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相关论文: The Exoplanet Orbit Database II: Updates to exopla…

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We present a database of well determined orbital parameters of exoplanets. This database comprises spectroscopic orbital elements measured for 427 planets orbiting 363 stars from radial velocity and transit measurements as reported in the…

We demonstrate the newly developed resource for exoplanet researchers - The Exoplanet Transit Database. This database is designed to be a web application and it is open for any exoplanet observer. It came on-line in September 2008. The ETD…

地球与行星天体物理 · 物理学 2014-11-20 Stanislav Poddaný , Luboš Brát , Ondřej Pejcha

We present a catalog of nearby exoplanets, available at http://exoplanets.org and ApJ 646, 505 (published version available at the link above). It contains the 172 known low mass companions with orbits established through radial velocity…

The current exoplanet database includes 5454 confirmed planets and candidate planets observed with the KEPLER mission. We find 932 planet pairs from which we extract distance and orbital period ratios. While earlier studies used the…

地球与行星天体物理 · 物理学 2017-09-26 Markus J. Aschwanden , Felix Scholkmann

We describe an online database for extra-solar planetary-mass candidates, updated regularly as new data are available. We first discuss criteria for the inclusion of objects in the catalog: "definition" of a planet and several aspects of…

地球与行星天体物理 · 物理学 2015-05-28 Jean Schneider , Cyrill Dedieu , Pierre Le Sidaner , Renaud Savalle , Ivan Zolotukhin

For much of human history we have wondered how our solar system formed, and whether there are any other planets like ours around other stars. Only in the last 20 years have we had direct evidence for the existence of exoplanets, with the…

太阳与恒星天体物理 · 物理学 2013-08-26 Jeffrey L. Coughlin

We describe the contents and functionality of the NASA Exoplanet Archive, a database and tool set funded by NASA to support astronomers in the exoplanet community. The current content of the database includes interactive tables containing…

Photometric survey data from the Kepler mission have been used to discover and characterize thousands of transiting exoplanet and eclipsing binary (EB) systems. These discoveries have enabled empirical studies of occurrence rates which…

地球与行星天体物理 · 物理学 2018-02-21 Daryll M. LaCourse , Thomas L. Jacobs

In this research, 14 light curves of 10 hot Jupiter exoplanets available on Exoplanet Transit Database (ETD) were analyzed. We extracted the transit parameters using EXOFAST software. Finally, we compared the planet's radius parameter…

地球与行星天体物理 · 物理学 2020-06-14 F. Davoudi , A. Poro , E. Paki , P. Mirshafie , F. Ahangarani , A. Farahani , M. Roshana , F. Abolhasani , Sh. Zamanpour , E. Lashgari , S. Modarres , A. Mohandes

The heterogeneity of papers dealing with the discovery and characterization of exoplanets makes every attempt to maintain a uniform exoplanet catalog almost impossible. Four sources currently available online (NASA Exoplanet Archive,…

地球与行星天体物理 · 物理学 2020-02-06 Eleonora Alei , Riccardo Claudi , Andrea Bignamini , Marco Molinaro

The number of extrasolar planets discovered is increasing, so that more than five thousand exoplanets have been confirmed to date. Now we have an opportunity to test the validity of the laws governing planetary systems and take steps to…

地球与行星天体物理 · 物理学 2024-02-29 Mahdiyar Mousavi-Sadr

The ExoClock project is an open platform aiming to monitor exoplanets by integrating observations from space and ground based telescopes. This study presents an updated catalogue of 620 exoplanet ephemerides, integrating 30000 measurements…

