TL;DR
This paper introduces the Astrometry Spread Function (ASF) for Gaia DR2, enabling precise modeling of expected astrometric uncertainties and excess noise, which enhances the analysis of various astrophysical phenomena.
Contribution
The paper develops and validates the ASF model for Gaia DR2, providing a new tool to characterize astrometric uncertainties and excess noise in Gaia data.
Findings
ASF accurately models Gaia DR2 astrometric uncertainties.
ASF enables estimation of excess source noise.
High completeness in Gaia astrometric sample for G<20.
Abstract
Gaia DR2 published positions, parallaxes and proper motions for an unprecedented 1,331,909,727 sources, revolutionising the field of Galactic dynamics. We complement this data with the Astrometry Spread Function (ASF), the expected uncertainty in the measured positions, proper motions and parallax for a non-accelerating point source. The ASF is a Gaussian function for which we construct the 5D astrometric covariance matrix as a function of position on the sky and apparent magnitude using the Gaia DR2 scanning law and demonstrate excellent agreement with the observed data. This can be used to answer the question `What astrometric covariance would Gaia have published if my star was a non-accelerating point source?'. The ASF will enable characterisation of binary systems, exoplanet orbits, astrometric microlensing events and extended sources which add an excess astrometric noise to the…
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