English
Related papers

Related papers: Gaia Data Release 2: The Celestial reference frame…

200 papers

Context. In the current ever increasing data volumes of astronomical surveys, automated methods are essential. Objects of known classes from the literature are necessary for training supervised machine learning algorithms, as well as for…

We present a sub-arcsecond cross-match of Gaia DR2 against the INT Photometric H-alpha Survey of the Northern Galactic Plane Data Release 2 (IPHAS DR2) and the Kepler-INT Survey (KIS). The resulting value-added catalogues (VACs) provide…

Solar and Stellar Astrophysics · Physics 2018-09-19 S. Scaringi , C. Knigge , J. E. Drew , M. Monguio , E. Breedt , M. Fratta , B. Gaensicke , T. J. Maccarone , A. F. Pala , C. Schill

The Gaia Data Release 2 (DR2) provided an unprecedented volume of precise astrometric and excellent photometric data. In terms of data mining the Gaia catalogue, machine learning methods have shown to be a powerful tool, for instance in the…

Astrophysics of Galaxies · Physics 2019-07-03 A. Castro-Ginard , C. Jordi , X. Luri , T. Cantat-Gaudin , L. Balaguer-Núñez

This note describes an effort to detect additional stellar sources in known transiting exoplanet (TEP) systems, which are unresolved or barely resolved in the Gaia Data Release 2 (DR2) catalogue. The presence of multiple unresolved stars in…

Earth and Planetary Astrophysics · Physics 2018-05-01 Daniel Evans

Recent work has shown that optical-radio position offsets and radio position variability are inversely correlated with the photometric variability of active galactic nuclei (AGN). A key prediction of these findings is that a reference frame…

Astrophysics of Galaxies · Physics 2026-01-23 Nathan Secrest , Sebastien Lambert

The first data release from the Gaia mission contains accurate positions and magnitudes for more than a billion sources, and proper motions and parallaxes for the majority of the 2.5~million Hipparcos and Tycho-2 stars. We describe three…

Instrumentation and Methods for Astrophysics · Physics 2016-09-15 C. Fabricius , U. Bastian , J. Portell , others

We present and make publicly available the second data release (DR2) of the Keck Observatory Database of Ionized Absorption toward Quasars (KODIAQ) survey. KODIAQ DR2 consists of a fully-reduced sample of 300 quasars at 0.07 < z_em < 5.29…

Context. Strongly lensed quasars are fundamental sources for cosmology. The Gaia space mission covers the entire sky with the unprecedented resolution of $0.18$" in the optical, making it an ideal instrument to search for gravitational…

