Contents. planet: 6 - Saturn satellites: S1-Mimas : 1, S2-Enceladus: 10, S3-Tethys : 24, S4-Dione : 15, S5-Rhea : 12, S6-Titan : 2 total number: 64 type: relative dates: 1980, 1995-1996 observatory: 005 - Meudon 025 - Stuttgart 073 - Bucharest 095 - Crimea-Nauchnij 130 - Lumezzane 156 - Catania Astrophysical Observatory 262 - European Southern Observatory, La Silla-DSS 387 - Tokyo-Dodaira 511 - Haute Provence 559 - Serra La Nave 586 - Pic du Midi 780 - Leander McCormick Observatory, Charlottesville 874 - Itajuba 999 - Bordeaux-Floirac Reference. Noyelles B., Vienne A., and Descamps P. (2003) Astrometric reduction of lightcurves observed during the PHESAT95 campaign of Saturnian satellites. Astronomy and Astrophysics. V. 401. P. 1159-1175. 2003A&A___401_1159N Informations. relative to: S1-Mimas : 17, S2-Enceladus: 12, S3-Tethys : 11, S4-Dione : 7, S5-Rhea : 12, S6-Titan : 5 reference frame: astrometric centre of frame: 1 - geocenter, 2 - heliocenter (see Format) epoch of equinox: J2000 time scale: UTC reduction: see reference coordinates: X, Y diff. refraction: no information receptor: CCD, photometer telescope: 005 - Reflector D=1.00 m 025 - Reflector D=0.30 m 073 - Reflector D=0.50 m 095 - Reflector D=0.60 m 130 - Reflector D=0.40 m 156 - Reflector D=0.91 m 210 - Reflector D=0.60 m, Reflector D=1.00 m 262 - Reflector D=0.50 m 387 - no information 511 - Reflector D=0.80 m 559 - no information 586 - Reflector D=1.05 m 780 - Reflector D=0.80 m 874 - Reflector D=0.60 m 999 - Reflector D=0.60 m observers: 005 - W. Thuillot, J.-E. Arlot, C. Ruatti, J. Berthier, F. Colas, P. Descamps, D. T. Vu 025 - W. Czech 073 - G. Oprescu 095 - T. R. Irsmambetova, E. M. Trunkovsky 130 - S. Foglia, M. Damani 156 - C. Blanco, V. D'Ambrosio, R. Riccioli 210 - V. G. Tejfel 262 - C. Ledoux 387 - no information 511 - J. Lecacheux, P. Laques 559 - no information 586 - P. Laques, 780 - B. Starosta 874 - C. H. Veiga 999 - G. Dourneau, J.-F. Le Campion, B. Viateau, M. Rapaport data included in standard data file: no Comments. From reference. We give astrometric results derived from reduction of 65 lightcurves made in 1995-1996 during the PHESAT95 campaign (Thuillot et al. 2001) and 4 results derived from Japanese observations made in 1980 (Soma & Nakamura 1982). The accuracy of these results is about 20-30 mas. The format of the present results are very near to the one of (Strugnell & Taylor 1990), more precisely it is the same as (Vienne, Thuillot, Veiga et al. 2001). There are three kinds of results: the best ones (reference 420), other good ones (reference 421) and the other ones, with a reference xxx, because we advise against using them. The split into these three groups has been made when visually comparing the measures with the adjusted theoretical lightcurves, and not when using the residuals. Format. 1. Opposition number, 1=1874 to 118=1995. 2. Year of the moment of observation. 3. Month of the moment of observation. 4. Day of the moment of observation with decimals. 5. TT-UTC in seconds. 6. UAI observatory code from the Minor Planet Center. 7. Qualification of observations (420 - the best ones, 421 - other good ones, xxx - other ones, because we advise against using them). 8. Observation type ( 1 - X, Y) 9. Subject satellite (Ns), reference satellite (Nr), Ns*10+Nr. 10. 11 (flags of presence of the first and second coordinates) 11. Value of X, arcsec. 12. Value of X, arcsec. 13. Reference system (2 - mean equator and equinox of J2000). 14. Reference frame (1 - geocentric, 2 - heliocentric). 15. Residuals of observations in X, arc-seconds (computed with TASS1.7) 16. Residuals of observations in Y, arc-seconds (computed with TASS1.7) 17. The number of the satellite used as reference in the computation of residuals. 18. 0 19. 2 --------------------------------------------------------------------------------