Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-24T02:03:43.907Z Has data issue: false hasContentIssue false
  • English
  • Français

A 3D-Study of the residual vector field

Published online by Cambridge University Press:  07 March 2018

Francisco J. Marco ,
María J. Martínez  and
Jose A. López
Francisco J. Marco
Affiliation:
Universidad Jaume I. Dept. Matemáticas, IMAC. Avda. Vicent Sos Baynat s/n, 12071, Castellón, Spain email: [email protected], [email protected]
María J. Martínez
Affiliation:
Universidad Politécnica de Valencia. Dept. MatemáticaAplicada. IUMPA. Camino de Vera s/n. 46022 Valencia. Spain email: [email protected]
Jose A. López
Affiliation:
Universidad Jaume I. Dept. Matemáticas, IMAC. Avda. Vicent Sos Baynat s/n, 12071, Castellón, Spain email: [email protected], [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

One of the important challenges that Gaia imposes on the Astrometric Catalogs, is a careful study in everything affected by parallax. A particularly important case is the necessary linkage Gaia - HCRF - ICRF2, which require methods of analysis that are accurate enough so that the provided results are at the same precision level as the work data.

Keywords

astronomical data bases: miscellaneouscatalogsreference systems
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 235 - 236
Copyright
Copyright © International Astronomical Union 2018