Astrophysics of Galaxies · Physics 2024-05-22 Gaia Collaboration , A. Krone-Martins , C. Ducourant , L. Galluccio , L. Delchambre , I. Oreshina-Slezak , R. Teixeira , J. Braine , J. -F. Le Campion , F. Mignard , W. Roux , A. Blazere , L. Pegoraro , A. G. A. Brown , A. Vallenari , T. Prusti , J. H. J. de Bruijne , F. Arenou , C. Babusiaux , A. Barbier , M. Biermann , O. L. Creevey , D. W. Evans , L. Eyer , R. Guerra , A. Hutton , C. Jordi , S. A. Klioner , U. Lammers , L. Lindegren , X. Luri , S. Randich , P. Sartoretti , R. Smiljanic , P. Tanga , N. A. Walton , C. A. L. Bailer-Jones , U. Bastian , M. Cropper , R. Drimmel , D. Katz , C. Soubiran , F. van Leeuwen , M. Audard , J. Bakker , R. Blomme , J. Castaneda , F. De Angeli , C. Fabricius , M. Fouesneau , Y. Fremat , A. Guerrier , E. Masana , R. Messineo , C. Nicolas , K. Nienartowicz , F. Pailler , P. Panuzzo , F. Riclet , G. M. Seabroke , R. Sordo , F. Thevenin , G. Gracia-Abril , J. Portell , D. Teyssier , M. Altmann , K. Benson , J. Berthier , P. W. Burgess , D. Busonero , G. Busso , H. Canovas , B. Carry , N. Cheek , G. Clementini , Y. Damerdji , M. Davidson , P. de Teodoro , A. Dell'Oro , E. Fraile Garcia , D. Garabato , P. Garcia-Lario , N. Garralda Torres , P. Gavras , R. Haigron , N. C. Hambly , D. L. Harrison , D. Hatzidimitriou , J. Hernandez , S. T. Hodgkin , B. Holl , S. Jamal , S. Jordan , A. C. Lanzafame , W. Loffler , A. Lorca , O. Marchal , P. M. Marrese , A. Moitinho , K. Muinonen , M. Nunez Campos , P. Osborne , E. Pancino , T. Pauwels , A. Recio-Blanco , M. Riello , L. Rimoldini , A. C. Robin , T. Roegiers , L. M. Sarro , M. Schultheis , C. Siopis , M. Smith , A. Sozzetti , E. Utrilla , M. van Leeuwen , K. Weingrill , U. Abbas , P. Abraham , A. Abreu Aramburu , C. Aerts , G. Altavilla , M. A. Alvarez , J. Alves , R. I. Anderson , T. Antoja , D. Baines , S. G. Baker , Z. Balog , C. Barache , D. Barbato , M. Barros , M. A. Barstow , S. Bartolome , D. Bashi , N. Bauchet , N. Baudeau , U. Becciani , L. R. Bedin , I. Bellas-Velidis , M. Bellazzini , W. Beordo , A. Berihuete , M. Bernet , C. Bertolotto , S. Bertone , L. Bianchi , A. Binnenfeld , T. Boch , A. Bombrun , S. Bouquillon , A. Bragaglia , L. Bramante , E. Breedt , A. Bressan , N. Brouillet , E. Brugaletta , B. Bucciarelli , A. G. Butkevich , R. Buzzi , E. Caffau , R. Cancelliere , S. Cannizzo , R. Carballo , T. Carlucci , M. I. Carnerero , J. M. Carrasco , J. Carretero , S. Carton , L. Casamiquela , M. Castellani , A. Castro-Ginard , V. Cesare , P. Charlot , L. Chemin , V. Chiaramida , A. Chiavassa , N. Chornay , R. Collins , G. Contursi , W. J. Cooper , T. Cornez , M. Crosta , C. Crowley , C. Dafonte , P. de Laverny , F. De Luise , R. De March , R. de Souza , A. de Torres , E. F. del Peloso , M. Delbo , A. Delgado , T. E. Dharmawardena , S. Diakite , C. Diener , E. Distefano , C. Dolding , K. Dsilva , J. Duran , H. Enke , P. Esquej , C. Fabre , M. Fabrizio , S. Faigler , M. Fatovic , G. Fedorets , J. Fernandez-Hernandez , P. Fernique , F. Figueras , Y. Fournier , C. Fouron , M. Gai , M. Galinier , A. Garcia-Gutierrez , M. Garcia-Torres , A. Garofalo , E. Gerlach , R. Geyer , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , R. Gomel , A. Gomez , J. Gonzalez-Nunez , I. Gonzalez-Santamaria , E. Gosset , M. Granvik , V. Gregori Barrera , R. Gutierrez-Sanchez , M. Haywood , A. Helmer , A. Helmi , K. Henares , S. L. Hidalgo , T. Hilger , D. Hobbs , C. Hottier , H. E. Huckle , M. Jablonska , F. Jansen , O. Jimenez-Arranz , J. Juaristi Campillo , S. Khanna , G. Kordopatis , A. Kospal , Z. Kostrzewa-Rutkowska , M. Kun , S. Lambert , A. F. Lanza , Y. Lebreton , T. Lebzelter , S. Leccia , I. Lecoeur-Taibi , G. Lecoutre , S. Liao , L. Liberato , E. Licata , H. E. P. Lindstrom , T. A. Lister , E. Livanou , A. Lobel , C. Loup , L. Mahy , R. G. Mann , M. Manteiga , J. M. Marchant , M. Marconi , D. Marin Pina , S. Marinoni , D. J. Marshall , J. Martin Lozano , J. M. Martin-Fleitas , G. Marton , N. Mary , A. Masip , D. Massari , A. Mastrobuono-Battisti , T. Mazeh , P. J. McMillan , J. Meichsner , S. Messina , D. Michalik , N. R. Millar , A. Mints , D. Molina , R. Molinaro , L. Molnar , G. Monari , M. Monguio , P. Montegriffo , A. Montero , R. Mor , A. Mora , R. Morbidelli , T. Morel , D. Morris , N. Mowlavi , D. Munoz , T. Muraveva , C. P. Murphy , I. Musella , Z. Nagy , S. Nieto , L. Noval , A. Ogden , C. Ordenovic , C. Pagani , I. Pagano , L. Palaversa , P. A. Palicio , L. Pallas-Quintela , A. Panahi , C. Panem , S. Payne-Wardenaar , A. Penttila , P. Pesciullesi , A. M. Piersimoni , M. Pinamonti , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , D. Pourbaix , A. Prsa , L. Pulone , E. Racero , M. Rainer , C. M. Raiteri , P. Ramos , M. Ramos-Lerate , M. Ratajczak , P. Re Fiorentin , S. Regibo , C. Reyle , V. Ripepi , A. Riva , H. -W. Rix , G. Rixon , N. Robichon , C. Robin , M. Romero-Gomez , N. Rowell , F. Royer , D. Ruz Mieres , K. A. Rybicki , G. Sadowski , A. Saez Nunez , A. Sagrista Selles , J. Sahlmann , V. Sanchez Gimenez , N. Sanna , R. Santovena , M. Sarasso , C. Sarrate Riera , E. Sciacca , J. C. Segovia , D. Segransan , S. Shahaf , A. Siebert , L. Siltala , E. Slezak , R. L. Smart , O. N. Snaith , E. Solano , F. Solitro , D. Souami , J. Souchay , L. Spina , E. Spitoni , F. Spoto , L. A. Squillante , I. A. Steele , H. Steidelmuller , J. Surdej , L. Szabados , F. Taris , M. B. Taylor , K. Tisanic , L. Tolomei , F. Torra , G. Torralba Elipe , M. Trabucchi , M. Tsantaki , A. Ulla , N. Unger , O. Vanel , A. Vecchiato , D. Vicente , S. Voutsinas , M. Weiler , L. Wyrzykowski , H. Zhao , J. Zorec , T. Zwitter , L. Balaguer-Nunez , N. Leclerc , S. Morgenthaler , G. Robert , S. Zucker

