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The hunt for compact objects is on. Rarely seen massive binaries with a compact object are a crucial phase in the evolution towards compact object mergers. In Gaia data release 3 (DR3), the first Gaia astrometric orbital solutions for…

太阳与恒星天体物理 · 物理学 2022-03-14 S. Janssens , T. Shenar , H. Sana , S. Faigler , N. Langer , P. Marchant , T. Mazeh , C. Schürmann , S. Shahaf

We present the latest results of our ongoing multiplicity study of (Community) TESS Objects of Interest, using astro- and photometric data from the ESA-Gaia mission, to detect stellar companions of these stars and to characterize their…

太阳与恒星天体物理 · 物理学 2021-10-04 M. Mugrauer , K. -U. Michel

Context. We report the exploitation of a sample of epoch astrometry for 157 000 asteroids, the same object in the Gaia Data Release 3, extended over the time coverage planned for the Gaia DR4, which is not expected before the end of 2025.…

地球与行星天体物理 · 物理学 2023-12-13 Gaia Collaboration , P. David , F. Mignard , D. Hestroffer , P. Tanga

Gaia-CRF3 is the celestial reference frame for positions and proper motions in the third release of data from the Gaia mission, Gaia DR3 (and for the early third release, Gaia EDR3, which contains identical astrometric results). The…

