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Related papers: A Gaia early DR3 mock stellar catalog: Galactic pr…

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The Early Gaia Data Release 3 (EDR3) provides precise astrometry for nearly 1.5 billion sources across the entire sky. A few tens of these are associated with neutron stars in the Milky Way and Magellanic Clouds. Here, we report on a search…

High Energy Astrophysical Phenomena · Physics 2020-12-14 John Antoniadis

Context. The observed scarcity of brown dwarfs in close orbits (within 10 au) around solar-type stars poses significant questions about the origins of these substellar companions. These questions impact our broader understanding of…

Earth and Planetary Astrophysics · Physics 2023-12-06 N. Unger , D. Ségransan , D. Barbato , J. -B. Delisle , J. Sahlmann , B. Holl , S. Udry

We independently determine the zero-point offset of the Gaia early Data Release-3 (EDR3) parallaxes based on $\sim 110,000$ W Ursae Majoris (EW)-type eclipsing binary systems. EWs cover almost the entire sky and are characterized by a…

Solar and Stellar Astrophysics · Physics 2021-04-28 Fangzhou Ren , Xiaodian Chen , Huawei Zhang , Richard de Grijs , Licai Deng , Yang Huang

Updated systemic proper motion estimates for 58 Milky Way satellite galaxies, based on Gaia Early Data Release 3 (EDR3), are provided. This sample is identical to that studied by McConnachie & Venn (2020) and the methodology is essentially…

Astrophysics of Galaxies · Physics 2020-12-16 Alan W. McConnachie , Kim A. Venn

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…

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 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 recent Gaia third data release (DR3) has brought some new exciting data about stellar binaries. It provides new opportunities to fully characterize more stellar systems and contribute to enforce our global knowledge of stars behaviour.…

Solar and Stellar Astrophysics · Physics 2023-10-04 S. Chevalier , C. Babusiaux , T. Merle , F. Arenou

In this work, we use the spectroscopy-based stellar color regression (SCR) method with ~ 0.7 million common stars between LAMOST DR7 and Gaia EDR3 to acquire color corrections in G - GRP and GBP - GRP. A sub-mmag precision is achieved. Our…

Solar and Stellar Astrophysics · Physics 2021-02-24 Zexi Niu , Haibo Yuan , Jifeng Liu

We develop, validate and apply a forward model to estimate stellar atmospheric parameters ($T_{\rm eff}$, $\log{g}$ and $\mathrm{[Fe/H]}$), revised distances and extinctions for 220 million stars with XP spectra from $\textit{Gaia}$ DR3.…

Solar and Stellar Astrophysics · Physics 2023-07-05 Xiangyu Zhang , Gregory M. Green , Hans-Walter Rix

The advent of high-precision Gaia parallaxes for Milky Way Cepheids enables per cent-level calibration of the local distance ladder and $H_0$. We revisit the Milky Way Cepheid calibration from Gaia EDR3 parallaxes using a fully…

Astrophysics of Galaxies · Physics 2026-03-11 Richard Stiskalek , Adam Riess , Harry Desmond , Guilhem Lavaux , Dan Scolnic

This work explores dynamical models of the Milky Way (MW) by analyzing a sample of 86,109 K giant stars selected through cross-matching the LAMOST DR8 and Gaia EDR3 surveys. Our earlier torus models in Wang et al. (2017) did not include…

Astrophysics of Galaxies · Physics 2025-05-26 Guang-Chen Sun , Qiao Wang , Shude Mao , Yichao Li , Richard J. Long , Ping-Jie Ding , Yougang Wang , Xin Zhang , Xuelei Chen

We present new three-dimensional (3D) interstellar dust reddening maps of the Galactic plane in three colours, E(G-Ks), E(Bp-Rp) and E(H-Ks). The maps have a spatial angular resolution of 6 arcmin and covers over 7000 deg$^2$ of the…

Astrophysics of Galaxies · Physics 2018-12-19 B. -Q. Chen , Y. Huang , H. -B. Yuan , C. Wang , D. -W. Fan , M. -S. Xiang , H. -W. Zhang , Z. -J. Tian , X. -W. Liu

The astrometric satellite Gaia recently released part of its third data set, which provides a good opportunity to hunt for more open clusters in the Milky Way. In this work, we conduct a blind search for open clusters in the Galactic disk…

Astrophysics of Galaxies · Physics 2022-04-20 C. J. Hao , Y. Xu , Z. Y. Wu , Z. H. Lin , D. J. Liu , Y. J. Li

We report 541 new open cluster candidates in Gaia EDR3 through revisiting the cluster results from an earlier analysis of the Gaia DR2, which revealed nearly a thousand open cluster candidates in the solar neighborhood (mostly d < 3 kpc)…

Astrophysics of Galaxies · Physics 2022-05-18 Zhihong He , Chunyan Li , Jing Zhong , Guimei Liu , Leya Bai , Songmei Qin , Yueyue Jiang , Xi Zhang , Li Chen

We perform a comprehensive determination of the systemic proper motions of 74 dwarf galaxies and dwarf galaxy candidates in the Local Group based on Gaia early data release 3. The outputs of the analysis for each galaxy, including…

Astrophysics of Galaxies · Physics 2022-01-12 G. Battaglia , S. Taibi , G. F. Thomas , T. K. Fritz

Stellar distances constitute a foundational pillar of astrophysics. The publication of 1.47 billion stellar parallaxes from Gaia is a major contribution to this. Yet despite Gaia's precision, the majority of these stars are so distant or…

Solar and Stellar Astrophysics · Physics 2021-02-26 C. A. L. Bailer-Jones , J. Rybizki , M. Fouesneau , M. Demleitner , R. Andrae

We provide an updated test for modifications of gravity from a sample of wide-binary stars from Gaia DR3, and their sky-projected relative velocities. Here we extend on our earlier 2023 study, using several updated selection cuts aimed at…

Astrophysics of Galaxies · Physics 2025-08-04 Charalambos Pittordis , Will Sutherland , Paul Shepherd

Context. The third Gaia Data Release, which includes BP/RP spectra for 219 million sources, has opened a new window in the exploration of the chemical history and evolution of the Milky Way. The wealth of information encapsulated in these…

Solar and Stellar Astrophysics · Physics 2024-03-14 T. Xylakis-Dornbusch , N. Christlieb , T. T. Hansen , T. Nordlander , K. B. Webber , J. Marshall

Gaia data and stellar surveys open the way to the construction of detailed 3D maps of the Galactic interstellar (IS) dust based on the synthesis of star distances and extinctions. Reliable extinction measurements require very accurate…

Astrophysics of Galaxies · Physics 2018-09-05 R. Lallement , L. Capitanio , L. Ruiz-Dern , C. Danielski , C. Babusiaux , J. L. Vergely , M. Elyajouri , F. Arenou , N. Leclerc