planet: 6-Saturn
  satellites: S7-Hyperion:4
total number: 4
        type: relative
       dates: 1984-1984
 observatory: 119 - Abastumani, Georgia

   Kisseleva T.P., Chanturiya S.M. (2000)
   The determination of positions of saturnian satellites -
   Dione, Rhea, Titan, Hyperion and Iapetus by photographic
   observations in Abastumany astrophysical observatory of
   science academy of Georgia.
   Izvestiia glavnoi astronomicheskoi observatorii
   Pulkovo. N. 214. P. 356-360.

         relative to: 6-Titan
     reference frame: astrometric
     centre of frame: topocentre
    epoch of equinox: J2000
          time scale: UTC
           reduction: ACT catalogue
         coordinates: differential
    diff. refraction: removed
            receptor: photographic
           telescope: Double wide-field astrograph,
                      D = 40 cm, F = 302.4 cm
           observers: Kisseleva T.P., Chanturiya S.M.
 data included in standard data file: no

     All these observations as absolutes
     are in the portion sm0027
          evaluation: The differences  O-C(X), O-C(Y) were
                      calculated by N.Emelianov with the theory by
                      Harper & Taylor.
                      With these O-C one have
                                                     X        Y
                      M. (mean)                    1.089"  -0.493"
                      R.M.S. (root mean square)    1.189"   0.589"

  1. Year   of the moment of observation
  2. Month  of the moment of observation
  3. Day    of the moment of observation with decimals
  4. Number of satellite (N sat)
  5. Number of reference satellite (N ref)
  6. Delta(alpha), arcsec
  7. Delta(delta), arcsec
  8. O-C(X) for alpha, arcsec
  9. O-C(Y) for delta, arcsec

Year      UTC      N   N     D(alpha)               O-C
  month day       sat ref          D(delta)  D(alpha) D(delta)
  with decimals                arcsec             arcsec