Astrometry of satellites I to V of Uranus 1990-1991

Details Astrometry of satellites I to V of Uranus 1990-1991 Astrometry of satellites I to V of Uranus 1990-1991

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..130...77j&link_type=abstract

Astronomy and Astrophysics Supplement, v.130, p.77-80

Astronomy and Astrophysics

Astrophysics

8

Planets And Satellites: Satellites Of Uranus, Observations Astrometry

Scientific paper

139 CCD images of the Uranian satellite system taken with the Jacobus Kapteyn Telescope in 1990 and 1991 have been calibrated astrometrically with two WFC photographic plates taken on the same telescope in 1996. The numbers of images are: I Ariel 139; II Umbriel 132; III Titania 137; IV Oberon 128; V Miranda 117; total 653. The root-mean-square (rms) fits of the inter-satellite positions to the numerical integration by \cite[Taylor (1998)]{Tayl:or} lie between 0.025" and 0.061", depending on which two satellites are compared. Table 7 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

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