地球与行星天体物理 · 物理学 2025-11-19 A. Kokori , A. Tsiaras , G. Pantelidou , A. Jones , A. Siakas , B. Edwards , G. Tinetti , A. Wünsche , Y. Jongen , F. Libotte , M. Correa , L. V. Mugnai , A. Bocchieri , A. R. Capildeo , E. Poultourtzidis , C. Sidiropoulos , L. Bewersdorff , G. Lekkas , G. Grivas , R. A. Buckland , S. R. -L. Futcher , P. Matassa , J. -P. Vignes , A. O. Kovacs , M. Raetz , B. E. Martin , A. Popowicz , D. Gakis , P. Batsela , V. Michalaki , A. Nastasi , C. Pereira , A. Iliadou , F. Walter , N. I. Paschalis , K. Vats , N. A-thano , R. Abraham , V. K. Agnihotri , M. Á. Álava-Amat , R. Albanesi , T. Alderweireldt , J. Alonso-Santiago , D. Q. Amat , L. Andrade , V. Anzallo , J. Aragones , E. Arce-Mansego , D. Arnot , R. A. Artola , C. Aumasson , M. Bachschmidt , R. Barberá-Córdoba , J. -F. Barrois , P. R. Barroy , M. Bastoni , V. Béjar , A. A. Belinski , A. Ben Lassoued , P. Bendjoya , B. Benei , D. Bennett , K. Bernacki , G. O. Bernard , L. Betti , G. Biesse , M. Billiani , P. Bosch-Cabot , V. Boucher , R. C. Boufleur , D. Boulakos , P. J. -M. Brandebourg , S. M. Brincat , X. Bros , A. Brosio , S. Brouillard , A. -M. Bruzzone , L. Cabona , C. Calamai , G. Calapai , Y. Calatayud-Borràs , M. Caló , F. Campos , A. Carbognani , F. Carretero , R. Casas , M. L. Castanheira , G. Catanzaro , L. Cavaglioni , C. -M. Chang , M. Chella , W. -H. Chen , P. -J. Chiu , R. Ciantini , J. -F. Coliac , J. Collins , F. Conti , G. Conzo , W. R. Cooney, , L. N. Correa , S. P. Cosentino , N. Crouzet , M. V. Crow , B. V. -H. -V. da-Silva , A. Damonte , D. Daniel , S. Dawes , L. de Almeida , P. De Backer , A. de Melo , M. Deldem , D. Deligeorgopoulos , Y. Delisle , F. Denjean , F. Dias , S. Diaz Lopez , T. Dittadi , N. Dodd , S. Doman , G. Domènech-Rams , T. G. Dooley , S. Drapkin-Junyent , F. Dubois , A. Dustor , R. Dymock , T. Eenmäe , M. Emilio , E. Esparza-Borges , J. Estevez , C. Falco , R. G. Farfán , P. Farissier , G. Farrall , G. Fernandez Rodriguez , A. Ferretti , G. Ferrini , L. Fini , J. Fiołka , G. Fleerackers , J. Flores-Martín , g. follero , S. Foschino , L. Fossi , M. Fowler , A. Frasca , E. Frigeni , I. Fukuda , A. Fukui , G. Furlato , D. Gabellini , T. Gainey , P. Gajdoš , D. Galán-Diéguez , P. Gamache , E. García Navarro , N. A. Garcia , A. García-Sánchez , A. Garmash , T. Gesser , A. Ginard , I. Gkolias , E. Gomez , G. F. Gonçalves , J. González-Edo , J. González-Rodríguez , G. Gruntz , B. Guillet , T. Guillot , M. N. Günther , H. Hautecler , Y. Hayashi , E. Herrero , K. Hills , H. S. Hodkinson , G. Holtkamp , G. R. Hunt , N. Iannascoli , M. Iozzi , M. Irzyk , K. Isogai , K. Johnson , P. Jóźwik-Wabik , A. E. Kaeouach , S. Kartal , H. Kiiskinen , Ü. Kivila , U. Kolb , J. Korth , D. Kustrin , S. -P. Lai , S. Lasota , F. Le Rhun , Y. H. Lee , D. Lefoulon , F. Legrele , H. Leipold , A. Liberti , T. Lien , Y. -H. Lin , F. Linsalata , J. H. Livingston , C. Lopresti , S. Lora , E. R. Lorenz , D. Madison , M. Mannucci , A. Marchini , A. Marino , J. -C. Mario , E. Maris , J. -B. Marquette , N. A. Maslennikova , A. E. McGregor , A. Mengoudis , P. Meni , M. Mesarč , M. Michelagnoli , J. Michelet , J. Mieglitz , M. Mifsud , M. Miller , S. A. Mills , E. Miny , S. Miquel Romero , D. Molina , S. Montchaud , B. Monteleone , M. Monticelli , N. Montigiani , M. Morales-Aimar , G. Morello , L. Moretti , M. Mori , F. Mortari , M. Müller , D. Mura , F. Murgas , N. Narita , A. Nath , R. Nicollerat , V. Noce , P. Norridge , A. J. Norton , Y. Ogmen , Z. Orbanic , J. Owen-Lloyd-Walters , E. P. Pace , E. Pakštienė , A. F. Pala , E. Palle , C. Pantacchini , I. Parenti , D. Patterson , E. Pavoni , A. W. Pereira , I. Peretto , V. Perroud , S. W. Peterson , V. Pettina , M. Phillips , J. Philpot , D. Pica , P. Pintr , J. -B. Pioppa , T. J. Plunkett , T. G. Prado , A. Prasad , R. A. Prestes , A. Putz , F. Régembal , L. Ribe , D. F. Rocha , J. Rodrigues , R. Roth , L. Rousselot , N. Rozand , X. Rubia , N. Ruocco , M. Salisbury , T. Salomon , L. Sassaro , J. E. -G. Savage , T. Savin , F. Scaggiante , F. -X. Schmider , M. Serrau , I. D. Sharp , D. Shave-Wall , A. F. Silva , V. Školník , A. Solmaz , A. Sonka , M. Spiller , T. H. Sprecher , R. Stanga , M. Stefanini , D. Stouraitis , M. Stratigou-Psarra , O. Suarez , D. Suys , M. Szkudlarek , M. F. Talafha , A. N. Tarasenkov , G. Tartalo-Montardit , C. Titescu , A. Tomacelli , A. H. Triaud , S. Tsavdaridis , K. Tsiganis , M. A. van der Grijp , S. Vanaverbeke , j. -p. vergne , J. Verheyden , J. Vilalta , P. Vuylsteke , P. Wagner , D. Walliang , C. H. Wang , I. Weller , D. E. Wright , K. O. Xenos , R. Yorke , O. Zamora , J. Zapata , M. Zejmo , M. Zulian

