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Related papers: Gaia Data Release 2: Catalogue validation

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The Gaia mission has detected a large number of active galactic nuclei (AGN) and galaxies, but these objects must be identified among the 1000-fold more numerous stars. Extant astrometric AGN catalogs do not have the uniform sky coverage…

Astrophysics of Galaxies · Physics 2018-06-13 Jennie Paine , Jeremy Darling , Alexandra Truebenbach

We report on a first census of Galactic black hole X-ray binary (BHXRB) properties with the second data release (DR2) of {\em Gaia}, focusing on dynamically confirmed and strong candidate black hole transients. DR2 provides five-parameter…

High Energy Astrophysical Phenomena · Physics 2019-03-20 Poshak Gandhi , Anjali Rao , Michael A. C. Johnson , John A. Paice , Thomas J. Maccarone

The Gaia Early Data Release 3 (Gaia EDR3) contains results derived from 78 billion individual field-of-view transits of 2.5 billion sources collected by the European Space Agency's Gaia mission during its first 34 months of continuous…

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the full data release, external catalogues, and simulations. We…

Solar and Stellar Astrophysics · Physics 2021-04-28 Gaia Collaboration , R. L. Smart , L. M. Sarro , J. Rybizki , C. Reylé , A. C. Robin , N. C. Hambly , U. Abbas , M. A. Barstow , J. H. J. de Bruijne , B. Bucciarelli , J. M. Carrasco , W. J. Cooper , S. T. Hodgkin , E. Masana , D. Michalik , J. Sahlmann , A. Sozzetti , A. G. A. Brown , A. Vallenari , T. Prusti , C. Babusiaux , M. Biermann , O. L. Creevey , D. W. Evans , L. Eyer , A. Hutton , F. Jansen , C. Jordi , S. A. Klioner , U. Lammers , L. Lindegren , X. Luri , F. Mignard , C. Panem , D. Pourbaix , S. Randich , P. Sartoretti , C. Soubiran , N. A. Walton , F. Arenou , C. A. L. Bailer-Jones , U. Bastian , M. Cropper , R. Drimmel , D. Katz , M. G. Lattanzi , F. van Leeuwen , J. Bakker , J. Castañeda , F. De Angeli , C. Ducourant , C. Fabricius , M. Fouesneau , Y. Frémat , R. Guerra , A. Guerrier , J. Guiraud , A. Jean-Antoine Piccolo , R. Messineo , N. Mowlavi , C. Nicolas , K. Nienartowicz , F. Pailler , P. Panuzzo , F. Riclet , W. Roux , G. M. Seabroke , R. Sordo , P. Tanga , F. Thévenin , G. Gracia-Abril , J. Portell , D. Teyssier , M. Altmann , R. Andrae , I. Bellas-Velidis , K. Benson , J. Berthier , R. Blomme , E. Brugaletta , P. W. Burgess , G. Busso , B. Carry , A. Cellino , N. Cheek , G. Clementini , Y. Damerdji , M. Davidson , L. Delchambre , A. Dell'Oro , J. Fernández-Hernández , L. Galluccio , P. García-Lario , M. Garcia-Reinaldos , J. González-Núñez , E. Gosset , R. Haigron , J. -L. Halbwachs , D. L. Harrison , D. Hatzidimitriou , U. Heiter , J. Hernández , D. Hestroffer , B. Holl , K. Janßen , G. Jevardat de Fombelle , S. Jordan , A. Krone-Martins , A. C. Lanzafame , W. Löffler , A. Lorca , M. Manteiga , O. Marchal , P. M. Marrese , A. Moitinho , A. Mora , K. Muinonen , P. Osborne , E. Pancino , T. Pauwels , A. Recio-Blanco , P. J. Richards , M. Riello , L. Rimoldini , T. Roegiers , C. Siopis , M. Smith , A. Ulla , E. Utrilla , M. van Leeuwen , W. van Reeven , A. Abreu Aramburu , S. Accart , C. Aerts , J. J. Aguado , M. Ajaj , G. Altavilla , M. A. Álvarez , J. Álvarez Cid-Fuentes , J. Alves , R. I. Anderson , E. Anglada Varela , T. Antoja , M. Audard , D. Baines , S. G. Baker , L. Balaguer-Núñez , E. Balbinot , Z. Balog , C. Barache , D. Barbato , M. Barros , S. Bartolomé , J. -L. Bassilana , N. Bauchet , A. Baudesson-Stella , U. Becciani , M. Bellazzini , M. Bernet , S. Bertone , L. Bianchi , S. Blanco-Cuaresma , T. Boch , A. Bombrun , D. Bossini , S. Bouquillon , A. Bragaglia , L. Bramante , E. Breedt , A. Bressan , N. Brouillet , A. Burlacu , D. Busonero , A. G. Butkevich , R. Buzzi , E. Caffau , R. Cancelliere , H. Cánovas , T. Cantat-Gaudin , R. Carballo , T. Carlucci , M. I Carnerero , L. Casamiquela , M. Castellani , A. Castro-Ginard , P. Castro Sampol , L. Chaoul , P. Charlot , L. Chemin , A. Chiavassa , M. -R. L. Cioni , G. Comoretto , T. Cornez , S. Cowell , F. Crifo , M. Crosta , C. Crowley , C. Dafonte , A. Dapergolas , M. David , P. David , P. de Laverny , F. De Luise , R. De March , J. De Ridder , R. de Souza , P. de Teodoro , A. de Torres , E. F. del Peloso , E. del Pozo , A. Delgado , H. E. Delgado , J. -B. Delisle , P. Di Matteo , S. Diakite , C. Diener , E. Distefano , C. Dolding , D. Eappachen , B. Edvardsson , H. Enke , P. Esquej , C. Fabre , M. Fabrizio , S. Faigler , G. Fedorets , P. Fernique , A. Fienga , F. Figueras , C. Fouron , F. Fragkoudi , E. Fraile , F. Franke , M. Gai , D. Garabato , A. Garcia-Gutierrez , M. García-Torres , A. Garofalo , P. Gavras , E. Gerlach , R. Geyer , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , R. Gomel , A. Gomez , I. Gonzalez-Santamaria , J. J. González-Vidal , M. Granvik , R. Gutiérrez-Sánchez , L. P. Guy , M. Hauser , M. Haywood , A. Helmi , S. L. Hidalgo , T. Hilger , N. Hładczuk , D. Hobbs , G. Holland , H. E. Huckle , G. Jasniewicz , P. G. Jonker , J. Juaristi Campillo , F. Julbe , L. Karbevska , P. Kervella , S. Khanna , A. Kochoska , M. Kontizas , G. Kordopatis , A. J. Korn , Z. Kostrzewa-Rutkowska , K. Kruszyńska , S. Lambert , A. F. Lanza , Y. Lasne , J. -F. Le Campion , Y. Le Fustec , Y. Lebreton , T. Lebzelter , S. Leccia , N. Leclerc , I. Lecoeur-Taibi , S. Liao , E. Licata , H. E. P. Lindstrøm , T. A. Lister , E. Livanou , A. Lobel , P. Madrero Pardo , S. Managau , R. G. Mann , J. M. Marchant , M. Marconi , M. M. S. Marcos Santos , S. Marinoni , F. Marocco , D. J. Marshall , L. Martin Polo , J. M. Martín-Fleitas , A. Masip , D. Massari , A. Mastrobuono-Battisti , T. Mazeh , P. J. McMillan , S. Messina , N. R. Millar , A. Mints , D. Molina , R. Molinaro , L. Molnár , P. Montegriffo , R. Mor , R. Morbidelli , T. Morel , D. Morris , A. F. Mulone , D. Munoz , T. Muraveva , C. P. Murphy , I. Musella , L. Noval , C. Ordénovic , G. Orrù , J. Osinde , C. Pagani , I. Pagano , L. Palaversa , P. A. Palicio , A. Panahi , M. Pawlak , X. Peñalosa Esteller , A. Penttilä , A. M. Piersimoni , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , E. Poretti , E. Poujoulet , A. Prša , L. Pulone , E. Racero , S. Ragaini , M. Rainer , C. M. Raiteri , N. Rambaux , P. Ramos , M. Ramos-Lerate , P. Re Fiorentin , S. Regibo , V. Ripepi , A. Riva , G. Rixon , N. Robichon , C. Robin , M. Roelens , L. Rohrbasser , M. Romero-Gómez , N. Rowell , F. Royer , K. A. Rybicki , G. Sadowski , A. Sagristà Sellés , J. Salgado , E. Salguero , N. Samaras , V. Sanchez Gimenez , N. Sanna , R. Santoveña , M. Sarasso , M. Schultheis , E. Sciacca , M. Segol , J. C. Segovia , D. Ségransan , D. Semeux , S. Shahaf , H. I. Siddiqui , A. Siebert , L. Siltala , E. Slezak , E. Solano , F. Solitro , D. Souami , J. Souchay , A. Spagna , F. Spoto , I. A. Steele , H. Steidelmüller , C. A. Stephenson , M. Süveges , L. Szabados , E. Szegedi-Elek , F. Taris , G. Tauran , M. B. Taylor , R. Teixeira , W. Thuillot , N. Tonello , F. Torra , J. Torra , C. Turon , N. Unger , M. Vaillant , E. van Dillen , O. Vanel , A. Vecchiato , Y. Viala , D. Vicente , S. Voutsinas , M. Weiler , T. Wevers , L. Wyrzykowski , A. Yoldas , P. Yvard , H. Zhao , J. Zorec , S. Zucker , C. Zurbach , T. Zwitter

