Star-Cluster Astrometry with Ground-Based Wide Field Imagers

Simple item page
dc.creatorBedin, L. R.
dc.creatorAnderson, J.
dc.creatorPiotto, G.
dc.creatorMomany, Y.
dc.creatorYadav, R. S.
dc.date2005-03-30
dc.date.accessioned2026-07-07T02:17:20Z
dc.date.available2026-07-07T02:17:20Z
dc.descriptionWe 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 $\sim$4 mas/frame in each coordinate (under 0.8 arcsec seeing conditions). We present some preliminary results here.
dc.description4 pages, 3 figures, from "Astrometry in the Age of the Next Generation of Large Telescopes", 18-20 October 2004, Flagstaff, ASP Conf. Ser. in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0503650
dc.identifierhttp://arxiv.org/abs/astro-ph/0503650
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9137
dc.subjectAstrophysics
dc.titleStar-Cluster Astrometry with Ground-Based Wide Field Imagers
dc.typetext

Files

Collections

arXiv