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相关论文: TOI-2015b: A Warm Neptune with Transit Timing Vari…

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The Transiting Exoplanet Survey Satellite, TESS, is currently carrying out an all-sky search for small planets transiting bright stars. In the first year of the TESS survey, steady progress was made in achieving the mission's primary…

Sub-Neptunes with $2-3R_\oplus$ are intermediate in size between rocky planets and Neptune-sized planets. The orbital properties and bulk compositions of transiting sub-Neptunes provide clues to the formation and evolution of close-in small…

地球与行星天体物理 · 物理学 2024-05-22 Y. Hori , A. Fukui , T. Hirano , N. Narita , J. P. de Leon , H. T. Ishikawa , J. D. Hartman , G. Morello , N. Abreu García , L. Álvarez Hernández , V. J. S. Béjar , Y. Calatayud-Borras , I. Carleo , G. Enoc , E. Esparza-Borges , I. Fukuda , D. Galán , S. Geraldía-González , Y. Hayashi , M. Ikoma , K. Ikuta , K. Isogai , T. Kagetani , Y. Kawai , K. Kawauchi , T. Kimura , T. Kodama , J. Korth , N. Kusakabe , A. Laza-Ramos , J. H. Livingston , R. Luque , K. Miyakawa , M. Mori , S. Muñoz Torres , F. Murgas , J. Orell-Miquel , E. Palle , H. Parviainen , A. Peláez-Torres , M. Puig-Subirá , M. Sánchez-Benavente , P. Sosa-Guillén , M. Stangret , Y. Terada , N. Watanabe , G. Á. Bakos , K. Barkaoui , C. Beichman , Z. Benkhaldoun , A. W. Boyle , D. R. Ciardi , C. A. Clark , K. A. Collins , K. I. Collins , D. M. Conti , I. J. M. Crossfield , M. E. Everett , E. Furlan , M. Ghachoui , M. Gillon , E. J. Gonzales , J. Higuera , K. Horne , S. B. Howell , E. Jehin , K. V. Lester , M. B. Lund , R. Matson , E. C. Matthews , F. J. Pozuelos , B. S. Safonov , J. E. Schlieder , R. P. Schwarz , R. Sefako , G. Srdoc , I. A. Strakhov , W. C. Waalkes , C. Ziegler , D. Charbonneau , Z. Essack , M. Timmermans , N. M. Guerrero , H. Harakawa , C. Hedges , M. Ishizuka , J. M. Jenkins , M. Konishi , T. Kotani , T. Kudo , T. Kurokawa , M. Kuzuhara , J. Nishikawa , M. Omiya , G. R. Ricker , S. Seager , T. Serizawa , S. Striegel , M. Tamura , A. Ueda , R. Vanderspek , S. Vievard , J. N. Winn

Among the thousands of exoplanets discovered to date, approximately a few hundred gas giants on short-period orbits are classified as "lonely" and only a few are in a multi-planet system with a smaller companion on a close orbit. The…

Mapping the orbital obliquity distribution of young planets is one avenue towards understanding mechanisms that sculpt the architectures of planetary systems. TOI-942 is a young field star, with an age of ~60 Myr, hosting a planetary system…

We present the validation of two planets orbiting M dwarfs, TOI-1696b and TOI-2136b. Both planets are mini-Neptunes orbiting nearby stars, making them promising prospects for atmospheric characterization with the James Webb Space Telescope.…

We report the spectroscopic confirmation and fundamental properties of TOI-757 b, a mini-Neptune on a 17.5-day orbit transiting a bright star ($V = 9.7$ mag) discovered by the TESS mission. We acquired high-precision radial velocity…

地球与行星天体物理 · 物理学 2024-07-31 A. Alqasim , N. Grieves , N. M. Rosário , D. Gandolfi , J. H. Livingston , S. Sousa , K. A. Collins , J. K. Teske , M. Fridlund , J. A. Egger , J. Cabrera , C. Hellier , A. F. Lanza , V. Van Eylen , F. Bouchy , R. J. Oelkers , G. Srdoc , S. Shectman , M. Günther , E. Goffo , T. Wilson , L. M. Serrano , A. Brandeker , S. X. Wang , A. Heitzmann , A. Bonfanti , L. Fossati , Y. Alibert , L. Delrez , R. Sefako , S. Barros , K. I. Collins , O. D. S. Demangeon , S. H. Albrecht , R. Alonso , J. Asquier , T. Barczy , D. Barrado , W. Baumjohann , T. Beck , W. Benz , N. Billot , L. Borsato , C. Broeg , E. M. Bryant , R. P. Butler , W. D. Cochran , A. Collier Cameron , A. C. M. Correia , J. D. Crane , Sz. Csizmadia , P. E. Cubillos , M. B. Davies , T. Daylan , M. Deleuil , A. Deline , B. -O. Demory , A. Derekas , B. Edwards , D. Ehrenreich , A. Erikson , Z. Essack , A. Fortier , K. Gazeas , M. Gillon , M. Gudel , J. Hasiba , A. P. Hatzes , Ch. Helling , T. Hirano , S. B. Howell , S. Hoyer , K. G. Isaak , J. M. Jenkins , S. Kanodia , L. L. Kiss , J. Korth , K. W. F. Lam , J. Laskar , A. Lecavelier des Etangs , M. Lendl , M. B. Lund , R. Luque , A. W. Mann , D. Magrin , P. F. L. Maxted , C. Mordasini , N. Narita , V. Nascimbeni , G. Nowak , G. Olofsson , H. P. Osborn , H. L. M. Osborne , D. Osip , R. Ottensamer , I. Pagano , E. Palle , G. Peter , G. Piotto , D. Pollacco , D. Queloz , R. Ragazzoni , N. Rando , H. Rauer , S. Redfield , I. Ribas , M. Rice , G. R. Ricker , M. Rieder , S. Salmon , N. C. Santos , G. Scandariato , S. Seager , D. Segransan , A. Shporer , A. E. Simon , A. M. S. Smith , M. Stalport , Gy. M. Szabo , I. Thompson , J. D. Twicken , S. Udry , R. Vanderspek , V. Van Grootel , J. Venturini , E. Villaver , J. Villaseñor , V. Viotto , I. Walter , N. A. Walton , J. N. Winn , S. W. Yee

This paper presents multi-band photometric follow-up observations of the Neptune-mass transiting planet GJ 436b, consisting of 5 new ground-based transit light curves obtained in May 2007. Together with one already published light curve we…

The main scientific goal of TESS is to find planets smaller than Neptune around stars that are bright enough to allow for further characterization studies. Given our current instrumentation and detection biases, M dwarfs are prime targets…

The Transit Timing Variations (TTVs) can be used as a diagnostic of gravitational interactions between planets in a multi-planet system. Many Kepler Objects of Interest (KOIs) exhibit significant TTVs, but KOI-142.01 stands out among them…

地球与行星天体物理 · 物理学 2015-06-15 David Nesvorny , David Kipping , Dirk Terrell , Joel Hartman , Gaspar A. Bakos , Lars A. Buchhave

We report the confirmation of a transiting planet around the bright, inactive M0.5 V star TOI-1235 (TYC 4384-1735-1, V = 11.5 mag), whose transit signal was detected in the photometric time series of Sectors 14, 20, and 21 of the TESS space…

We report the discovery of a 1.32$^{+0.10}_{-0.10}$ $\mathrm{M_{\rm Jup}}$ planet orbiting on a 75.12 day period around the G3V $10.8^{+2.1}_{-3.6}$ Gyr old star TOI-5542 (TIC 466206508; TYC 9086-1210-1). The planet was first detected by…