Implementing the Gaia Astrometric Global Iterative Solution (AGIS) in Java
arXiv:1108.2206 · doi:10.1007/s10686-011-9248-z
Abstract
This paper provides a description of the Java software framework which has been constructed to run the Astrometric Global Iterative Solution for the Gaia mission. This is the mathematical framework to provide the rigid reference frame for Gaia observations from the Gaia data itself. This process makes Gaia a self calibrated, and input catalogue independent, mission. The framework is highly distributed typically running on a cluster of machines with a database back end. All code is written in the Java language. We describe the overall architecture and some of the details of the implementation.
Accepted for Experimental Astronomy
References in corpus (2)
Cited by in corpus (6)
- Gaia Data Release 1: Astrometry - one billion positions, two million proper motions and parallaxes
- The Gaia inertial reference frame and the tilting of the Milky Way disk
- Gaia predicted brown dwarf detection rates around FGK stars in astrometry, radial velocity, and photometric transits
- The Global sphere reconstruction (GSR) - Demonstrating an independent implementation of the astrometric core solution for Gaia
- A conjugate gradient algorithm for the astrometric core solution of Gaia
- The MPI + CUDA Gaia AVU-GSR Parallel Solver Toward Next-generation Exascale Infrastructures