Astrometric observations of Nereid in 2006-2007
DOURNEAU, G.
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
TANG, Z. H.
United Laboratory for Optical Astrometry
Shanghai Astronomical Observatory [Shanghai] [SHAO]
< Réduire
United Laboratory for Optical Astrometry
Shanghai Astronomical Observatory [Shanghai] [SHAO]
Langue
en
Article de revue
Ce document a été publié dans
Monthly Notices of the Royal Astronomical Society. 2008, vol. 391, p. 1791-1795
Oxford University Press (OUP): Policy P - Oxford Open Option A
Résumé en anglais
In this paper, we present 112 new CCD astrometric positions of Nereid, the second and faint satellite of Neptune (mv ! 19). We observed this small satellite in the 2006-2007 period with the 1m and the 2.16m telescopes of ...Lire la suite >
In this paper, we present 112 new CCD astrometric positions of Nereid, the second and faint satellite of Neptune (mv ! 19). We observed this small satellite in the 2006-2007 period with the 1m and the 2.16m telescopes of Xinglong Station near Beijing, both equipped with large CCD detectors of 1340 × 1300 and 2048 × 2048 pixels, respectively. The high-density and highly accurate star catalogue UCAC2 (Zacharias, 2004) was used in the reduction so that a classical astrometric calibration method was applied. We have shown that our observations of Nereid appear to be of equal or higher precision (! ! 0.2”) than most of the recent CCD ones.< Réduire
Mots clés en anglais
planets and satellites
satellites of Neptune
astrometry
Origine
Importé de halUnités de recherche