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200 papers

Gaia mission will offer an exceptional opportunity to perform variability studies. The data homogeneity, its optimised photometric systems, composed of 11 medium and 4-5 broad bands, the high photometric precision in G band of one milli-mag…

Astrophysics · Physics 2007-05-23 Laurent Eyer

Gaia is the next astrometry mission of the European Space Agency (ESA), following up on the success of the Hipparcos mission. With a focal plane containing 106 CCD detectors, Gaia will survey the entire sky and repeatedly observe the…

Instrumentation and Methods for Astrophysics · Physics 2015-06-03 J. H. J. de Bruijne

We present and analyse mock stellar catalogues that match the selection criteria and observables (including uncertainties) of the Gaia satellite data release 2 (DR2). The source are six cosmological high-resolution magneto-hydrodynamic…

Context. This study has been developed in the framework of the computational simulations executed for the preparation of the ESA Gaia astrometric mission. Aims. We focus on describing the objects and characteristics that Gaia will…

Gaia DR2 provides a unique all-sky catalogue of 550'737 variable stars, of which 151'761 are long-period variable (LPV) candidates with G variability amplitudes larger than 0.2 mag (5-95% quantile range). About one-fifth of the LPV…

The second data release of ESA's Gaia satellite (Gaia DR2) revolutionised astronomy by providing accurate distances, proper motions, apparent magnitudes, and in many cases temperatures and radial velocities for an unprecedented number of…

Instrumentation and Methods for Astrophysics · Physics 2018-12-18 Tomaž Zwitter

I provide a summary of the ESA space astrometry mission Gaia regarding its main objectives and current status following the 2nd data release (Gaia DR2) in April 2018. The Gaia achievements in astrometry are assessed with a historical…

Instrumentation and Methods for Astrophysics · Physics 2019-06-24 F. Mignard

Gaia Data Release 2 (Gaia DR2) provides high accuracy and precision astrometric parameters (position, parallax, and proper motion) for more than 1 billion sources and is revolutionizing astrometry. For a fast-moving target such as an…

Instrumentation and Methods for Astrophysics · Physics 2021-08-25 Z. J. Zheng , Q. Y. Peng , F. R. Lin

The second data release from the Gaia mission (Gaia DR2) includes, among its billion entries, as- trometric parameters for binary companions to a number of known pulsars, including white dwarf companions to millisecond pulsars and the…

Solar and Stellar Astrophysics · Physics 2018-08-30 Ross J. Jennings , David L. Kaplan , Shami Chatterjee , James M. Cordes , Adam T. Deller

The Gaia satellite was selected as a cornerstone mission of the European Space Agency (ESA) in October 2000 and confirmed in 2002 with a current target launch date of 2011. The Gaia mission will gather on the same observational principles…

Astrophysics · Physics 2007-05-23 L. Eyer , F. Mignard

Gaia will observe more than one billion objects brighter than V=20, including stars, asteroids, galaxies and quasars. As Gaia performs real time detection (i.e. without an input catalogue) the intrinsic properties of most of these objects…

Astrophysics · Physics 2007-05-23 C. A. L. Bailer-Jones

We highlight the power of the Gaia DR2 in studying many fine structures of the Hertzsprung-Russell diagram (HRD). Gaia allows us to present many different HRDs, depending in particular on stellar population selections. We do not aim here…

