Characterizing the Astrometric Errors in the Gaia Catalogue
(2011) In EAS Publications Series 45(GAIA: At the Frontiers of Astrometry). p.117-122- Abstract
- Accurate characterization of the errors in the global astrometric solution for Gaia is essential for making optimal use of the catalogue data. We investigate the structure of the covariance between the estimated astrometric parameters by studying the properties of the astrometric least squares solution. We find that astrometric errors can be separated in a star and an attitude part, due to the estimation of the star and attitude parameters respectively. Hence the covariances can be separated in a star, an attitude and a cross term. This is demonstrated using our scalable simulation tool AGISLab, where the covariances are estimated statistically using Monte Carlo techniques.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/1894766
- author
- Holl, Berry
LU
; Lindegren, Lennart
LU
and Hobbs, David LU
- organization
- publishing date
- 2011
- type
- Contribution to journal
- publication status
- published
- subject
- in
- EAS Publications Series
- volume
- 45
- issue
- GAIA: At the Frontiers of Astrometry
- pages
- 117 - 122
- publisher
- EDP Sciences
- external identifiers
-
- wos:000289226200020
- scopus:79956132212
- ISSN
- 1633-4760
- DOI
- 10.1051/eas/1045020
- language
- English
- LU publication?
- yes
- id
- eebcbd87-1daf-45bf-ae24-c7f8a94bf90b (old id 1894766)
- date added to LUP
- 2016-04-01 10:15:05
- date last changed
- 2025-04-04 14:24:26
@article{eebcbd87-1daf-45bf-ae24-c7f8a94bf90b, abstract = {{Accurate characterization of the errors in the global astrometric solution for Gaia is essential for making optimal use of the catalogue data. We investigate the structure of the covariance between the estimated astrometric parameters by studying the properties of the astrometric least squares solution. We find that astrometric errors can be separated in a star and an attitude part, due to the estimation of the star and attitude parameters respectively. Hence the covariances can be separated in a star, an attitude and a cross term. This is demonstrated using our scalable simulation tool AGISLab, where the covariances are estimated statistically using Monte Carlo techniques.}}, author = {{Holl, Berry and Lindegren, Lennart and Hobbs, David}}, issn = {{1633-4760}}, language = {{eng}}, number = {{GAIA: At the Frontiers of Astrometry}}, pages = {{117--122}}, publisher = {{EDP Sciences}}, series = {{EAS Publications Series}}, title = {{Characterizing the Astrometric Errors in the Gaia Catalogue}}, url = {{http://dx.doi.org/10.1051/eas/1045020}}, doi = {{10.1051/eas/1045020}}, volume = {{45}}, year = {{2011}}, }