Astrometry with large un-astrometric telescopes

Details Astrometry with large un-astrometric telescopes Astrometry with large un-astrometric telescopes

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..607p&link_type=abstract

In: Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 J

Astronomy and Astrophysics

Astronomy

Astrometry

Scientific paper

Over the last few decades the number of large-sized telescopes has grown dramatically. Revolutionary CCD technology in combination with the steadily increasing power of computers has changed the way that observational data are being collected and reduced. These new telescopes were designed to produce sharp images of stars and galaxies and are nor necessarily optimized for astrometric measurements. Other drawbacks may include a small field-of-view typically 30 arcmin or less. Further there is presently a lack of reference stars in the range 18

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