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The discovery of the short-period giant exoplanet population, the so-called hot Jupiter population, and their link to brown dwarfs and low-mass stars challenges the conventional view of planet formation and evolution. We took advantage of…

NASA's Kepler mission identified over 4000 extrasolar planets that transit (cross in front of) their host stars. This sample has revealed detailed features in the demographics of planet sizes and orbital spacings. However, knowledge of…

地球与行星天体物理 · 物理学 2025-07-11 Gregory J. Gilbert , Erik A. Petigura , Paige M. Entrican

We present a study of the relative sizes of planets within the multiple candidate systems discovered with the $Kepler$ mission. We have compared the size of each planet to the size of every other planet within a given planetary system after…

The analysis of the CoRoT space mission data was performed aiming to test a method that selects, among the several light curves observed, the transiting systems that likely host a low-mass star orbiting the main target. The method…

太阳与恒星天体物理 · 物理学 2011-04-01 Ronaldo Da Silva , Adriana Silva-Valio

Context. The pioneer space mission for photometric planet searches, CoRoT, steadily monitors about 12,000 stars in each of its fields of view; it is able to detect transit candidates early in the processing of the data and before the end of…

We have performed an extensive search for planet candidates in the publicly available Kepler Long Cadence data from quarters Q1 through Q6. The search method consists of initial de-trending of the data, applying the trend filtering…

地球与行星天体物理 · 物理学 2012-11-28 Xu Huang , Gáspár Á. Bakos , Joel D. Hartman

The vast majority of the 4700 confirmed planets and planet candidates discovered by the Kepler mission were first found by the Kepler pipeline. In the pipeline, after a transit signal is found, all data points associated with those transits…

地球与行星天体物理 · 物理学 2017-04-05 Joseph R. Schmitt , Jon M. Jenkins , Debra A. Fischer

We report on the masses, sizes, and orbits of the planets orbiting 22 Kepler stars. There are 49 planet candidates around these stars, including 42 detected through transits and 7 revealed by precise Doppler measurements of the host stars.…

地球与行星天体物理 · 物理学 2014-01-20 Geoffrey W. Marcy , Howard Isaacson , Andrew W. Howard , Jason F. Rowe , Jon M. Jenkins , Stephen T. Bryson , David W. Latham , Steve B. Howell , Thomas N. Gautier , Natalie M. Batalha , Leslie A. Rogers , David Ciardi , Debra A. Fischer , Ronald L. Gilliland , Hans Kjeldsen , Jørgen Christensen-Dalsgaard , Daniel Huber , William J. Chaplin , Sarbani Basu , Lars A. Buchhave , Samuel N. Quinn , William J. Borucki , David G. Koch , Roger Hunter , Douglas A. Caldwell , Jeffrey Van Cleve , Rea Kolbl , Lauren M. Weiss , Erik Petigura , Sara Seager , Timothy Morton , John Asher Johnson , Sarah Ballard , Chris Burke , William D. Cochran , Michael Endl , Phillip MacQueen , Mark E. Everett , Jack J. Lissauer , Eric B. Ford , Guillermo Torres , Francois Fressin , Timothy M. Brown , Jason H. Steffen , David Charbonneau , Gibor S. Basri , Dimitar D. Sasselov , Joshua Winn , Roberto Sanchis-Ojeda , Jessie Christiansen , Elisabeth Adams , Christopher Henze , Andrea Dupree , Daniel C. Fabrycky , Jonathan J. Fortney , Jill Tarter , Matthew J. Holman , Peter Tenenbaum , Avi Shporer , Philip W. Lucas , William F. Welsh , Jerome A. Orosz , T. R. Bedding , T. L. Campante , G. R. Davies , Y. Elsworth , R. Handberg , S. Hekker , C. Karoff , S. D. Kawaler , M. N. Lund , M. Lundkvist , T. S. Metcalfe , A. Miglio , V. Silva Aguirre , D. Stello , T. R. White , Alan Boss , Edna Devore , Alan Gould , Andrej Prsa , Eric Agol , Thomas Barclay , Jeff Coughlin , Erik Brugamyer , Fergal Mullally , Elisa V. Quintana , Martin Still , Susan E. hompson , David Morrison , Joseph D. Twicken , Jean-Michel Désert , Josh Carter , Justin R. Crepp , Guillaume Hébrard , Alexandre Santerne , Claire Moutou , Charlie Sobeck , Douglas Hudgins , Michael R. Haas , Paul Robertson , Jorge Lillo-Box , David Barrado

(Abridged) NASA's Kepler mission has provided several thousand transiting planet candidates, yet only a small subset have been confirmed as true planets. Therefore, the most fundamental question about these candidates is the fraction of…

In the spring of 2009, the Kepler Mission commenced high-precision photometry on nearly 156,000 stars to determine the frequency and characteristics of small exoplanets, conduct a guest observer program, and obtain asteroseismic data on a…

地球与行星天体物理 · 物理学 2020-05-27 William J. Borucki

Aims. We present our re-analyze the Kepler photometric dataset, searching for planetary transits using an alternative processing pipeline to the one used by the Kepler Mission. Methods. The SARS pipeline was tested extensively by processing…

地球与行星天体物理 · 物理学 2015-06-05 Aviv Ofir , Stefan Dreizler

Planet formation theories predict a large but still undetected population of short-period terrestrial planets orbiting brown dwarfs. Should specimens of this population be discovered transiting relatively bright and nearby brown dwarfs, the…

地球与行星天体物理 · 物理学 2016-12-21 Matthias Y. He , Amaury H. M. J. Triaud , Michaël Gillon

We present the results of a search for planetary companions orbiting near hot Jupiter planet candidates (Jupiter-size candidates with orbital periods near 3 days) identified in the Kepler data through its sixth quarter of science…

Doppler planet searches have discovered that giant planets follow orbits with a wide range of orbital eccentricities, revolutionizing theories of planet formation. The discovery of hundreds of exoplanet candidates by NASA's Kepler mission…

We present an investigation of twelve candidate transiting planets from Kepler with orbital periods ranging from 34 to 207 days, selected from initial indications that they are small and potentially in the habitable zone (HZ) of their…

We investigate the role that planet detection order plays in the Kepler planet detection pipeline. The Kepler pipeline typically detects planets in order of descending signal strength (MES). We find that the detectability of transits…

地球与行星天体物理 · 物理学 2019-01-11 Jon K. Zink , Jessie L. Christiansen , Bradley M. S. Hansen

CoRoT, which was launched successfully on the 27th of December 2006, is the first space mission to have the search for planetary transits at the heart of its science programme. It is expected to be able to detect transits of planets with…

Context. Transit detection algorithms are mathematical tools used for detecting planets in the photometric data of transit surveys. In this work we study their application to space-based surveys. Aims: Space missions are exploring the…

地球与行星天体物理 · 物理学 2012-12-06 J. Cabrera , Sz. Csizmadia , A. Erikson , H. Rauer , S. Kirste

One of the objectives of the CoRoT mission is the search for transiting extrasolar planets using high-precision photometry, and the accurate characterization of their fundamental parameters. The CoRoT satellite consecutively observes…