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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The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite
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TL;DR: The TESS Asteroseismic Target List (ATL) as discussed by the authors is composed of bright, cool main-sequence and subgiant stars and forms part of the larger target list of the TESS AST Consortium, which uses the Gaia Data Release 2 and Extended Hipparcos Compilation (XHIP) to derive fundamental stellar properties, to calculate detection probabilities, and to produce a rank-ordered target list.
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A Spectroscopic Analysis of the California-Kepler Survey Sample: I. Stellar Parameters, Planetary Radii and a Slope in the Radius Gap
TL;DR: In this paper, a quantitative spectroscopic analysis was conducted on archival Keck/HIRES high-resolution spectra from the California-Kepler- Survey (CKS) sample of transiting planetary host stars identified from the $Kepler$ mission.
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TL;DR: In this paper, a high-resolution analysis of a sample of 48 T Tauri stars was performed and the authors found that most of the mass loss occurs close to the central star, within a few au, through an MHD driven wind.
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Reference star differential imaging of close-in companions and circumstellar disks with the NIRC2 vortex coronagraph at W.M. Keck Observatory
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TL;DR: Reference star differential imaging (RDI) is a powerful strategy for high contrast imaging as discussed by the authors, and it has been shown that RDI provides improved sensitivity to point sources at small angular separations compared to ADI.
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Mapping the Magnetic Interstellar Medium in Three Dimensions over the Full Sky with Neutral Hydrogen
TL;DR: In this article, the 3D Stokes parameter maps of neutral hydrogen (HI) emission were constructed using full-sky spectroscopic HI data and compared to Planck maps of the polarized dust emission at 353 GHz.
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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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Gaia Data Release 2: using Gaia parallaxes
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