Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2
TLDR
In this paper, the authors used a weak distance prior that varies smoothly as a function of Galactic longitude and latitude according to a Galaxy model to infer distances to essentially all 1.33 billion stars with parallaxes published in the second Gaia data release.Abstract:
For the vast majority of stars in the second Gaia data release, reliable distances cannot be obtained by inverting the parallax. A correct inference procedure must instead be used to account for the nonlinearity of the transformation and the asymmetry of the resulting probability distribution. Here we infer distances to essentially all 1.33 billion stars with parallaxes published in the second \gaia\ data release. This is done using a weak distance prior that varies smoothly as a function of Galactic longitude and latitude according to a Galaxy model. The irreducible uncertainty in the distance estimate is characterized by the lower and upper bounds of an asymmetric confidence interval. Although more precise distances can be estimated for a subset of the stars using additional data (such as photometry), our goal is to provide purely geometric distance estimates, independent of assumptions about the physical properties of, or interstellar extinction towards, individual stars. We analyse the characteristics of the catalogue and validate it using clusters. The catalogue can be queried on the Gaia archive using ADQL at this http URL and downloaded from this http URL .read more
Citations
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The Atari Disk, a Metal-poor Stellar Population in the Disk System of the Milky Way
TL;DR: In this paper , a chemodynamical approach was developed to assign 36,010 metal-poor SkyMapper stars to various Galactic stellar populations by using two independent techniques (velocity and action space behavior), Gaia EDR3 astrometry, and photometric metallicities.
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Exploring the pertubed Milky Way disk and the substructures of the outer disk
Y. Xu,Chao Liu,Hai-Jun Tian,H. J. Newberg,C. F. P. Laporte,Bo Zhang,H. F. Wang,Jing Li,Licai Deng +8 more
TL;DR: In this article, the authors show that the spiral feature exits not only in the solar vicinity but also extends to about 15 kpc from the Galactic center, and then disappears beyond this radius.
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Revisiting Kepler-444. I. Seismic modeling and inversions of stellar structure
Gaël Buldgen,M. Farnir,C. Pezzotti,Patrick Eggenberger,Sébastien Salmon,Josefina Montalbán,Jason W. Ferguson,Saniya Khan,Vincent Bourrier,B. M. Rendle,Georges Meynet,Andrea Miglio,Arlette Noels +12 more
TL;DR: In this paper, the authors used local and global minimization techniques to study the internal structure of the exoplanet-host star Kepler-444 and provided a detailed characterization of the star's internal structure and evolution.
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Evidence of Hubble Flow-like Motion of Young Stellar Populations away from the Perseus Arm
Carlos Román-Zúñiga,Alexandre Roman-Lopes,Mauricio Tapia,Jesús Hernández,Valeria Ramírez-Preciado +4 more
TL;DR: In this paper, the authors presented evidence of coherent outward motion of a sample of young stars in the Perseus Arm, whose apparent origin is located in the vicinity of the W3/W4/W5 complex.
Journal ArticleDOI
The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?
József Varga,József Varga,Michiel R. Hogerheijde,Michiel R. Hogerheijde,R. van Boekel,L. Klarmann,Romain Petrov,L. B. F. M. Waters,L. B. F. M. Waters,Stephane Lagarde,Eric Pantin,Ph. Berio,Gerd Weigelt,Sylvie Robbe-Dubois,Bruno Lopez,Florentin Millour,Jean-Charles Augereau,H. Méheut,Anthony Meilland,Th. Henning,Walter Jaffe,Felix Bettonvil,Paul Bristow,Karl Heinz Hofmann,Alexis Matter,G. Zins,Sebastian Wolf,F. Allouche,F. Donnan,D. Schertl,Carsten Dominik,M. Heininger,M. Lehmitz,Pierre Cruzalèbes,Andreas Glindemann,Klaus Meisenheimer,Claudia Paladini,Markus Schöller,Julien Woillez,Lars Venema,E. Kokoulina,G. Yoffe,Péter Ábrahám,Péter Ábrahám,S. Abadie,Roberto Abuter,M. Accardo,T. Adler,Tibor Agócs,P. Antonelli,A. Böhm,C. Bailet,G. Bazin,Udo Beckmann,J. Beltran,W. Boland,P. Bourget,R. Brast,Yves Bresson,Leonard Burtscher,R. Castillo,A. Chelli,Claudia Cid,Jean-Michel Clausse,C. Connot,Ralf Conzelmann,William C. Danchi,William C. Danchi,M. de Haan,Marco Delbo,M. Ebert,Eddy Elswijk,Y. Fantei,R. Frahm,V. Gámez Rosas,A. Gabasch,Alexandre Gallenne,Alexandre Gallenne,Alexandre Gallenne,E. Garces,P. Girard,F. Y. J. Gonté,J. C. González Herrera,Uwe Graser,P. Guajardo,F. Guitton,Xavier Haubois,Josef Hron,Norbert Hubin,R. Huerta,J. W. Isbell,Derek Ives,Gerd Jakob,A. Jaskó,A. Jaskó,L. Jochum,Ralf Klein,J. Kragt,G. Kroes,S. Kuindersma,L. Labadie,W. Laun,R. S. Le Poole,Christoph Leinert,J.-L. Lizon,Marcelo Lopez,Antoine Mérand,A. Marcotto,N. Mauclert,T. Maurer,Leander Mehrgan,J. Meisner,K. Meixner,M. Mellein,L. Mohr,S. Morel,L. Mosoni,Ramón Navarro,Udo Neumann,E. Nußbaum,Laurent Pallanca,Luca Pasquini,I. Percheron,J.-U. Pott,Eszter Pozna,A. Ridinger,F. Rigal,M. Riquelme,Th. Rivinius,Ronald Roelfsema,Ralf-Rainer Rohloff,S. Rousseau,Nicolas Schuhler,M. Schuil,A. Soulain,Ph. Stee,C. Stephan,R. ter Horst,N. Tromp,Farrokh Vakili,A. van Duin,J. Vinther,Markus Wittkowski,F. Wrhel +143 more
TL;DR: In this paper, the authors used simple geometric models to fit the interferometric visibilities and closure phases of the inner disk of HD 163296 to detect potential disk asymmetries and found that the brightness maximum of the asymmetry is located at the NW part of the disk image, nearly at the position angle of the semimajor axis.
