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Paper: Star-Cluster Astrometry with Ground-Based Wide Field Imagers
Volume: 338, Astrometry in the Age of the Next Generation of Large Telescopes
Page: 118
Authors: Bedin, L.R.; Anderson, J.; Piotto, G.; Momany, Y.; Yadav, R.S.
Abstract: We show the astrometric potential of the Wide Field Imager at the focus of the MPI-ESO 2.2m Telescope. Currently, we are able to measure the position of a well-exposed star with a precision of ~4 mas/frame in each coordinate (under 0.8 arcsec seeing conditions). We present some preliminary results here.
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