.7)(+0.7) days, respectively. A combined analysis of transit and RV data yields an inner transiting planet with a mass of 6.14(-0.42)(+0.39) M-Jup and a radius of 1.00(-0.04)(+0.04) R-Jup, and an outer planet with a minimum mass of 8.02(-0.18)(+0.18) M-Jup, indicating a massive giant pair. A detailed dynamical analysis of the system reveals that the planets are locked in a strong firstorder, eccentricity-type 2:1 MMR, which makes TIC 279401253 one of the rare examples of truly resonant architectures supporting disk-induced planet migration. The bright host star, V approximate to 11.9 mag, the relatively short orbital period (P-b = 76.80(-0.06)(+0.06) days), and pronounced eccentricity (e = 0.448(-0.029)(+0.029)) make the transiting planet a valuable target for atmospheric investigation with the James Webb Space Telescope and ground-based extremely large telescopes. |
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2041-8205 |
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WOS:000960668500001 |
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UAI @ alexi.delcanto @ |
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1833 |
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Jones, M.I.; Reinarz, Y.; Brahm, R .; Tala Pinto, M.; Eberhardt, J.; Rojas, F.; Triaud, A.H.M.J.; Gupta, A.F.; Ziegler, C.; Hobson, M.J.; Jordan, A.; Henning, T.; Trifonov, T.; Schlecker, M.; Espinoza, N.; Torres-Miranda, P.; Sarkis, P.; Ulmer-Moll, S.; Lendl, M.; Uzundag, M.; Moyano, M.; Hesse, K.; Caldwell, D.A.; Shporer, A.; Lund, M.B.; Jenkins, J.M.; Seager, S.; Winn, J.N.; Ricker, G.R.; Burke, C.J.; Figueira, P.; Psaridi, A.; Al Moulla, K.; Mounzer, D.; Standing, M.R.; Martin, D.V.; Dransfield, G.; Baycroft, T.; Dragomir, D.; Boyle, G.; Suc, V.; Mann, A.W.; Timmermans, M.; Ducrot, E.; Hooton, M.J.; Zuniga-Fernandez, S.; Sebastian, D.; Gillon, M.; Queloz, D.; Carson, J.; Lissauer, J.J. |
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A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS |
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2024 |
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Astronomy & Astrophysics |
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Astron. Astrophys. |
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683 |
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A192 |
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techniques: photometric; techniques: radial velocities; planets and satellites: composition; planets and satellites: detection; planets and satellites: formation; planets and satellites: gaseous planets |
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We report on the confirmation and follow-up characterization of two long-period transiting substellar companions on low-eccentricity orbits around TIC 4672985 and TOI-2529, whose transit events were detected by the TESS space mission. Ground-based photometric and spectroscopic follow-up from different facilities, confirmed the substellar nature of TIC 4672985 b, a massive gas giant in the transition between the super-Jupiters and brown dwarfs mass regime. From the joint analysis we derived the following orbital parameters: P = 69.0480(-0.0005)(+0.0004) d, M-p = 12.74(-1.01)(+1.01) M-J, R-p = 1.026(-0.067)(+0.065) R-J and e = 0.018(-0.004)(+0.004). In addition, the RV time series revealed a significant trend at the similar to 350 m s(-1) yr(-1) level, which is indicative of the presence of a massive outer companion in the system. TIC 4672985 b is a unique example of a transiting substellar companion with a mass above the deuterium-burning limit, located beyond 0.1 AU and in a nearly circular orbit. These planetary properties are difficult to reproduce from canonical planet formation and evolution models. For TOI-2529 b, we obtained the following orbital parameters: P = 64.5949(-0.0003)(+0.0003) d, M-p = 2.340(-0.195)(+0.197) M-J, R-p = 1.030(-0.050)(+0.050) R-J and e = 0.021(-0.015)(+0.024), making this object a new example of a growing population of transiting warm giant planets. |
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0004-6361 |
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WOS:001188136600004 |
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UAI @ alexi.delcanto @ |
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1978 |
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Sha, L.Z.; Vanderburg, A.M.; Huang, C.X.; Armstrong, D.J.; Brahm, R.; Giacalone, S.; Wood, M.L.; Collins, K.A.; Nielsen, L.D.; Hobson, M.J.; Ziegler, C.; Howell, S.B.; Torres-Miranda, P.; Mann, A.W.; Zhou, G.R.; Delgado-Mena, E.; Rojas, F.I.; Abe, L.; Trifonov, T.; Adibekyan, V.; Sousa, S.G.; Fajardo-Acosta, S.B.; Guillot, T.; Howard, S.; Littlefield, C.; Hawthorn, F.; Schmider, F.X.; Eberhardt, J.; Tan, T.G.; Osborn, A.; Schwarz, R.P.; Strom, P.; Jordan, A.; Wang, G.V.; Henning, T.; Massey, B.; Law, N.; Stockdale, C.; Furlan, E.; Srdoc, G.; Wheatley, P.J.; Navascues, D.B.; Lissauer, J.J.; Stassun, K.G.; Ricker, G.R.; Vanderspek, R.K.; Latham, D.W.; Winn, J.N.; Seager, S.; Jenkins, J.M.; Barclay, T.; Bouma, L.G.; Christiansen, J.L.; Guerrero, N.; Rose, M.E. |
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TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system |
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2023 |
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Monthly Notices Of The Royal Astronomical Society |
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Mon. Not. Roy. Astron. Soc. |
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524 |
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1 |
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1113-1138 |
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techniques: photometric; techniques: radial velocities; planets and satellites: detection; planets and satellites: formation; planets and satellites: gaseous planets; stars: individual: TOI-2000 (TIC 371188886) |
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Hot jupiters (P < 10 d, M > 60 M.) are almost always found alone around their stars, but four out of hundreds known have inner companion planets. These rare companions allow us to constrain the hot jupiter's formation history by ruling out high-eccentricity tidal migration. Less is known about inner companions to hot Saturn-mass planets. We report here the discovery of the TOI-2000 system, which features a hot Saturn-mass planet with a smaller inner companion. The mini-neptune TOI-2000 b (2.70 +/- 0.15 R-circle plus, 11.0 +/- 2.4 M.) is in a 3.10-d orbit, and the hot saturn TOI-2000 c (8.14(+0.31) (-0.30) R-circle plus, 81.7(-4.6)(+4.7) M.) is in a 9.13-d orbit. Both planets transit their host star TOI-2000 (TIC 371188886, V = 10.98, TESS magnitude = 10.36), a metal-rich ([Fe/H] = 0.439 (+0.041)(-0.043)) G dwarf 173 pc away. TESS observed the two planets in sectors 9-11 and 36-38, and we followed up with groundbased photometry, spectroscopy, and speckle imaging. Radial velocities from CHIRON, FEROS, and HARPS allowed us to confirm both planets by direct mass measurement. In addition, we demonstrate constraining planetary and stellar parameters with MIST stellar evolutionary tracks through Hamiltonian Monte Carlo under the PYMC framework, achieving higher sampling efficiency and shorter run time compared to traditional Markov chain Monte Carlo. Having the brightest host star in the V band among similar systems, TOI-2000 b and c are superb candidates for atmospheric characterization by the JWST, which can potentially distinguish whether they formed together or TOI-2000 c swept along material during migration to form TOI-2000 b. |
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0035-8711 |
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WOS:001038648500002 |
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UAI @ alexi.delcanto @ |
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1873 |
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