References
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Panahi,Michał Pawlak,A. M. Piersimoni,F. X. Pineau,Emese Plachy,G. Plum,E. Poggio,E. Poujoulet,Andrej Prsa,L. Pulone,E. Racero,S. Ragaini,Nicolas Rambaux,M. Ramos-Lerate,S. Regibo,Céline Reylé,F. Riclet,V. Ripepi,Alberto Riva,A. Rivard,Guy Rixon,T. Roegiers,Maroussia Roelens,M. Romero-Gómez,Nicholas Rowell,Frédéric Royer,L. Ruiz-Dern,G. Sadowski,T. Sagristà Sellés,Johannes Sahlmann,Jesus Salgado,E. Salguero,Nicoletta Sanna,Toni Santana-Ros,M. Sarasso,H. Savietto,M. Schultheis,Eva Sciacca,M. Segol,J. C. Segovia,Damien Ségransan,I-C. Shih,L. Siltala,A. F. Silva,Richard L. Smart,K. W. Smith,E. Solano,F. Solitro,Rosanna Sordo,S. SoriaNieto,J. Souchay,A. Spagna,Federica Spoto,U. Stampa,Iain A. Steele,H. Steidelmüller,C.A. Stephenson,H. Stoev,F. F. Suess,Jean Surdej,László Szabados,E. Szegedi-Elek,D. Tapiador,Francois Taris,G. Tauran,Mark Taylor,Ramachrisna Teixeira,David Terrett,P. Teyssandier,William Thuillot,A. Titarenko,F. TorraClotet,C. Turon,Ana Ulla,E. Utrilla,S. Uzzi,M. 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TL;DR: In this article, the power of the Gaia DR2 in studying many fine structures of the Hertzsprung-Russell diagram (HRD) was highlighted, depending in particular on stellar population selections.
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Gaia Early Data Release 3: Summary of the contents and survey properties
Anthony G. A. Brown,Antonella Vallenari,T. Prusti,J. H. J. de Bruijne,C. Babusiaux,C. A. L. Bailer-Jones +5 more
TL;DR: Gaia DR2 as mentioned in this paper is the second Gaia data release, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability, for sources brighter than magnitude 21.
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Gaia Data Release 2: Catalogue validation
Frédéric Arenou,Xavier Luri,Carine Babusiaux,Claus Fabricius,Amina Helmi,Tatiana Muraveva,Annie C. Robin,Federica Spoto,Antonella Vallenari,Teresa Antoja,Tristan Cantat-Gaudin,Carme Jordi,N. Leclerc,Céline Reylé,M. Romero-Gómez,I-C. Shih,S. Soria,Christophe Barache,Diego Bossini,A. Bragaglia,Maarten A. Breddels,M. Fabrizio,Sébastien Lambert,P. M. Marrese,Davide Massari,André Moitinho,N. Robichon,L. Ruiz-Dern,Rosanna Sordo,Jovan Veljanoski,P. Di Matteo,L. Eyer,G. Jasniewicz,E. Pancino,Caroline Soubiran,A. Spagna,Paolo Tanga,C. Turon,C. Zurbach +38 more
TL;DR: 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 half a million of stellar sources and orbits for thousands of solar system objects as discussed by the authors.
Journal ArticleDOI
Estimating Distances from Parallaxes
TL;DR: In this paper, the authors investigate the properties and performance of various prior assumptions and examine their implications, and demonstrate that a simple prior which decreases asymptotically to zero at infinite distance has good performance, accommodates nonpositive parallaxes, and does not require a bias correction.
Journal ArticleDOI
Gaia Data Release 2: using Gaia parallaxes
Xavier Luri,Anthony G. A. Brown,L. M. Sarro,Frédéric Arenou,Coryn A. L. Bailer-Jones,Alfred Castro-Ginard,J. H. J. de Bruijne,T. Prusti,C. Babusiaux,C. Babusiaux,H. E. Delgado +10 more
TL;DR: The main recommendation is to always treat the derivation of (astro-)physical parameters from astrometric data, in particular when parallaxes are involved, as an inference problem which should preferably be handled with a full Bayesian approach.
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