Contents.
planet: 6 - Saturn
satellites: S1 Mimas : 359,
S2 Enceladus : 359,
S3 Thetys : 359,
S4 Dione : 359,
S5 Rhea : 359,
S6 - Titan : 359
total number: 2154
type: relative
dates: 2002-2006
observatory: 286 - Yunnan Observatory
Reference.
Peng Q. Y., Vienne A., Wu X. P., Gan L. L., Desmars J. (2008)
CCD POSITIONS OF SATURN AND ITS MAJOR SATELLITES FROM 2002–2006.
The Astronomical Journal. V. 136. P. 2214–2221.
2008AJ____136_2214P
Informations.
relative to: planet
reference frame: astrometric
centre of frame: geocenter
epoch of equinox: true of date
time scale: UTC
reduction: see reference
coordinates: X, Y
diff. refraction: no information
receptor: CCD
telescope: 1 m telescope
observers: Peng Q. Y., Wu X. P., Gan L. L.
data included in standard data file: no
Comments.
Format.
1. Idenfication of series from Table 2 of the article for the scale
factor and orienation corresponding to each series, ID1.
2. Exposure identification, ID2.
3. Year of Observation (UTC and not light-time corrected).
4. Month of Observation (UTC and not light-time corrected).
5. Day of Observation (UTC and not light-time corrected).
6. IAU observatory code, Obs.
7. Observation type (1 = X, Y), Type.
8. Subject satellite (1-6 = S1 - S6) and reference body (0 = Saturn), Sub.
9. X, arcsec.
10. Y, arcsec.
11. Estimated error in X, arcsec, ErrX.
(Errors from both pixel positions and calibration parameters)
12. Estimated error in Y, arcsec, ErrY.
(Errors from both pixel positions and calibration parameters)
13. Reference system, S (1 = true equator and equinox of date of observation).
14. Reference frame, F (1 = Geocentric).
15. Residual of X with JPL ephemeris, arcsec, O-C_X.
16. Residual of Y with JPL ephemeris, arcsec, O-C_Y.
17. 0 - Saturn use as reference in the computation of (O-C), R.
18. Number of the series (number of the line in the Table 2), Ser.
19. Original X coordinate in pixel coordinates.
20. Original Y coordinate in pixel coordinates.
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ID1 ID2 Month Obs Sub X Y ErrX ErrY O-C_X O-C_Y Ser X Y
Year Day Type arcsec arcsec -arcsec- S F R pix pix
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