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Estimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2
Open accessAbstract
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 toward, individual stars. We analyze the characteristics of the catalog and validate it using clusters. The catalog can be queried using ADQL at http://gaia.ari.uni-heidelberg.de/tap.html (which also hosts the Gaia catalog) and downloaded from http://www.mpia.de/~calj/gdr2_distances.html .
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“1SWASP J140747.93-394542.6 (hereafter J1407) is a premain-sequence, 16 Myr old, 0 : 9 M , V = 12 : 3 mag K5 star with parallax 7 : 1835 0 : 0447 mas (Gaia Collaboration et al. 2018), consistent with d = 138 : 7 0 : 6 pc (Bailer-Jones et al. 2018) and membership of the Sco-Cen OB association (Mamajek et al. 2012).”
From ALMA and NACO observations towards the young exoring transit system J1407 (V1400 Cen) (2020) · cites this paper as Bailer-Jones et al. 2018
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Metadata
- Authors
- Bailer-Jones, C. A. L., Rybizki, J., Fouesneau, M., Mantelet, G., & Andrae, R.
- Affiliations
- Max Planck Institute for Astronomy (DE)
- Heidelberg University (DE)
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2018-07-20
- Volume
- 156
- Issue
- 2
- Pages
- 58
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2798430172
- Cited by
- 1,829
- References
- 11
- Citations by year
- 2026: 42 · 2025: 61 · 2024: 81 · 2023: 110 · 2022: 181 · 2021: 322 · 2020: 506 · 2019: 411 · 2018: 114
- FWCI
- 177.86
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- The Astronomical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- MPG.PuRe (Max Planck Society) (submittedVersion)
- arXiv (Cornell University)
- Funders
- European Space Agency
- Max-Planck-Institut für Astronomie
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astronomical Observations and Instrumentation
- Keywords
- stellar distances, parallax, Gaia DR2, galactic models, star clusters
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