A new method for dynamical analysis of orientation errors from non regular samples

Details A new method for dynamical analysis of orientation errors from non regular samples A new method for dynamical analysis of orientation errors from non regular samples

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jsrs.meet..232l&link_type=abstract

In: Journées 2004 - systèmes de référence spatio-temporels. Fundamental astronomy: new concepts and models for high accuracy obs

Astronomy and Astrophysics

Astronomy

Reference Systems, Orientation

Scientific paper

The main aim of this paper is the analysis of the orientation errors of
a celestial reference system from the differences between observed and
calculated positions for a set of selected minor planets. In this paper
a new numerical method not based on the Gauss-Markov will be presented.

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