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Exoplanet research is at the forefront of contemporary astronomy recommendations. As more and more exoplanets are discovered and vetted, databases and catalogs are built to collect information. Various resources are available to scientists…

Exoplanet science often involves using the system parameters of real exoplanets for tasks such as simulations, fitting routines, and target selection for proposals. Several exoplanet catalogues are already well established but often lack a…

地球与行星天体物理 · 物理学 2016-09-21 Ryan Varley

In this study, we investigated the differences between four commonly-used exoplanet catalogs (exoplanet.eu; exoplanetarchive.ipac.caltech.edu; openexoplanetcatalogue.com; exoplanets.org) using a Kolmogorov-Smirnov (KS) test. We found a…

地球与行星天体物理 · 物理学 2018-08-31 Dolev Bashi , Ravit Helled , Shay Zucker

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…

I present a new kind of astronomical database based on small text files and a distributed version control system. This encourages the community to work collaboratively. It creates a decentralized, completely open and democratic way of…

地球与行星天体物理 · 物理学 2012-12-05 Hanno Rein

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

The Exoplanet Orbit Database (EOD) compiles orbital, transit, host star, and other parameters of robustly detected exoplanets reported in the peer-reviewed literature. The EOD can be navigated through the Exoplanet Data Explorer (EDE)…

地球与行星天体物理 · 物理学 2015-06-23 Eunkyu Han , Sharon X. Wang , Jason T. Wright , Y. Katherina Feng , Ming Zhao , Jacob I. Brown , Colin Hancock

We present the Exoplanet Simple Orbit Fitting Toolbox (ExoSOFT), a new, open-source suite to fit the orbital elements of planetary or stellar mass companions to any combination of radial velocity and astrometric data. To explore the…

天体物理仪器与方法 · 物理学 2017-11-13 Kyle Mede , Timothy D. Brandt

Context: Exoplanets have now been proven to be very common. The number of its detections continues to grow following the development of better instruments and missions. One key step for the understanding of these worlds is their…

The NASA Exoplanet Archive and the Exoplanet Follow-up Observing Program service are two widely used resources for the exoplanet community. The NASA Exoplanet Archive provides a complete and accurate accounting of exoplanetary systems…

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…

Exoplanet atmospheric retrieval is a computational technique widely used to infer properties of planetary atmospheres from remote spectroscopic observations. Retrieval codes typically employ Bayesian sampling algorithms or machine learning…

地球与行星天体物理 · 物理学 2023-03-24 Ryan J. MacDonald , Natasha E. Batalha

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

One of the most exciting developments in the field of exoplanets has been the progression from 'stamp-collecting' to demography, from discovery to characterisation, from exoplanets to comparative exoplanetology. There is an exhilaration…

地球与行星天体物理 · 物理学 2018-12-05 Jessie L. Christiansen

We introduce a general range of science drivers for using the Virtual Observatory (VO) and identify some common aspects to these as well as the advantages of VO data access. We then illustrate the use of existing VO tools to tackle multi…

天体物理仪器与方法 · 物理学 2009-06-09 Jonathan A. Tedds

SWEET-Cat (Stars With ExoplanETs Catalogue) was originally introduced in 2013, and since then, the number of confirmed exoplanets has increased significantly. A crucial step for a comprehensive understanding of these new worlds is the…

The ExoClock project has been created with the aim of increasing the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides of Ariel candidates over an extended period, in order to…

