Contents.
      planet: 5 - Jupiter
  satellites: J1-Io      : 149,
              J2-Europe  :  36,
              J3-Ganymede:  20,
              J4-Callisto:   4
total number: 209
        type: relative
       dates: 1990-1992
 observatory: ESO: European Southern Obs. Chile
              BMD: Bowie Maryland USA
              GEA: Grup d'Estuds Astron. No. Spain
              RCI: Reggio Calabria Italy
              ORM: Oak Ridge Obs. Mass. USA
              CAT: Catania Astrophys. Obs. Sicily
              TOK: Tokyo Obs. Japan
              NIC: Nice Obs. France
              TER: Collurania Obs. Teramo Italy
              CAF: Calern, Cote d'Azur France
              KAV: Vainu Bappu Obs. Kavalur India
              PRI: Providence Rhode Island USA
              HAN: Harastua Norway
              OHP: Obs. Haute-Provence France
              PAR: Paris Obs. France
              BSP: Barcelona Spain
              KAK: Kakuda Japan
              ZNL: Zoetermeer Netherlands
              SFC: San Francisco Cal. USA
              DAC: Devon Ast. Obs. Alberta Canada
              BNZ: Adams Obs. Blenheim N. Zealand
              LOW: Lowell Obs. Flagstaff Ariz. USA
              VIA: Victoria NSW Australia
              PIC: Pic du Midi France
              RIO: Rio de Janeiro Brazil
              BOR: Bordeaux Univ. Obs. France
              MEU: Meudon Obs. France
              CNR: Cluj-Napoca Obs. Romania
              SSA: Siding Spring Obs. Australia
              MKH: Mauna Kea, Hawaii
              TOC: Toronto Ontario Canada
              BRB: Brasopolis Brazil
              DNC: Durham North Carolina USA
              BER: Berlin Germany
              HEG: Heuweiler Germany
              ESS: Essen Germany
              HNY: Holtsville New York USA
              TMR: Timisoara Romania
              TPK: Topeka Kansas USA
              BEL: Belgrade Obs. Serbia

Reference.
   Kaas A. A., Aksnes K., Franklin F., Lieske J. (1999)
   Astrometry from Mutual Phenomena
   of the Galilean Satellites in 1990-1992.
   The Astronomical Journal. V. 117. N. 4. P. 1933-1941.
   1999AJ____117_1933K

Informations.
         relative to: J1-Io      :  10,
                      J2-Europe  : 158,
                      J3-Ganymede:  30,
                      J4-Callisto:  11
     reference frame: astrometric
     centre of frame: topocentre
    epoch of equinox: no information
          time scale: UTC
           reduction: no information
         coordinates: differential or X, Y  ???
    diff. refraction: no information
            receptor: photometry
           telescope: no information
           observers: no information
 data included in standard data file: no

Comments.

Format.
  1. (Code of obs) Code of observatory (see above)
  2. (Ref sat) Reference satellite (eclipsing or occulting)
  3. (Type of ev.) Type of mutual phenomena: o - occultation, e - eclipse
  4. Subject satellite (eclipsed or occulted)
  5. Year   of the moment of observation
  6. Day (!) of the moment of observation
  7. Month  of the moment of observation
  8. Hour   of the moment of observation
  9. Minute of the moment of observation
 10. Second of the moment of observation with decimals
 11. (DT) Time correction, see article (correction to the midtime taken
                                        without the phase correction), s
 12. (Dx) Longitude correction to Sampson's (1921) theory, km
 13. (Dz) Latitude correction to Sampson's (1921) theory, km
 14. (D(R.A.)) Separation between the satellites
       (subject satellite - reference satellite) in right ascension, arcsec
       (geocentric for occultation, heliocentric for eclipse)
 15. (D(decl.)) Separation between the satellites
       (subject satellite - reference satellite) in declination, arcsec
       (geocentric for occultation, heliocentric for eclipse)
 16. (JED) Ephemeris time at Jupiter
 17. (PH1) Orbital phase angle, degrees (geocentric for occultation,
           heliocentric for eclipse)
 18. (PH2) Orbital phase angle, degrees (geocentric for occultation,
           heliocentric for eclipse)
 19. (Weight) Weights calculated according to a formula
        discussed by Aksnes and Franklin (1976)
 20. (N) Note (if equal to 1) that latitude correction is not accurate
     (see article, it corresponds to the apperance of Dz in parentheses
      in the table in the article)

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Code Ref Type Sub                                       D(R.A.) D(decl.)                  Weight
of   sat of  sat     day                                               JED -    PH1   PH2      Note
obs      ev.     Year  month   UTC        DT     Dx   Dz              2448000
                             h  m  s      s      km   km arcsec arcsec          deg   deg
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