Solar and Stellar Astrophysics · Physics 2018-08-15 Gaia Collaboration , C. Babusiaux , F. van Leeuwen , M. A. Barstow , C. Jordi , A. Vallenari , D. Bossini , A. Bressan , T. Cantat-Gaudin , M. van Leeuwen , A. G. A. Brown , T. Prusti , J. H. J. de Bruijne , C. A. L. Bailer-Jones , M. Biermann , D. W. Evans , L. Eyer , F. Jansen , S. A. Klioner , U. Lammers , L. Lindegren , X. Luri , F. Mignard , C. Panem , D. Pourbaix , S. Randich , P. Sartoretti , H. I. Siddiqui , C. Soubiran , N. A. Walton , F. Arenou , U. Bastian , M. Cropper , R. Drimmel , D. Katz , M. G. Lattanzi , J. Bakker , C. Cacciari , J. Castañeda , L. Chaoul , N. Cheek , F. DeAngeli , C. Fabricius , R. Guerra , B. Holl , E. Masana , R. Messineo , N. Mowlavi , K. Nienartowicz , P. Panuzzo , J. Portell , M. Riello , G. M. Seabroke , P. Tanga , F. Thévenin , G. Gracia-Abril , G. Comoretto , M. Garcia-Reinaldos , D. Teyssier , M. Altmann , R. Andrae , M. Audard , I. Bellas-Velidis , K. Benson , J. Berthier , R. Blomme , P. Burgess , G. Busso , B. Carry , A. Cellino , G. Clementini , M. Clotet , O. Creevey , M. Davidson , J. DeRidder , L. Delchambre , A. Dell'Oro , C. Ducourant , J. Fernández-Hernández , M. Fouesneau , Y. Frémat , L. Galluccio , M. García-Torres , J. González-Núñez , J. J. González-Vidal , E. Gosset , L. P. Guy , J. -L. Halbwachs , N. C. Hambly , D. L. Harrison , J. Hernández , D. Hestroffer , S. T. Hodgkin , A. Hutton , G. Jasniewicz , A. Jean-Antoine-Piccolo , S. Jordan , A. J. Korn , A. Krone-Martins , A. C. Lanzafame , T. Lebzelter , W. Löffler , M. Manteiga , P. M. Marrese , J. M. Martín-Fleitas , A. Moitinho , A. Mora , K. Muinonen , J. Osinde , E. Pancino , T. Pauwels , J. -M. Petit , A. Recio-Blanco , P. J. Richards , L. Rimoldini , A. C. Robin , L. M. Sarro , C. Siopis , M. Smith , A. Sozzetti , M. Süveges , J. Torra , W. vanReeven , U. Abbas , A. Abreu Aramburu , S. Accart , C. Aerts , G. Altavilla , M. A. Álvarez , R. Alvarez , J. Alves , R. I. Anderson , A. H. Andrei , E. Anglada Varela , E. Antiche , T. Antoja , B. Arcay , T. L. Astraatmadja , N. Bach , S. G. Baker , L. Balaguer-Núñez , P. Balm , C. Barache , C. Barata , D. Barbato , F. Barblan , P. S. Barklem , D. Barrado , M. Barros , S. Bartholomé Muñoz , J. -L. Bassilana , U. Becciani , M. Bellazzini , A. Berihuete , S. Bertone , L. Bianchi , O. Bienaymé , S. Blanco-Cuaresma , T. Boch , C. Boeche , A. Bombrun , R. Borrachero , S. Bouquillon , G. Bourda , A. Bragaglia , L. Bramante , M. A. Breddels , N. Brouillet , T. Brüsemeister , E. Brugaletta , B. Bucciarelli , A. Burlacu , D. Busonero , A. G. Butkevich , R. Buzzi , E. Caffau , R. Cancelliere , G. Cannizzaro , R. Carballo , T. Carlucci , J. M. Carrasco , L. Casamiquela , M. Castellani , A. Castro-Ginard , P. Charlot , L. Chemin , A. Chiavassa , G. Cocozza , G. Costigan , S. Cowell , F. Crifo , M. Crosta , C. Crowley , J. Cuypers , C. Dafonte , Y. Damerdji , A. Dapergolas , P. David , M. David , P. deLaverny , F. DeLuise , R. DeMarch , D. deMartino , R. deSouza , A. deTorres , J. Debosscher , E. delPozo , M. Delbo , A. Delgado , H. E. Delgado , S. Diakite , C. Diener , E. Distefano , C. Dolding , P. Drazinos , J. Durán , B. Edvardsson , H. Enke , K. Eriksson , P. Esquej , G. Eynard Bontemps , C. Fabre , M. Fabrizio , S. Faigler , A. J. Falcão , M. Farràs Casas , L. Federici , G. Fedorets , P. Fernique , F. Figueras , F. Filippi , K. Findeisen , A. Fonti , E. Fraile , M. Fraser , B. Frézouls , M. Gai , S. Galleti , D. Garabato , F. García-Sedano , A. Garofalo , N. Garralda , A. Gavel , P. Gavras , J. Gerssen , R. Geyer , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , F. Glass , M. Gomes , M. Granvik , A. Gueguen , A. Guerrier , J. Guiraud , R. Gutiérrez-Sánchez , R. Haigron , D. Hatzidimitriou , M. Hauser , M. Haywood , U. Heiter , A. Helmi , J. Heu , T. Hilger , D. Hobbs , W. Hofmann , G. Holland , H. E. Huckle , A. Hypki , V. Icardi , K. Janßen , G. JevardatdeFombelle , P. G. Jonker , Á. L. Juhász , F. Julbe , A. Karampelas , A. Kewley , J. Klar , A. Kochoska , R. Kohley , K. Kolenberg , M. Kontizas , E. Kontizas , S. E. Koposov , G. Kordopatis , Z. Kostrzewa-Rutkowska , P. Koubsky , S. Lambert , A. F. Lanza , Y. Lasne , J. -B. Lavigne , Y. LeFustec , C. LePoncin-Lafitte , Y. Lebreton , S. Leccia , N. Leclerc , I. Lecoeur-Taibi , H. Lenhardt , F. Leroux , S. Liao , E. Licata , H. E. P. Lindstrøm , T. A. Lister , E. Livanou , A. Lobel , M. López , S. Managau , R. G. Mann , G. Mantelet , O. Marchal , J. M. Marchant , M. Marconi , S. Marinoni , G. Marschalkó , D. J. Marshall , M. Martino , G. Marton , N. Mary , D. Massari , G. Matijevič , T. Mazeh , P. J. McMillan , S. Messina , D. Michalik , N. R. Millar , D. Molina , R. Molinaro , L. Molnár , P. Montegriffo , R. Mor , R. Morbidelli , T. Morel , D. Morris , A. F. Mulone , T. Muraveva , I. Musella , G. Nelemans , L. Nicastro , L. Noval , W. O'Mullane , C. Ordénovic , D. Ordóñez-Blanco , P. Osborne , C. Pagani , I. Pagano , F. Pailler , H. Palacin , L. Palaversa , A. Panahi , M. Pawlak , A. M. Piersimoni , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , E. Poujoulet , A. Prša , L. Pulone , E. Racero , S. Ragaini , N. Rambaux , M. Ramos-Lerate , S. Regibo , C. Reylé , F. Riclet , V. Ripepi , A. Riva , A. Rivard , G. Rixon , T. Roegiers , M. Roelens , M. Romero-Gómez , N. Rowell , F. Royer , L. Ruiz-Dern , G. Sadowski , T. Sagristà Sellés , J. Sahlmann , J. Salgado , E. Salguero , N. Sanna , T. Santana-Ros , M. Sarasso , H. Savietto , M. Schultheis , E. Sciacca , M. Segol , J. C. Segovia , D. Ségransan , I-C. Shih , L. Siltala , A. F. Silva , R. L. Smart , K. W. Smith , E. Solano , F. Solitro , R. Sordo , S. SoriaNieto , J. Souchay , A. Spagna , F. Spoto , U. Stampa , I. A. Steele , H. Steidelmüller , C. A. Stephenson , H. Stoev , F. F. Suess , J. Surdej , L. Szabados , E. Szegedi-Elek , D. Tapiador , F. Taris , G. Tauran , M. B. Taylor , R. Teixeira , D. Terrett , P. Teyssandier , W. Thuillot , A. Titarenko , F. TorraClotet , C. Turon , A. Ulla , E. Utrilla , S. Uzzi , M. Vaillant , G. Valentini , V. Valette , A. vanElteren , E. Van Hemelryck , M. Vaschetto , A. Vecchiato , J. Veljanoski , Y. Viala , D. Vicente , S. Vogt , C. vonEssen , H. Voss , V. Votruba , S. Voutsinas , G. Walmsley , M. Weiler , O. Wertz , T. Wevers , Ł. Wyrzykowski , A. Yoldas , M. Žerjal , H. Ziaeepour , J. Zorec , S. Zschocke , S. Zucker , C. Zurbach , T. Zwitter