We evaluate the extent to which newly detected exoplanetary systems containing at least four planets adhere to a generalized Titius-Bode (TB) relation. We find that the majority of exoplanet systems in our sample adhere to the TB relation…

地球与行星天体物理 · 物理学 2015-06-15 Timothy Bovaird , Charles H. Lineweaver

The Kepler mission has discovered over 2500 exoplanet candidates in the first two years of spacecraft data, with approximately 40% of them in candidate multi-planet systems. The high rate of multiplicity combined with the low rate of…

A new catalogue of extrasolar planets is presented by re-analysing a selection of published radial velocity data sets using EXOFIT (Balan & Lahav 2009). All objects are treated on an equal footing within a Bayesian framework, to give…

地球与行星天体物理 · 物理学 2012-12-20 Morgan D. J. Hollis , Sreekumar T. Balan , Greg Lever , Ofer Lahav

The Kepler Mission is exploring the diversity of planets and planetary systems. Its legacy will be a catalog of discoveries sufficient for computing planet occurrence rates as a function of size, orbital period, star-type, and insolation…

地球与行星天体物理 · 物理学 2014-09-08 Natalie M. Batalha

The high-precision photometry from NASA's Kepler and TESS missions has revolutionized exoplanet detection, enabling the discovery of over 5500 confirmed exoplanets via the transit method and around 10000 additional candidates awaiting…

地球与行星天体物理 · 物理学 2025-12-02 Sarah Huang , Chen Jiang

In this study, 19 exoplanets were studied. Their photometric observations were obtained from the ETD. After performing the data reduction steps, its parameters were obtained through Exofast online software. Then calculated orbital…

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