$Context$. Gaia Second Data Release provides precise astrometry and photometry for more than 1.3 billion sources. This catalog opens a new era concerning the characterization of open clusters and test stellar models, paving the way for a…

The Gaia satellite will survey the entire celestial sphere down to 20th magnitude, obtaining astrometry, photometry, and low resolution spectrophotometry on one billion astronomical sources, plus radial velocities for over one hundred…

Context. Gaia Early Data Release 3 (EDR3), published in December 2020, features improved photometry and astrometry over that published in the previous DR2 file, and includes a substantially larger number of sources, of the order of 2,000…

Astrophysics of Galaxies · Physics 2021-12-14 I. González-Santamaría , M. Manteiga , A. Manchado , A. Ulla , C. Dafonte , P. López Varela

The third data release by the Gaia mission of the European Space (DR3) is the first release to provide the community with a large sample of observations for more than 150 thousand Solar System objects, including asteroids and natural…

The Gaia second data release contains high-accuracy astrometric measurements of thousands of solar system bodies. These measurements raise the possibility of determining asteroid masses by modeling scattering events between massive objects…

Earth and Planetary Astrophysics · Physics 2023-12-20 Zachary Murray

The Hipparcos catalog provides the first epoch of the celestial reference frame (CRF) in the optical domain and serves as an indispensable tool to verify and improve the Gaia CRF for the brighter stars ($V<11$ mag) and to identify the…

Solar and Stellar Astrophysics · Physics 2022-10-05 Valeri V. Makarov

We present an overview of the sample of northern hemisphere white dwarfs within 40 pc of the Sun detected from $Gaia$ Data Release 2 (DR2). We find that 521 sources are spectroscopically confirmed degenerate stars, 111 of which were first…

The Gaia Early Data Release 3 (EDR3) provides trigonometric parallaxes for 1.5 billion stars, with reduced systematics compared to Gaia Data Release 2 and reported precisions better by up to a factor of two. New to EDR3 is a tentative model…

Astrophysics of Galaxies · Physics 2021-04-28 Joel C. Zinn

Open clusters are convenient probes of the structure and history of the Galactic disk. They are also fundamental to stellar evolution studies. The second Gaia data release contains precise astrometry at the sub-milliarcsecond level and…

We investigate a sample of 2293 ICRF2 extragalactic radio-loud sources with accurate positions determined by VLBI, mostly active galactic nuclei (AGN) and quasars, which are cross-matched with optical sources in the first Gaia release (Gaia…

The Gaia third Data Release (DR3) presents a catalogue of 474\,026 stars with variability induced by magnetic activity. For each star, the catalogue provides a list of about 70 parameters among which the most important are the stellar…

The Gaia space mission is crafting revolutionary astrometric, photometric and spectroscopic catalogues that will allow us to map our Galaxy, but only if we know the completeness of this Gaia-verse of catalogues: what stars does it contain…

Instrumentation and Methods for Astrophysics · Physics 2020-07-29 Douglas Boubert , Andrew Everall , Berry Holl
‹ Prev 1 4 5 6 7 8 10 Next ›