Contents. planet: 6 - Saturn satellites: S2-Enceladus : 151, S3-Tethys : 598, S4-Dione : 527, S5-Rhea : 970, S7-Hyperion : 106, S8-Iapetus : 184 total number: 2536 type: relative dates: 1995-1995 observatory: 073 - Bucharest Reference. Vass G. (1997) CCD positions of the saturnian satellites. Romanian astronomical journal. V. 7. No. 1. P. 45-109. 1997RoAJ____7___45V Informations. relative to: S3-Tethys : 63, S4-Dione : 129, S6-Titan :2285, S8-Iapetus : 59 reference frame: astrometric centre of frame: geocentre epoch of equinox: date time scale: UTC reduction: no information coordinates: X, Y diff. refraction: no information receptor: CCD telescope: Astrograph, F = 6 m, D = 38 cm observers: Vass G. data included in standard data file: no Comments. O-C(X), O-C(Y) are published evaluation: The differences O-C(X), O-C(Y) are published in the article. For these values one have X Y M. (mean) 0.188" -0.066" R.M.S. (root mean square) 0.563" 0.860" The differences O-C(X)e, O-C(Y)e were calculated by N.Emelianov with the theory by Harper & Taylor. With these O-C one have X Y M. (mean) -0.002" 0.038" R.M.S. (root mean square) 0.340" 0.228" Format. 1. Number of satellite (N sat) 2. Number of reference satellite (N ref) 3. Year of the moment of observation 4. Month of the moment of observation 5. Day of the moment of observation with decimals 6. Hour of the moment of observation 7. Minute of the moment of observation 8. Seconde of the moment of observation 9. X, arcsec 10. O-C(X) for X, arcsec 11. Y, arcsec 12. O-C(Y) for Y, arcsec 13. Signal to Noise ratio (S/N) 14. Integration time, seconds 15. Dispersion for X, arcsec 16. Dispersion for Y, arcsec ------------------------------------------------------------------------------ N UTC X O-C Y O-C Integr. Disp. N ref h m s (X) (Y) time (X) (Y) sat Year month day arcsec arcsec S/N sec. arcsec ------------------------------------------------------------------------------