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- W3098889135 abstract "In order to study the potential in high precision CCD astrometry of irregular satellites, we have made experimental observations for Himalia, the sixth and irregular satellite of Jupiter. A total of 185 CCD observations were obtained by using the 2.4 m telescope and 1 m telescope at Yunnan Observatories over ten nights. Preliminary analysis for the observations were made, including the geometric distortion, the atmospheric refraction, and also the phase effect. All positions of Himalia are measured relative to the reference stars from the catalogue UCAC4 in each CCD field of view. The theoretical positions of Himalia were retrieved from the IMCCE, while the positions of Jupiter were obtained based on the planetary theory INPOP13C. The results show that the mean (O-C) (observed minus computed) residuals are -0.004 and -0.002 arcsec in right ascension and declination, respectively. The standard deviation of (O-C) residuals are estimated at about 0.04 arcsec in each direction." @default.
- W3098889135 created "2020-11-23" @default.
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- W3098889135 date "2016-11-29" @default.
- W3098889135 modified "2023-09-23" @default.
- W3098889135 title "Preliminary results of CCD observations targeting Himalia acquired at Yunnan Observatories in 2015" @default.
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- W3098889135 doi "https://doi.org/10.1088/1674-4527/16/12/186" @default.
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