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More than half a million of the 1.69 billion sources in Gaia Data Release 2 (DR2) are published with photometric time series that exhibit light variations during the 22 months of observation. An all-sky classification of common…

The second data release of the Gaia mission includes an advance catalog of variable stars. The classification of these stars are based on sparse photometry from the first 22 months of the mission. We set out to investigate the purity and…

Solar and Stellar Astrophysics · Physics 2018-12-12 László Molnár , Emese Plachy , Áron L. Juhász , Lorenzo Rimoldini

The Gaia second Data Release (DR2) presents a first mapping of full-sky RR Lyrae stars and Cepheids observed by the spacecraft during the initial 22 months of science operations. The Specific Object Study (SOS) pipeline, developed to…

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 Gaia DR2 sample of short-timescale variable candidates results from the investigation of the first 22 months of Gaia photometry for a subsample of sources at the Gaia faint end. For this exercise, we limited ourselves to the case of…

We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability, for sources brighter than magnitude 21. In addition epoch astrometry…

We present a comparison of the Gaia DR1 samples of pulsating variable stars - Cepheids and RR Lyrae type - with the OGLE Collection of Variable Stars aiming at the characterization of the Gaia mission performance in the stellar variability…

The third Gaia Data Release, covering 34 months of data, includes the second Gaia catalogue of long-period variables (LPVs), with G variability amplitudes larger than 0.1 mag (5-95% quantile range). The paper describes the production and…

The second data release (DR2) of Gaia provides mean photometry in three bands for $\sim$1.4 billion sources, but light curves and variability properties are available for only $\sim$0.5 million of them. Here, we provide a census of…

We present the methods devised to identify the BY Dra variables candidates in Gaia DR2 and infer their variability parameters. BY Dra candidates are pre-selected from their position in the HR diagram, built from Gaia parallaxes, $G$…

The second Gaia data release (DR2), contains very precise astrometric and photometric properties for more than one billion sources, astrophysical parameters for dozens of millions, radial velocities for millions, variability information for…

Gaia is undertaking a deep synoptic survey of the Galaxy, but photometry from individual epochs has, as of yet, only been released for a minimal number of sources. We show that it is possible to identify variable stars in Gaia Data Release…

Instrumentation and Methods for Astrophysics · Physics 2021-03-03 Shion Andrew , Samuel J. Swihart , Jay Strader

The Gaia Data Release 2 contains the 1st release of radial velocities complementing the kinematic data of a sample of about 7 million relatively bright, late-type stars. Aims: This paper provides a detailed description of the Gaia…

At the core of the Gaia mission is a multi-epoch survey consisting of astrometric, photometric, spectrophotometric, and spectroscopic measurements. The astrometric time series provides parallaxes and proper motions, along with information…

Instrumentation and Methods for Astrophysics · Physics 2024-12-05 Laurent Eyer

Context. Cepheids are pulsating stars that play a crucial role in several astrophysical contexts. Among the different types, the Classical Cepheids are fundamental tools for the calibration of the extragalactic distance ladder. They are…

Gaia Data Release 2 (Gaia DR2) contains results for 1693 million sources in the magnitude range 3 to 21 based on observations collected by the European Space Agency Gaia satellite during the first 22 months of its operational phase. We…

The third Gaia Data Release (DR3) provided photometric time series of more than 2 million long-period variable (LPV) candidates. Anticipating the publication of full radial-velocity (RV) in DR4, this Focused Product Release (FPR) provides…

