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Related papers: NGTS-4b: A sub-Neptune Transiting in the Desert

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Context: The sub-Jovian or Neptunian desert is a previously-identified region of parameter space where there is a relative dearth of intermediate-mass planets at short orbital periods. Aims: We present the discovery of a new transiting…

HATS-8b is a low density transiting super-Neptune discovered as part of the HATSouth project. The planet orbits its solar-like G dwarf host (V=14.03 $\pm$ 0.10 and T$_{eff}$ =5679 $\pm$ 50 K) with a period of 3.5839 d. HATS-8b is the third…

We report the confirmation and mass determination of a mini-Neptune transiting the M3.5 V star TOI-4438 (G 182-34) every 7.44 days. A transit signal was detected with NASA's TESS space mission in the sectors 40, 52, and 53. In order to…

IW ../submit_V2/abstract.txt ( Row 1 Col 1 6:48 Ctrl-K H for help We report the discovery by the HATSouth network of HATS-7b, a transiting Super-Neptune with a mass of 0.120+/-0.012MJ, a radius of 0.563+/-(0.046,0.034)RJ, and an orbital…

This Letter reports on the photometric detection of transits of the Neptune-mass planet orbiting the nearby M-dwarf star GJ 436. It is by far the closest, smallest and least massive transiting planet detected so far. Its mass is slightly…

Astrophysics · Physics 2010-03-01 M. Gillon , F. Pont , B. -O. Demory , F. Mallmann , M. Mayor , T. Mazeh , D. Queloz , A. Shporer , S. Udry , C. Vuissoz

We report the discovery of the massive hot Jupiter NGTS-13b by the Next Generation Transit Survey (NGTS). The V = 12.7 host star is likely in the subgiant evolutionary phase with log g$_{*}$ = 4.04 $\pm$ 0.05, T$_{eff}$ = 5819 $\pm$ 73 K,…

We report on the discovery of HAT-P-11b, the smallest radius transiting extrasolar planet (TEP) discovered from the ground, and the first hot Neptune discovered to date by transit searches. HAT-P-11b orbits the bright (V=9.587) and metal…

The interiors of giant planets remain poorly understood. Even for the planets in the Solar System, difficulties in observation lead to large uncertainties in the properties of planetary cores. Exoplanets that have undergone rare…

Earth and Planetary Astrophysics · Physics 2020-07-17 David J. Armstrong , Théo A. Lopez , Vardan Adibekyan , Richard A. Booth , Edward M. Bryant , Karen A. Collins , Alexandre Emsenhuber , Chelsea X. Huang , George W. King , Jorge Lillo-box , Jack J. Lissauer , Elisabeth C. Matthews , Olivier Mousis , Louise D. Nielsen , Hugh Osborn , Jon Otegi , Nuno C. Santos , Sérgio G. Sousa , Keivan G. Stassun , Dimitri Veras , Carl Ziegler , Jack S. Acton , Jose M. Almenara , David R. Anderson , David Barrado , Susana C. C. Barros , Daniel Bayliss , Claudia Belardi , Francois Bouchy , César Briceno , Matteo Brogi , David J. A. Brown , Matthew R. Burleigh , Sarah L. Casewell , Alexander Chaushev , David R. Ciardi , Kevin I. Collins , Knicole D. Colón , Benjamin F. Cooke , Ian J. M. Crossfield , Rodrigo F. Díaz , Magali Deleuil , Elisa Delgado Mena , Olivier D. S. Demangeon , Caroline Dorn , Xavier Dumusque , Philipp Eigmuller , Michael Fausnaugh , Pedro Figueira , Tianjun Gan , Siddharth Gandhi , Samuel Gill , Michael R. Goad , Maximilian N. Guenther , Ravit Helled , Saeed Hojjatpanah , Steve B. Howell , James Jackman , James S. Jenkins , Jon M. Jenkins , Eric L. N. Jensen , Grant M. Kennedy , David W. Latham , Nicholas Law , Monika Lendl , Michael Lozovsky , Andrew W. Mann , Maximiliano Moyano , James McCormac , Farzana Meru , Christoph Mordasini , Ares Osborn , Don Pollacco , Didier Queloz , Liam Raynard , George R. Ricker , Pamela Rowden , Alexandre Santerne , Joshua E. Schlieder , S. Seager , Lizhou Sha , Thiam-Guan Tan , Rosanna H. Tilbrook , Eric Ting , Stéphane Udry , Roland Vanderspek , Christopher A. Watson , Richard G. West , Paul A. Wilson , Joshua N. Winn , Peter Wheatley , Jesus Noel Villasenor , Jose I. Vines , Zhuchang Zhan

Gliese 436 is an M dwarf with a mass of 0.45 Msun and hosts the extrasolar planet GL 436b [3, 6, 7, 2], which is currently the least massive transiting planet with a mass of ~23.17 Mearth [10], and the only planet known to transit an M…

We present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days a nearby M4.5V-type star, identified through photometric measurements from the TESS mission. The host star is located $33$ pc away with a radius of…

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