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• W2173304562 startingPage "A71" @default.
• W2173304562 abstract "Context. Gaia’s very accurate astrometric measurements will allow the optical realisation of the International Celestial Reference System to be improved by a few orders of magnitude. Several sets of quasars are used to define a kinematically stable non-rotating reference frame with the barycentre of the solar system as its origin. Gaia will also observe a large number of galaxies. Although they are not point-like, it may be possible to determine accurate positions and proper motions for some of their compact bright features." @default.
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• W2173304562 date "2016-04-14" @default.
• W2173304562 modified "2023-10-15" @default.
• W2173304562 title "<i>Gaia</i>reference frame amid quasar variability and proper motion patterns in the data" @default.
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• W2173304562 doi "https://doi.org/10.1051/0004-6361/201527935" @default.
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