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Early time-series photometry from NASA's Kepler spacecraft has revealed a planet transiting the star we term Kepler-4, at RA = 19h02m27.68s, Dec = +50:08:08.7. The planet has an orbital period of 3.213 days and shows transits with a…

We present the results of 45 transit observations obtained for the transiting exoplanet HAT-P-32b. The transits have been observed using several telescopes mainly throughout the YETI network. In 25 cases, complete transit light curves with…

We report on the discovery of HAT-P-10b, the lowest mass (0.46 +/- 0.03 MJ) transiting extrasolar planet (TEP) discovered to date by transit searches. HAT-P-10b orbits the moderately bright V=11.89 K dwarf GSC 02340-01714, with a period P =…

We present Transit Timing Variations (TTVs) of HAT-P-12b, a low-density sub-Saturn mass planet orbiting a metal-poor K4 dwarf star. Using 14 years of observational data (2009-2022), our study incorporates 7 new ground-based photometric…

Transiting planets in nearby young clusters offer the opportunity to study the atmospheres and dynamics of planets during their formative years. To this end, we focused on K2-25b -- a close-in ($P$=3.48 days), Neptune-sized exoplanet…

We report the discovery of a transiting, Rp = 4.347+/-0.099REarth, circumbinary planet (CBP) orbiting the Kepler K+M Eclipsing Binary (EB) system KIC 12351927 (Kepler-413) every ~66 days on an eccentric orbit with ap = 0.355+/-0.002AU, ep =…

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…

天体物理学 · 物理学 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 two exoplanets transiting high-jitter stars. HAT-P-32b orbits the bright V=11.289 star GSC 3281-00800, with a period P = 2.150008 d. The stellar and planetary masses and radii depend on the eccentricity of the…

We refined the ephemeris of seven transiting exoplanets HAT-P-6b, HAT-P-12b, HAT-P-18b, HAT-P-22b, HAT-P-32b, HAT-P-33b, and HAT-P-52b. We observed 11 transits from eight observatories in different filters for HAT-P-6b and HAT-P-32b. Also,…

We report the discovery of a Neptune-size (R_p = 3.87 +/- 0.06 R_Earth) transiting circumbinary planet, Kepler-1661 b, found in the Kepler photometry. The planet has a period of ~175 days and its orbit precesses with a period of only 35…

We present the first secondary eclipse and phase curve observations for the highly eccentric hot Jupiter HAT-P-2b in the 3.6, 4.5, 5.8, and 8.0 \mu m bands of the Spitzer Space Telescope. The 3.6 and 4.5 \mu m data sets span an entire…

We report Spitzer/IRAC photometry of the transiting giant exoplanet HAT-P-1b during its secondary eclipse. This planet lies near the postulated boundary between the pM and pL-class of hot Jupiters, and is important as a test of models for…

About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot…

地球与行星天体物理 · 物理学 2020-09-30 James S. Jenkins , Matías R. Díaz , Nicolás T. Kurtovic , Néstor Espinoza , Jose I. Vines , Pablo A. Peña Rojas , Rafael Brahm , Pascal Torres , Pía Cortés-Zuleta , Maritza G. Soto , Eric D. Lopez , George W. King , Peter J. Wheatley , Joshua N. Winn , David R. Ciardi , George Ricker , Roland Vanderspek , David W. Latham , Sara Seager , Jon M. Jenkins , Charles A. Beichman , Allyson Bieryla , Christopher J. Burke , Jessie L. Christiansen , Christopher E. Henze , Todd C. Klaus , Sean McCauliff , Mayuko Mori , Norio Narita , Taku Nishiumi , Motohide Tamura , Jerome Pitogo de Leon , Samuel N. Quinn , Jesus Noel Villaseñor , Michael Vezie , Jack J. Lissauer , Karen A. Collins , Kevin I. Collins , Giovanni Isopi , Franco Mallia , Andrea Ercolino , Cristobal Petrovich , Andrés Jordán , Jack S. Acton , David J. Armstrong , Daniel Bayliss , François Bouchy , Claudia Belardi , Edward M. Bryant , Matthew R. Burleigh , Juan Cabrera , Sarah L. Casewell , Alexander Chaushev , Benjamin F. Cooke , Philipp Eigmüller , Anders Erikson , Emma Foxell , Boris T. Gänsicke , Samuel Gill , Edward Gillen , Maximilian N. Günther , Michael R. Goad , Matthew J. Hooton , James A. G. Jackman , Tom Louden , James McCormac , Maximiliano Moyano , Louise D. Nielsen , Don Pollacco , Didier Queloz , Heike Rauer , Liam Raynard , Alexis M. S. Smith , Rosanna H. Tilbrook , Ruth Titz-Weider , Oliver Turner , Stéphane Udry , Simon. R. Walker , Christopher A. Watson , Richard G. West , Enric Palle , Carl Ziegler , Nicholas Law , Andrew W. Mann

We report the discovery of a sub-Jupiter mass exoplanet transiting a magnitude V=11.7 host star 1SWASP J030928.54+304024.7. A simultaneous fit to the transit photometry and radial-velocity measurements yield a planet mass M_p=0.53+-0.07M_J,…

TOI-1422 is a G2 V star ($V = 10.6$ mag) known to host a warm Neptune-sized planet, TOI-1422 b, with a mass and radius of about $9M_{\oplus}$ and $4R_{\oplus}$, on a circular orbit with a period of $12.997$ days. An outer planetary…

We present new transit observations acquired between 2014 and 2018 for the hot exoplanets GJ 436 b, HAT-P-3 b, HAT-P-19 b, WASP-3 b, and XO-2 b. New mid-transit times extend the timespan covered by observations of these exoplanets and allow…

地球与行星天体物理 · 物理学 2018-11-28 G. Maciejewski , M. Stangret , J. Ohlert , C. S. Basaran , J. Maciejczak , M. Puciata-Mroczynska , E. Boulanger

We report the discovery of HATS-2b, the second transiting extrasolar planet detected by the HATSouth survey. HATS-2b is moving on a circular orbit around a V=13.6 mag, K-type dwarf star (GSC 6665-00236), at a separation of 0.0230 \pm 0.0003…

Transit events of extrasolar planets offer a wealth of information for planetary characterization. However, for many known targets, the uncertainty of their predicted transit windows prohibits an accurate scheduling of follow-up…

As part of the NASA EPOXI Mission of Opportunity, we observed seven known transiting extrasolar planet systems in order to construct time series photometry of extremely high phase coverage and precision. Here we present the results for four…