Gaia astrometry for stars with too few observations. A Bayesian approach
Michalik, Daniel LU ; Lindegren, Lennart LU
; Hobbs, David
LU
and Butkevich, Alexey G.
(2015)
In Astronomy & Astrophysics
583.
- Abstract
- Context. The astrometric solution for Gaia aims to determine at least five parameters for each star, representing its position, parallax, and proper motion, together with appropriate estimates of their uncertainties and correlations. This requires at least five distinct observations per star. In the early data reductions the number of observations may be insufficient for a five-parameter solution, and even after the full mission many stars will remain under-observed, including faint stars at the detection limit and transient objects. In such cases it is reasonable to determine only the two position parameters. The formal uncertainties of such a two-parameter solution would however grossly underestimate the actual errors in position, due to... (More)
- Context. The astrometric solution for Gaia aims to determine at least five parameters for each star, representing its position, parallax, and proper motion, together with appropriate estimates of their uncertainties and correlations. This requires at least five distinct observations per star. In the early data reductions the number of observations may be insufficient for a five-parameter solution, and even after the full mission many stars will remain under-observed, including faint stars at the detection limit and transient objects. In such cases it is reasonable to determine only the two position parameters. The formal uncertainties of such a two-parameter solution would however grossly underestimate the actual errors in position, due to the neglected parallax and proper motion. Aims. We aim to develop a recipe to calculate sensible formal uncertainties that can be used in all cases of under-observed stars. Methods. Prior information about the typical ranges of stellar parallaxes and proper motions is incorporated in the astrometric solution by means of Bayes' rule. Numerical simulations based on the Gaia Universe Model Snapshot (GUMS) are used to investigate how the prior influences the actual errors and formal uncertainties when different amounts of Gaia observations are available. We develop a criterion for the optimum choice of priors, apply it to a wide range of cases, and derive a global approximation of the optimum prior as a function of magnitude and galactic coordinates. Results. The feasibility of the Bayesian approach is demonstrated through global astrometric solutions of simulated Gaia observations. With an appropriate prior it is possible to derive sensible positions with realistic error estimates for any number of available observations. Even though this recipe works also for well-observed stars it should not be used where a good five-parameter astrometric solution can be obtained without a prior. Parallaxes and proper motions from a solution using priors are always biased and should not be used. (Less)
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/8539618
- author
- Michalik, Daniel
LU
; Lindegren, Lennart
LU
; Hobbs, David
LU
and Butkevich, Alexey G.
- organization
- publishing date
- 2015
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- astrometry, methods: data analysis, methods: numerical, parallaxes, proper motions, space vehicles: instruments
- in
- Astronomy & Astrophysics
- volume
- 583
- article number
- A68
- publisher
- EDP Sciences
- external identifiers
-
- wos:000365072200132
- scopus:84946555278
- ISSN
- 0004-6361
- DOI
- 10.1051/0004-6361/201526936
- language
- English
- LU publication?
- yes
- id
- 012c0496-a92e-4dac-9a36-6651afbf608a (old id 8539618)
- date added to LUP
- 2016-04-01 12:52:59
- date last changed
- 2024-01-09 04:23:28
@article{012c0496-a92e-4dac-9a36-6651afbf608a,
abstract = {{Context. The astrometric solution for Gaia aims to determine at least five parameters for each star, representing its position, parallax, and proper motion, together with appropriate estimates of their uncertainties and correlations. This requires at least five distinct observations per star. In the early data reductions the number of observations may be insufficient for a five-parameter solution, and even after the full mission many stars will remain under-observed, including faint stars at the detection limit and transient objects. In such cases it is reasonable to determine only the two position parameters. The formal uncertainties of such a two-parameter solution would however grossly underestimate the actual errors in position, due to the neglected parallax and proper motion. Aims. We aim to develop a recipe to calculate sensible formal uncertainties that can be used in all cases of under-observed stars. Methods. Prior information about the typical ranges of stellar parallaxes and proper motions is incorporated in the astrometric solution by means of Bayes' rule. Numerical simulations based on the Gaia Universe Model Snapshot (GUMS) are used to investigate how the prior influences the actual errors and formal uncertainties when different amounts of Gaia observations are available. We develop a criterion for the optimum choice of priors, apply it to a wide range of cases, and derive a global approximation of the optimum prior as a function of magnitude and galactic coordinates. Results. The feasibility of the Bayesian approach is demonstrated through global astrometric solutions of simulated Gaia observations. With an appropriate prior it is possible to derive sensible positions with realistic error estimates for any number of available observations. Even though this recipe works also for well-observed stars it should not be used where a good five-parameter astrometric solution can be obtained without a prior. Parallaxes and proper motions from a solution using priors are always biased and should not be used.}},
author = {{Michalik, Daniel and Lindegren, Lennart and Hobbs, David and Butkevich, Alexey G.}},
issn = {{0004-6361}},
keywords = {{astrometry; methods: data analysis; methods: numerical; parallaxes; proper motions; space vehicles: instruments}},
language = {{eng}},
publisher = {{EDP Sciences}},
series = {{Astronomy & Astrophysics}},
title = {{Gaia astrometry for stars with too few observations. A Bayesian approach}},
url = {{http://dx.doi.org/10.1051/0004-6361/201526936}},
doi = {{10.1051/0004-6361/201526936}},
volume = {{583}},
year = {{2015}},
}