Summary: This note describes the results of a planet-course project in which the Gaia detectability of a planet in circular orbit around a solar-like star was studies with AGISLab. Besides a short theoretical background we describe how we modelled and simulated our data.

Bibtex entry for this abstract:

@UNPUBLISHED{LL:BH-003,
author = {B.~Holl},
title={{A}strometric planet detectability with Gaia, a short AGISLab study},
institution={Lund Observatory},
year={2011},
month={September},
url={http://www.rssd.esa.int/doc_fetch.php?id=3097428},
note={GAIA-C3-TN-LU-BH-003},
type={Technical note}
}