天体物理仪器与方法 · 物理学 2022-11-23 Gaia Collaboration , S. A. Klioner , L. Lindegren , F. Mignard , J. Hernández , M. Ramos-Lerate , U. Bastian , M. Biermann , A. Bombrun , A. de Torres , E. Gerlach , R. Geyer , T. Hilger , D. Hobbs , U. L. Lammers , P. J. McMillan , H. Steidelmüller , D. Teyssier , C. M. Raiteri , S. Bartolomé , M. Bernet , J. Castañeda , M. Clotet , M. Davidson , C. Fabricius , N. Garralda Torres , J. J. González-Vidal , J. Portell , N. Rowell , F. Torra , J. Torra , A. G. A. Brown , A. Vallenari , T. Prusti , J. H. J. de Bruijne , F. Arenou , C. Babusiaux , O. L. Creevey , C. Ducourant , D. W. Evans , L. Eyer , R. Guerra , A. Hutton , C. Jordi , X. Luri , C. Panem , D. Pourbaix , S. Randich , P. Sartoretti , C. Soubiran , P. Tanga , N. A. Walton , C. A. L. Bailer-Jones , R. Drimmel , F. Jansen , D. Katz , M. G. Lattanzi , F. van Leeuwen , J. Bakker , C. Cacciari , F. De Angeli , M. Fouesneau , Y. Frémat , L. Galluccio , A. Guerrier , U. Heiter , E. Masana , R. Messineo , N. Mowlavi , C. Nicolas , K. Nienartowicz , F. Pailler , P. Panuzzo , F. Riclet , W. Roux , G. M. Seabroke , R. Sordo , F. Thévenin , G. Gracia-Abril , M. Altmann , R. Andrae , M. Audard , I. Bellas-Velidis , K. Benson , J. Berthier , R. Blomme , P. W. Burgess , D. Busonero , G. Busso , H. Cánovas , B. Carry , A. Cellino , N. Cheek , G. Clementini , Y. Damerdji , P. de Teodoro , M. Nuñez Campos , L. Delchambre , A. Dell'Oro , P. Esquej , J. Fernández-Hernández , E. Fraile , D. Garabato , P. García-Lario , E. Gosset , R. Haigron , J. -L. Halbwachs , N. C. Hambly , D. L. Harrison , D. Hestroffer , S. T. Hodgkin , B. Holl , K. Janßen , G. Jevardat de Fombelle , S. Jordan , A. Krone-Martins , A. C. Lanzafame , W. Löffler , O. Marchal , P. M. Marrese , A. Moitinho , K. Muinonen , P. Osborne , E. Pancino , T. Pauwels , A. Recio-Blanco , C. Reylé , M. Riello , L. Rimoldini , T. Roegiers , J. Rybizki , L. M. Sarro , C. Siopis , M. Smith , A. Sozzetti , E. Utrilla , M. van Leeuwen , U. Abbas , P. Ábrahám , A. Abreu Aramburu , C. Aerts , J. J. Aguado , M. Ajaj , F. Aldea-Montero , G. Altavilla , M. A. Álvarez , J. Alves , R. I. Anderson , E. Anglada Varela , T. Antoja , D. Baines , S. G. Baker , L. Balaguer-Núñez , E. Balbinot , Z. Balog , C. Barache , D. Barbato , M. Barros , M. A. Barstow , J. -L. Bassilana , N. Bauchet , U. Becciani , M. Bellazzini , A. Berihuete , S. Bertone , L. Bianchi , A. Binnenfeld , S. Blanco-Cuaresma , T. Boch , D. Bossini , S. Bouquillon , A. Bragaglia , L. Bramante , E. Breedt , A. Bressan , N. Brouillet , E. Brugaletta , B. Bucciarelli , A. Burlacu , A. G. Butkevich , R. Buzzi , E. Caffau , R. Cancelliere , T. Cantat-Gaudin , R. Carballo , T. Carlucci , M. I. Carnerero , J. M. Carrasco , L. Casamiquela , M. Castellani , A. Castro-Ginard , L. Chaoul , P. Charlot , L. Chemin , V. Chiaramida , A. Chiavassa , N. Chornay , G. Comoretto , G. Contursi , W. J. Cooper , T. Cornez , S. Cowell , F. Crifo , M. Cropper , M. Crosta , C. Crowley , C. Dafonte , A. Dapergolas , P. David , P. de Laverny , F. De Luise , R. De March , J. De Ridder , R. de Souza , E. F. del Peloso , E. del Pozo , M. Delbo , A. Delgado , J. -B. Delisle , C. Demouchy , T. E. Dharmawardena , S. Diakite , C. Diener , E. Distefano , C. Dolding , H. Enke , C. Fabre , M. Fabrizio , S. Faigler , G. Fedorets , P. Fernique , A. Fienga , F. Figueras , Y. Fournier , C. Fouron , F. Fragkoudi , M. Gai , A. Garcia-Gutierrez , M. Garcia-Reinaldos , M. García-Torres , A. Garofalo , A. Gavel , P. Gavras , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , R. Gomel , A. Gomez , J. González-Núñez , I. González-Santamaría , M. Granvik , P. Guillout , J. Guiraud , R. Gutiérrez-Sánchez , L. P. Guy , D. Hatzidimitriou , M. Hauser , M. Haywood , A. Helmer , A. Helmi , M. H. Sarmiento , S. L. Hidalgo , N. Hładczuk , G. Holland , H. E. Huckle , K. Jardine , G. Jasniewicz , A. Jean-Antoine Piccolo , Ó. Jiménez-Arranz , J. Juaristi Campillo , F. Julbe , L. Karbevska , P. Kervella , S. Khanna , G. Kordopatis , A. J. Korn , Á Kóspál , Z. Kostrzewa-Rutkowska , K. Kruszyńska , M. Kun , P. Laizeau , S. Lambert , A. F. Lanza , Y. Lasne , J. -F. Le Campion , Y. Lebreton , T. Lebzelter , S. Leccia , N. Leclerc , I. Lecoeur-Taibi , S. Liao , E. L. Licata , H. E. P. Lindstrøm , T. A. Lister , E. Livanou , A. Lobel , A. Lorca , C. Loup , P. Madrero Pardo , A. Magdaleno Romeo , S. Managau , R. G. Mann , M. Manteiga , J. M. Marchant , M. Marconi , J. Marcos , M. M. S. Marcos Santos , D. Marín Pina , S. Marinoni , F. Marocco , D. J. Marshall , L. Martin Polo , J. M. Martín-Fleitas , G. Marton , N. Mary , A. Masip , D. Massari , A. Mastrobuono-Battisti , T. Mazeh , 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 , T. Muraveva , C. P. Murphy , I. Musella , Z. Nagy , L. Noval , F. Ocaña , A. Ogden , C. Ordenovic , J. O. Osinde , C. Pagani , I. Pagano , L. Palaversa , P. A. Palicio , L. Pallas-Quintela , A. Panahi , S. Payne-Wardenaar , X. Peñalosa Esteller , A. Penttilä , B. Pichon , A. M. Piersimoni , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , A. Prša , L. Pulone , E. Racero , S. Ragaini , M. Rainer , N. Rambaux , P. Ramos , P. Re Fiorentin , S. Regibo , P. J. Richards , C. Rios Diaz , V. Ripepi , A. Riva , H. -W. Rix , G. Rixon , N. Robichon , A. C. Robin , C. Robin , M. Roelens , H. R. O. Rogues , L. Rohrbasser , M. Romero-Gómez , F. Royer , D. Ruz Mieres , K. A. Rybicki , G. Sadowski , A. Sáez Núñez , A. Sagristà Sellés , J. Sahlmann , 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 , A. Silvelo , E. Slezak , I. Slezak , R. L. Smart , O. N. Snaith , E. Solano , F. Solitro , D. Souami , J. Souchay , A. Spagna , L. Spina , F. Spoto , I. A. Steele , C. A. Stephenson , M. Süveges , J. Surdej , L. Szabados , E. Szegedi-Elek , F. Taris , M. B. Taylor , R. Teixeira , L. Tolomei , N. Tonello , G. Torralba Elipe , M. Trabucchi , A. T. Tsounis , C. Turon , A. Ulla , N. Unger , M. V. Vaillant , E. van Dillen , W. van Reeven , O. Vanel , A. Vecchiato , Y. Viala , D. Vicente , S. Voutsinas , M. Weiler , T. Wevers , Ł. Wyrzykowski , A. Yoldas , P. Yvard , H. Zhao , J. Zorec , S. Zucker , T. Zwitter

