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
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Census of R Coronae Borealis Stars. I. Infrared Light Curves from Palomar Gattini IR
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TL;DR: The first systematic IR census of R Coronae Borealis (RCB) stars in the Milky Way was conducted by Tisserand et al. as discussed by the authors, who used IR light curves from the Palomar Gattini IR (PGIR) survey.
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Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy
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TL;DR: In this paper, a large systematic study combining the direct asteroseismic analysis with the spectroscopy on the lithium-rich stars is presented, which reveals that the distribution of lithium rich low-mass evolved stars steeply decline with the increasing lithium abundance, showing an upper limit around 2.6 dex.
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A Gaia Survey for Young Stars Associated with the Lupus Clouds
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Most EL CVn systems are inner binaries of hierarchical triples
F. Lagos,F. Lagos,Matthias R. Schreiber,Matthias R. Schreiber,Steven G. Parsons,Boris T. Gänsicke,N. Godoy +6 more
TL;DR: In this article, it was shown that EL CVn systems are inner binaries of hierarchical triples and indeed descend from very close main sequence binaries that experience stable mass transfer, and they were found to be the progenitor systems of the A/F main sequence star companions.
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Gaia Early Data Release 3: Summary of the contents and survey properties
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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
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Estimating Distances from Parallaxes
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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
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