Precise positions of Phoebe determined with CCD image-overlapping calibration

Details Precise positions of Phoebe determined with CCD image-overlapping calibration Precise positions of Phoebe determined with CCD image-overlapping calibration

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006mnras.366..208p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 366, Issue 1, pp. 208-212.

Astronomy and Astrophysics

Astronomy

3

Astrometry, Planets And Satellites: Individual: Phoebe

Scientific paper

This paper presents 210 positions of Phoebe, the ninth satellite of Saturn, observed with the 1-m telescope at the Yunnan Observatory during the years 2003-2005, using a CCD image-overlapping calibration method proposed recently by Peng et al. After the observed positions of Phoebe are compared with its theoretical positions computed by the new JPL ephemerides DE405 and SAT199, the mean residuals (observed minus computed) are 0.21 and -0.05arcsec in right ascension and declination, respectively, with a standard deviation of 0.06arcsec.

Affiliated with

Also associated with

No associations

Rating

Precise positions of Phoebe determined with CCD image-overlapping calibration does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Precise positions of Phoebe determined with CCD image-overlapping calibration, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Precise positions of Phoebe determined with CCD image-overlapping calibration will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1493738