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(Abridged) WASP-5b is a highly irradiated dense hot Jupiter orbiting a G4V star every 1.6 days. We observed two secondary eclipses of WASP-5b in the J, H and K bands simultaneously. Thermal emission of WASP-5b is detected in the J and K…

地球与行星天体物理 · 物理学 2014-05-08 Guo Chen , Roy van Boekel , Nikku Madhusudhan , Hongchi Wang , Nikolay Nikolov , Ulf Seemann , Thomas Henning

In the last few decades planet search surveys have been focusing on solar type stars, and only recently the high-mass regimes. This is mostly due to challenges arising from the lack of instrumental precision, and more importantly, the…

We report the discovery and characterization of TOI-2005b, a warm Jupiter on an eccentric (e~0.59), 17.3-day orbit around a V_mag = 9.867 rapidly rotating F-star. The object was detected as a candidate by TESS and the planetary nature of…

The hot Jupiter WASP-12b is one of the largest, hottest, and best-studied extrasolar planets. We revisit our recent analysis of WASP-12b's emission spectrum in light of near-infrared spectroscopic measurements which have been claimed to…

地球与行星天体物理 · 物理学 2013-04-26 Ian J. M. Crossfield , Travis Barman , Brad M. S. Hansen , Ichi Tanaka , Tadayuki Kodama

Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights into their atmospheres, but the properties of lower-mass exoplanets (sub-Neptune) remain largely unconstrained because of the challenges of…

Fast-rotating hot stars are challenging targets for exoplanet searches due to rotational broadening and stellar variability. Moreover, hot stars often exhibit pulsations, an additional source of scatter in both photometric and spectroscopic…

Two decades after the discovery of 51 Peg b, the formation processes and atmospheres of short-period gas giants remain poorly understood. Observations of eccentric systems provide key insights on those topics as they can illuminate how a…

地球与行星天体物理 · 物理学 2016-06-06 Julien de Wit , Nikole K. Lewis , Jonathan Langton , Gregory Laughlin , Drake Deming , Konstantin Batygin , Jonathan J Fortney

Giant planets on long period orbits around the nearest stars are among the easiest to directly image. Unfortunately these planets are difficult to fully constrain by indirect methods, e.g., transit and radial velocity (RV). In this study,…

We report the discovery of WASP-190b, an exoplanet on a 5.37-day orbit around a mildly-evolved F6 IV-V star with V = 11.7, T_eff = 6400 $\pm$ 100 K, M$_{*}$ = 1.35 $\pm$ 0.05 M_sun and R$_{*}$ = 1.6 $\pm$ 0.1 R_sun. The planet has a radius…

We report Gemini Planet Imager H band high-contrast imaging/integral field spectroscopy and polarimetry of the HD 100546, a 10 $Myr$-old early-type star recently confirmed to host a thermal infrared bright (super)jovian protoplanet at wide…

地球与行星天体物理 · 物理学 2015-12-02 Thayne Currie , Ryan Cloutier , Sean Brittain , Carol Grady , Adam Burrows , Takayuki Muto , Scott J. Kenyon , Marc J. Kuchner

We report the discovery by the WASP transit survey of a giant planet in a close orbit (0.0295+-0.0009 AU) around a moderately bright (V=11.6, K=10) G9 dwarf (0.89+-0.08 M_sun, 0.84+-0.03 R_sun) in the Southern constellation Eridanus. Thanks…

We report detection of thermal emission from the exoplanet WASP-19b at 3.6, 4.5, 5.8 and 8.0 micron. We used the InfraRed Array Camera on the Spitzer Space Telescope to observe two occultations of WASP-19b by its host star. We combine our…

Direct imaging has just started the inventory of the population of gas giant planets on wide-orbits around young stars in the solar neighborhood. Following this approach, we carried out a deep imaging survey in the near-infrared using…

We present the discovery and characterization of five hot and warm Jupiters -- TOI-628 b (TIC 281408474; HD 288842), TOI-640 b (TIC 147977348), TOI-1333 b (TIC 395171208, BD+47 3521A), TOI-1478 b (TIC 409794137), and TOI-1601 b (TIC…

地球与行星天体物理 · 物理学 2021-03-31 Joseph E. Rodriguez , Samuel N. Quinn , George Zhou , Andrew Vanderburg , Louise D. Nielsen , Robert A. Wittenmyer , Rafael Brahm , Phillip A. Reed , Chelsea X. Huang , Sydney Vach , David R. Ciardi , Ryan J. Oelkers , Keivan G. Stassun , Coel Hellier , B. Scott Gaudi , Jason D. Eastman , Karen A. Collins , Allyson Bieryla , Sam Christian , David W. Latham , Ilaria Carleo , Duncan J. Wright , Elisabeth Matthews , Erica J. Gonzales , Carl Ziegler , Courtney D. Dressing , Steve B. Howell , Thiam-Guan Tan , Justin Wittrock , Peter Plavchan , Kim K. McLeod , David Baker , Gavin Wang , Don Radford , Richard P. Schwarz , Massimiliano Esposito , George R. Ricker , Roland K. Vanderspek , Sara Seager , Joshua N. Winn , Jon M. Jenkins , Brett Addison , D. R. Anderson , Thomas Barclay , Thomas G. Beatty , Perry Berlind , Francois Bouchy , Michael Bowen , Brendan P. Bowler , C. E. Brasseur , César Briceño , Douglas A. Caldwell , Michael L. Calkins , Priyanka Chaturvedi , Guillaume Chaverot , Sudhish Chimaladinne , Jessie L. Christiansen , Kevin Collins , Ian J. M. Crossfield , Kevin Eastridge , N'estor Espinoza , Gilbert A. Esquerdo , Dax Feliz , Tyler Fenske , William Fong , Tianjun Gan , Steven Giacalone , Holden Gill , Lindsey Gordon , Alex Granados , Nolan Grieves , Eike W. Guenther , Natalia Guerrero , Thomas Henning , Christopher E. Henze , Katharine Hesse , Melissa J. Hobson , Jonathan Horner , David J. James , Eric L. N. Jensen , Mary Jimenez , Andrés Jordán , Stephen R. Kane , John Kielkopf , Kingsley Kim , Rudolf B. Kuhn , Natasha Latouf , Nicholas M. Law , Alan M. Levine , Michael B. Lund , Andrew W. Mann , Shude Mao , Rachel A. Matson , Scott McDermott , Matthew W. Mengel , Jessica Mink , Patrick Newman , Tanner O'Dwyer , Jack Okumura , Enric Palle , Joshua Pepper , Elisa V. Quintana , Paula Sarkis , Arjun Savel , Joshua E. Schlieder , Chloe Schnaible , Avi Shporer , Ramotholo Sefako , Julia Seidel , Robert J. Siverd , Brett Skinner , Manu Stalport , Daniel J. Stevens , Caitlin Stibbards , C. G. Tinney , R. G. West , Daniel A. Yahalomi , Hui Zhang

Close-in giant exoplanets with temperatures greater than 2,000 K (''ultra-hot Jupiters'') have been the subject of extensive efforts to determine their atmospheric properties using thermal emission measurements from the Hubble and Spitzer…

We report the discovery of WASP-4b, a large transiting gas-giant planet with an orbital period of 1.34 days. This is the first planet to be discovered by the SuperWASP-South observatory and CORALIE collaboration and the first planet…

In this paper, the CoRoT Exoplanet Science Team announces its 14th discovery. Herein, we discuss the observations and analyses that allowed us to derive the parameters of this system: a hot Jupiter with a mass of $7.6 \pm 0.6$ Jupiter…