The early third data release (EDR3) of the European Space Agency satellite Gaia provides coordinates, parallaxes, and proper motions for ~1.47 billion sources in our Milky Way, based on 34 months of observations. The combination of Gaia DR2…

星系天体物理 · 物理学 2021-03-17 Tommaso Marchetti

In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the Gaia mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data…

太阳与恒星天体物理 · 物理学 2022-06-15 Richard Culpan , Stephan Geier , Ingrid Pelisoli , Nicole Reindl , Nicola Gentile Fusillo , Alina Vorontseva

In this work we report the discovery and analysis of three new triply eclipsing triple star systems found with the TESS mission during its observations of the northern skies: TICs 193993801, 388459317, and 52041148. We utilized the TESS…

Context. In 2020, the initial version of the Stellar Potential Perturbers Database (StePPeD) was presented with the aim to deliver up-to-date information on the stars and stellar systems that may perturb a long-period comet motion. We used…

太阳与恒星天体物理 · 物理学 2022-08-24 Piotr A. Dybczyński , Filip Berski , Jakub Tokarek , Edyta Podlewska-Gaca , Krzysztof Langner , Przemysław Bartczak

The latest Gaia data release enables us to accurately identify stars that are more luminous than would be expected on the basis of their spectral type and distance. During an investigation of the 329 best Solar twin candidates uncovered…

We present the latest results of our ongoing multiplicity study of (Community) TESS Objects of Interest, using astrometric and photometric data from the ESA-Gaia mission to detect stellar companions of these stars and characterize their…

太阳与恒星天体物理 · 物理学 2023-06-06 M. Mugrauer , J. Rück , K. -U. Michel

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…

The Gaia Data Release 3 (DR3), published in June 2022, delivers a diverse set of astrometric, photometric, and spectroscopic measurements for more than a billion stars. The wealth and complexity of the data makes traditional approaches for…

星系天体物理 · 物理学 2023-02-15 F. Anders , A. Khalatyan , A. B. A. Queiroz , S. Nepal , C. Chiappini

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…

星系天体物理 · 物理学 2021-12-14 I. González-Santamaría , M. Manteiga , A. Manchado , A. Ulla , C. Dafonte , P. López Varela

The recent Gaia Data Release 3 has unveiled a catalog of over eight hundred thousand binary systems, providing orbital solutions for half of them. Since most of them are unresolved astrometric binaries, several astrophysical parameters that…

太阳与恒星天体物理 · 物理学 2023-07-10 Xabier Pérez-Couto , Jose Á. Docobo , Pedro P. Campo

In the new era of large-scale astronomical surveys, automated methods of analysis and classification of bulk data are a fundamental tool for fast and efficient production of deliverables. This becomes ever more imminent as we enter the Gaia…

天体物理仪器与方法 · 物理学 2017-06-28 A. Kochoska , N. Mowlavi , A. Prsa , I. Lecoeur-Taibi , B. Holl , L. Rimoldini , M. Suveges , L. Eyer

The third data release (DR3) of the European Space Agency satellite Gaia provides coordinates, parallaxes, proper motions, and radial velocities for a sample of $\sim 34$ million stars. We use the combined 6-dimensional phase space…

星系天体物理 · 物理学 2022-07-06 Tommaso Marchetti , Fraser A. Evans , Elena Maria Rossi

We present multi-epoch spectroscopic follow-up of a sample of ellipsoidal variables selected from Gaia DR3 as candidates for hosting quiescent black holes (BHs) and neutron stars (NSs). Our targets were identified as BH/NS candidates…

太阳与恒星天体物理 · 物理学 2023-07-31 Pranav Nagarajan , Kareem El-Badry , Antonio C. Rodriguez , Jan van Roestel , Benjamin Roulston

The first results of a new survey are reported, which explores the 2nd data release of the ESA-Gaia mission, in order to search for stellar companions of (Community) TESS Objects of Interest and to characterize their properties. In total,…

太阳与恒星天体物理 · 物理学 2021-01-13 M. Mugrauer , K. -U. Michel

In this paper we reanalyze the extended ETV curves of the formerly identified triple star candidates and many other $Kepler$ EBs. Besides the confirmations of the former findings and/or the improvements of the triple systems' orbital…

The detection of exoplanets using astrometry has long been an area of interest, but is fraught with challenges. The Gaia mission is fundamentally reshaping this field thanks to its unprecedentedly precise all-sky astrometric observations.…