The ESA Gaia mission provides a unique time-domain survey for more than 1.6 billion sources with G ~ 21 mag. We showcase stellar variability across the Galactic colour-absolute magnitude diagram (CaMD), focusing on pulsating, eruptive, and…

Precise measurement of the fundamental parameters of stellar systems, including mass and radius, depends critically on how well the stellar distances are known. Astrometry from space provides parallax measurements of unprecented accuracy,…

Solar and Stellar Astrophysics · Physics 2021-11-10 Mashhoor Ahmad Al-Wardat , Abdallah M. Hussein , Hamid M. Al-Naimiy , Martin A. Barstow

Hidden within the Gaia satellite's multiple data releases lies a valuable cache of dark companions. To facilitate the efficient and reliable detection of these companions via combined analyses involving Gaia, Hipparcos, and Tycho-2…

Solar and Stellar Astrophysics · Physics 2024-02-08 Fabo Feng , Yicheng Rui , Yifan Xuan , Hugh R. A. Jones

In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of new all-sky data from ground-based photometric surveys and the Gaia mission Data Release 2, we compiled an updated catalogue…

Solar and Stellar Astrophysics · Physics 2020-04-08 S. Geier

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…

Gaia is a satellite mission of the European Space Agency which is creating a catalogue of extremely accurate positions, distances and space motions of two billion stars in our Galaxy, along with more than one hundred thousand solar system…

Instrumentation and Methods for Astrophysics · Physics 2025-09-16 Michael Perryman

Context: Planetary Nebula distance scales often suffer for model dependent solutions. Model independent trigonometric parallaxes have been rare. Space based trigonometric parallaxes are now available for a larger sample using the second…

Solar and Stellar Astrophysics · Physics 2018-08-15 Stefan Kimeswenger , Daniela Barría

Gaia is a space mission currently measuring the five astrometric parameters as well as spectrophotometry of at least 1 billion stars to G = 20.7 mag with unprecedented precision. The sixth parameter in phase space (radial velocity) is also…