This is confirmed at several places inside the paper. A systematic component of 0.3 mas should be added to the parallax uncertainties". 2016 ) states that "For the primary astrometric data set the typical uncertainty is about 0.3 mas for the. The abstract of the Gaia DR1 release paper (Gaia Collaboration et al. What happens to newly detected solar system objects (Gaia asteroid observations)? I'm not interested in stars, I'm interested in galaxies. How can Gaia G, BP and/or RP values be transformed to V magnitudes? When will you start releasing information about them? Will you calculate orbital elements for them? I'm not interested in stars, I'm interested in minor bodies in the Solar System. Where can I check how many times and when Gaia will observe my favourite object? What is the Robust Scatter Estimate (RSE)? What does the first Gaia catalogue look like? Is there any way to find out about transient objects immediately to do follow-up observations on-ground? Is there an input catalogue for Gaia? If yes, how are transient objects like supernova discovered? What is the Gaia scanning law and how does it work? What will be the most common type of star in the Gaia catalogue? How many objects in our solar system will Gaia detect? What is Gaia's astrometric, photometric and spectroscopic performance? What can amateur astronomers contribute to the mission? ![]() Which telescopes are being used to track Gaia from the ground? When did Gaia's routine science operations phase start? ![]() Where will I be able to find all scientific papers that use Gaia data? How shall I acknowledge Gaia? When do I acknowledge Gaia?
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