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Optimality of the maximum likelihood estimator in astrometry
(EDP Sciences, 2018)
Context. Astrometry relies on the precise measurement of positions and motions of celestial objects. Driven by the ever-increasing
accuracy of astrometric measurements, it is important to critically assess the maximum ...
Optical astrometry of Benchmark radio sources IV. New results in the southern hemisphere
(1997-05-01)
Optical positions relative to the International
Reference Stars Catalogue (IRS), and therefore in the system
of the FK5, have been obtained for the optical counterparts
of 40 compact extragalactic radio sources south
of ...
Ground-based CCD astrometry with wide-field imagers. II. A star catalog for M 67: WFI@2.2 m MPG/ESO astrometry, FLAMES@VLT radial velocities
(2008)
Context. The solar-age open cluster M 67 (C0847+120, NGC 2682) is a touchstone in studies of the old Galactic disk. Despite its outstanding role, the census of cluster membership for M 67 at fainter magnitudes and their ...
Information and decision theory as applied to astronomy: The case of astrometry and photometry
(2015)
Applying results from information and decision theory, in particular the Cram´er-Rao lower variance bound, we place limits on the maximum astrometric precision attainable by a CCD detector given the properties of the source, ...
CCD astrometry of faint compact extragalactic radio sources. II.
(2001)
Optical positions relative to the Hipparcos Catalogue (ESA 1997) have been obtained for the optical
counterparts of 28 faint (B 20−23) southern compact extragalactic radio sources (CERS). Most of these sources
are not ...