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

The second Gaia data release (DR2) delivers accurate and homogeneous photometry data of the whole sky to an exquisite quality, reaching down to the unprecedented milli-magnitude (mmag) level for the G, GRP, and GBP passbands. However, the…

Solar and Stellar Astrophysics · Physics 2021-03-10 Zexi Niu , Haibo Yuan , Jifeng Liu

We present the flux tables of the spectro-photometric standard stars (SPSS) used to calibrate in flux the Gaia DR2 and (E)DR3 data releases. The latest SPSS grid version contains 112 stars, whose flux tables agree to better than 1% with the…

The GAIA astrometric mission has recently been approved as one of the next two `cornerstones' of ESA's science programme, with a launch date target of not later than mid-2012. GAIA will provide positional and radial velocity measurements…

Gaia Data Release 3 (Gaia DR3) contains the second release of the combined radial velocities. It is based on the spectra collected during the first 34 months of the nominal mission. The longer time baseline and the improvements of the…

We discuss the Gaia Data Release 1 (September 2016) and preliminary work on maximising the benefit for cool white dwarf (WD) science in advance of the full parallax catalogue which will appear around one year later in DR2. The Tycho…

Solar and Stellar Astrophysics · Physics 2017-02-09 Nigel Hambly , Nick Rowell , Marco Lam

ESA Gaia mission is producing the more accurate source catalogue in astronomy up to now. That represents a challenge on the archiving area to make accessible this information to the astronomers in an efficient way. Also, new astronomical…

We discuss the impact that Gaia, a European Space Agency (ESA) cornerstone mission that has been in scientific operations since July 2014, is expected to have on the definition of the cosmic distance ladder and the study of resolved stellar…

Solar and Stellar Astrophysics · Physics 2018-06-08 Gisella Clementini , Alessia Garofalo , Tatiana Muraveva , Vincenzo Ripepi

Gaia is an all sky, high precision astrometric and photometric satellite of the European Space Agency (ESA) due for launch in 2010-2011. Its primary mission is to study the composition, formation and evolution of our Galaxy. Gaia will…

Astrophysics · Physics 2009-11-10 C. A. L. Bailer-Jones

Astrometry from space has unique advantages over ground-based observations: the all-sky coverage, relatively stable, and temperature and gravity invariant operating environment delivers precision, accuracy and sample volume several orders…

Instrumentation and Methods for Astrophysics · Physics 2018-03-28 Gerard Gilmore

Context: Accurate distance measurements are fundamental to the study of Planetary Nebulae (PNe) but have long been elusive. The most accurate and model-independent distance measurements for galactic PNe come from the trigonometric…

Solar and Stellar Astrophysics · Physics 2020-07-01 N. Chornay , N. A. Walton

CONTEXT. The Gaia Collaboration has used Gaia-DR2 sources with six-dimensional (6D) phase space information to derive kinematical maps within 5 kpc of the Sun, which is a reachable range for stars with relative error in distance lower than…

Astrophysics of Galaxies · Physics 2019-01-09 M. Lopez-Corredoira , F. Sylos Labini

One of the novelties of the Gaia-DR3 with respect to the previous data releases is the publication of the multiband light curves of about 1 million AGN. The goal of this work was the creation of a catalogue of variable AGN, whose selection…

The European Gaia astrometry mission is due for launch in 2011. Gaia will rely on the proven principles of ESA's Hipparcos mission to create an all-sky survey of about one billion stars throughout our Galaxy and beyond, by observing all…

Context. Strong gravitationally lensed quasars are among the most interesting and useful observable extragalactic phenomena. Because their study constitutes a unique tool in various fields of astronomy, they are highly sought, not without…

To illustrate the potential of GDR2, we provide a first look at the kinematics of the Milky Way disc, within a radius of several kiloparsecs around the Sun. We benefit for the first time from a sample of 6.4 million F-G-K stars with full 6D…