地球与行星天体物理 · 物理学 2023-02-22 A. Kokori , A. Tsiaras , B. Edwards , A. Jones , G. Pantelidou , G. Tinetti , L. Bewersdorff , A. Iliadou , Y. Jongen , G. Lekkas , A. Nastasi , E. Poultourtzidis , C. Sidiropoulos , F. Walter , A. Wünsche , R. Abraham , V. K. Agnihotri , R. Albanesi , E. Arce-Mansego , D. Arnot , M. Audejean , C. Aumasson , M. Bachschmidt , G. Baj , P. R. Barroy , A. A. Belinski , D. Bennett , P. Benni , K. Bernacki , L. Betti , A. Biagini , P. Bosch , P. Brandebourg , L. Brát , M. Bretton , S. M. Brincat , S. Brouillard , A. Bruzas , A. Bruzzone , R. A. Buckland , M. Caló , F. Campos , A. Carreno , J. -A. Carrion Rodrigo , R. Casali , G. Casalnuovo , M. Cataneo , C. -M. Chang , L. Changeat , V. Chowdhury , R. Ciantini , M. Cilluffo , J. -F. Coliac , G. Conzo , M. Correa , G. Coulon , N. Crouzet , M. V. Crow , I. Curtis , D. Daniel , S. Dawes , B. Dauchet , M. Deldem , D. Deligeorgopoulos , G. Dransfield , R. Dymock , T. Eenmäe , P. Evans , N. Esseiva , C. Falco , R. G. Farfán , E. Fernández-Lajús , S. Ferratfiat , S. L. Ferreira , A. Ferretti , J. Fiołka , M. Fowler , S. R. Futcher , D. Gabellini , T. Gainey , J. Gaitan , P. Gajdoš , A. García-Sánchez , J. Garlitz , C. Gillier , C. Gison , F. Grau Horta , G. Grivas , J. Gonzales , D. Gorshanov , P. Guerra , T. Guillot , C. A. Haswell , T. Haymes , V. -P. Hentunen , K. Hills , K. Hose , T. Humbert , F. Hurter , T. Hynek , M. Irzyk , J. Jacobsen , A. L. Jannetta , K. Johnson , P. Jóźwik-Wabik , A. E. Kaeouach , W. Kang , H. Kiiskinen , T. Kim , Ü. Kivila , B. Koch , U. Kolb , H. Kučáková , S. -P. Lai , D. Laloum , S. Lasota , L. A. Lewis , G. -I. Liakos , F. Libotte , C. Lopresti , F. Lomoz , R. Majewski , A. Malcher , M. Mallonn , M. Mannucci , A. Marchini , J. -M. Mari , A. Marino , G. Marino , J. -C. Mario , J. -B. Marquette , F. A. Martínez-Bravo , M. Mašek , P. Matassa , P. Michel , J. Michelet , M. Miller , E. Miny , T. Mollier , D. Molina , B. Monteleone , N. Montigiani , M. Morales-Aimar , F. Mortari , M. Morvan , L. V. Mugnai , G. Murawski , L. Naponiello , R. Naves , J. -L. Naudin , D. Néel , R. Neito , S. Neveu , A. Noschese , Y. Öğmen , O. Ohshima , Z. Orbanic , E. P. Pace , C. Pantacchini , N. I. Paschalis , C. Pereira , I. Peretto , V. Perroud , M. Phillips , P. Pintr , J. -B. Pioppa , J. Plazas , A. J. Poelarends , A. Popowicz , J. Purcell , N. Quinn , M. Raetz , D. Rees , F. Regembal , M. Rocchetto , P. -F. Rocci , M. Rockenbauer , R. Roth , L. Rousselot , X. Rubia , N. Ruocco , E. Russo , M. Salisbury , F. Salvaggio , A. Santos , J. Savage , F. Scaggiante , D. Sedita , S. Shadick , A. F. Silva , N. Sioulas , V. Školník , M. Smith , M. Smolka , A. Solmaz , N. Stanbury , D. Stouraitis , T. -G. Tan , M. Theusner , G. Thurston , F. -P. Tifner , A. Tomacelli , A. Tomatis , J. Trnka , M. Tylšar , P. Valeau , J. -P. Vignes , A. Villa , A. Vives Sureda , K. Vora , M. Vrašťák , D. Walliang , B. Wenzel , D. E. Wright , R. Zambelli , M. Zhang , M. Zíbar

"exoplanet" is a toolkit for probabilistic modeling of astronomical time series data, with a focus on observations of exoplanets, using PyMC3 (Salvatier et al., 2016). PyMC3 is a flexible and high-performance model-building language and…

OrbDot is a Python package for studying the secular (long-term) evolution of exoplanet orbits from observational data. It employs nested sampling algorithms to fit evolutionary models to any combination of transit and eclipse mid-times,…

天体物理仪器与方法 · 物理学 2025-09-08 Simone R. Hagey , Aaron Boley

The Exoplanet Imaging Data Challenge is a community-wide effort meant to offer a platform for a fair and common comparison of image processing methods designed for exoplanet direct detection. For this purpose, it gathers on a dedicated…

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