Solar and Stellar Astrophysics · Physics 2023-10-11 Gaia Collaboration , Gaia Collaboration , M. Trabucchi , N. Mowlavi , T. Lebzelter , I. Lecoeur-Taibi , M. Audard , L. Eyer , P. García-Lario , P. Gavras , B. Holl , G. Jevardat de Fombelle , K. Nienartowicz , L. Rimoldini , P. Sartoretti , R. Blomme , Y. Frémat , O. Marchal , Y. Damerdji , A. G. A. Brown , A. Guerrier , P. Panuzzo , D. Katz , G. M. Seabroke , K. Benson , R. Haigron , M. Smith , A. Lobel , A. Vallenari , T. Prusti , J. H. J. de Bruijne , F. Arenou , C. Babusiaux , A. Barbier , M. Biermann , O. L. Creevey , C. Ducourant , D. W. Evans , R. Guerra , A. Hutton , C. Jordi , S. A. Klioner , U. Lammers , L. Lindegren , X. Luri , F. Mignard , S. Randich , R. Smiljanic , P. Tanga , N. A. Walton , C. A. L. Bailer-Jones , U. Bastian , M. Cropper , R. Drimmel , M. G. Lattanzi , C. Soubiran , F. van Leeuwen , J. Bakker , J. Castañeda , F. De Angeli , C. Fabricius , M. Fouesneau , L. Galluccio , E. Masana , R. Messineo , C. Nicolas , F. Pailler , F. Riclet , W. Roux , R. Sordo , F. Thévenin , G. Gracia-Abril , J. Portell , D. Teyssier , M. Altmann , J. Berthier , P. W. Burgess , D. Busonero , G. Busso , H. Cánovas , B. Carry , N. Cheek , G. Clementini , M. Davidson , P. de Teodoro , L. Delchambre , A. Dell'Oro , E. Fraile Garcia , D. Garabato , N. Garralda Torres , N. C. Hambly , D. L. Harrison , D. Hatzidimitriou , J. Hernández , S. T. Hodgkin , S. Jamal , S. Jordan , A. Krone-Martins , A. C. Lanzafame , W. Löffler , A. Lorca , P. M. Marrese , A. Moitinho , K. Muinonen , M. Nuñez Campos , I. Oreshina-Slezak , P. Osborne , E. Pancino , T. Pauwels , A. Recio-Blanco , M. Riello , A. C. Robin , T. Roegiers , L. M. Sarro , M. Schultheis , C. Siopis , A. Sozzetti , E. Utrilla , M. van Leeuwen , K. Weingrill , U. Abbas , P. Ábrahám , A. Abreu Aramburu , C. Aerts , G. Altavilla , M. A. Álvarez , J. Alves , F. Anders , R. I. Anderson , T. Antoja , D. Baines , S. G. Baker , Z. Balog , C. Barache , D. Barbato , M. Barros , M. A. Barstow , S. Bartolomé , 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 , A. Blazere , T. Boch , A. Bombrun , S. Bouquillon , A. Bragaglia , J. Braine , 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 , M. David , P. de Laverny , F. De Luise , R. De March , J. De Ridder , 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. Durán , H. Enke , P. Esquej , C. Fabre , M. Fabrizio , S. Faigler , M. Fatović , G. Fedorets , J. Fernández-Hernández , P. Fernique , F. Figueras , Y. Fournier , C. Fouron , M. Gai , M. Galinier , A. Garcia-Gutierrez , M. García-Torres , A. Garofalo , E. Gerlach , R. Geyer , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , R. Gomel , A. Gomez , J. González-Núñez , I. González-Santamaría , E. Gosset , M. Granvik , V. Gregori Barrera , R. Gutiérrez-Sánchez , M. Haywood , A. Helmer , A. Helmi , K. Henares , S. L. Hidalgo , T. Hilger , D. Hobbs , C. Hottier , H. E. Huckle , M. Jabłońska , F. Jansen , Ó. Jiménez-Arranz , J. Juaristi Campillo , S. Khanna , G. Kordopatis , Á Kóspál , Z. Kostrzewa-Rutkowska , M. Kun , S. Lambert , A. F. Lanza , J. -F. Le Campion , Y. Lebreton , S. Leccia , G. Lecoutre , S. Liao , L. Liberato , E. Licata , H. E. P. Lindstrøm , T. A. Lister , E. Livanou , C. Loup , L. Mahy , R. G. Mann , M. Manteiga , J. M. Marchant , M. Marconi , D. Marín Pina , S. Marinoni , D. J. Marshall , J. Martín Lozano , J. M. Martín-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. Molnár , G. Monari , M. Monguió , P. Montegriffo , A. Montero , R. Mor , A. Mora , R. Morbidelli , T. Morel , D. Morris , 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 , L. Pegoraro , A. Penttilä , P. Pesciullesi , A. M. Piersimoni , M. Pinamonti , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , D. Pourbaix , A. Prša , L. Pulone , E. Racero , M. Rainer , C. M. Raiteri , P. Ramos , M. Ramos-Lerate , M. Ratajczak , P. Re Fiorentin , S. Regibo , C. Reylé , V. Ripepi , A. Riva , H. -W. Rix , G. Rixon , N. Robichon , C. Robin , M. Romero-Gómez , N. Rowell , F. Royer , D. Ruz Mieres , K. A. Rybicki , G. Sadowski , A. Sáez Núñez , A. Sagristà Sellés , J. Sahlmann , V. Sanchez Gimenez , N. Sanna , R. Santoveña , M. Sarasso , C. Sarrate Riera , E. Sciacca , J. C. Segovia , D. Ségransan , 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. Steidelmüller , J. Surdej , L. Szabados , F. Taris , M. B. Taylor , R. Teixeira , K. Tisanić , L. Tolomei , F. Torra , G. Torralba Elipe , M. Tsantaki , A. Ulla , N. Unger , O. Vanel , A. Vecchiato , D. Vicente , S. Voutsinas , M. Weiler , Ł. Wyrzykowski , H. Zhao , J. Zorec , T. Zwitter , L. Balaguer-Núñez , N. Leclerc , S. Morgenthaler , G. Robert , S. Zucker
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