Contents.
      planet: 6 - Saturn
  satellites: S1 - Mimas:       5
              S2 - Enceladus:  14
              S3 - Tethys:     19
              S4 - Dione:       8
              S5 - Rhea:        6
total number: 26
        type: relative
       dates: 2008-2009
 observatory: see below

Reference.
Arlot J.-E., Emelyanov N. V., Lainey V., Andreev M., Assafin M.,
Braga-Ribas F., Camargo J. I. B., Casas R., Christou A., Colas F.,
Da Silva Neto D. N., Dechambre O., Dias-Oliveira A., Dourneau G.,
Farmakopoulos A., Gault D., George T., Gorshanov D. L., Herald D.,
Kozlov V., Kurenya A., Le Campion J. F., Lecacheux J., Loader B.,
Massalle A., Mc Brien M., Murphy A., Parakhin N., Roman-Lopes A.,
Schnabel C., Sergeev A., Tsamis V., Valdes Sada P.,
Vieira-Martins R., Zhang X. 
Astrometric results of observations of mutual occultations and eclipses
of the Saturnian satellites in 2009.
Astronomy and Astrophysics. 2012. V. 544. Id. A29. 
   2012A&A___544A__29A

Informations.
           relative to: relative to other satellite
       reference frame: astrometric
       center of frame: topocenter
      epoch of equinox: ICRF
            time scale: UTC
             reduction: mutual phenomena
           coordinates: X, Y
      diff. refraction: no information
              receptor: photometric CCD, Video
             telescope: see in the paper
             observers: see in the paper
data included in standard data file: no

Comments.
  See Coordinates of observatories
                                            Code     Longitude     Lalitude  Altitude
Titre of observatory                                 deg  '  "    deg  '  "     m
-------------------------------------------------------------------------------------
Ellinogermaniki Agogi School Obs. (Greece)   ATH      23 53 35 E   37 59 52 N  165
Canberra (Australia)                         KAM     149 03 48 E   35 23 49 S  582
Bordeaux (France)                            BDX       0 31 36 W   44 50 06 N   73
Darfield (New Zealand)                       DAR     172 06 24 E   43 28 53 S  210
Itajuba (Brazil)                             IT1      45 35  0 W   22 32 06 S 1870
Itajuba (Brazil)                             IT2      45 35  0 W   22 32 06 S 1870
CTIO, Cerro Tololo (Chile)                   LAS      70 48 53 W   30 09 55 S 2200
Meudon (France)                              MEU       2 13 54 E   48 48 18 N  162
Monterrey (Mexico)                           MTR     100 20 46 W   25 37 23 N  689
Montigny-le–Bretonneux (France)              MON       2 00 52 E   48 45 54 N  168
Pic du Midi (France)                         PIC       0 08 34 E   42 56 11 N 2850
Pulkovo-Kislovodsk (Russia)                  GAS      42 40 04 E   43 44 52 N 2070
Sabadell (Spain)                             SAB       2 05 29 E   41 33 04 N  224
Sabadell (Spain)                             SAM       2 05 29 E   41 33 04 N  224
San Esteve Sesrovires (Spain)                SCH       1 52 22 E   41 29 40 N  170
Sydney (Australia)                           SYD     150 38 34 E   33 39 37 S  271
Terskol (Russia)                             TER      42 30 03 E   43 16 36 N 3100
Umatilla (Oregon, USA)                       UMA     119 17 46 W   45 55 20 N  130
Yunnan Obs. (China)                          YUN     102 47 15 E   25 01 45 N 1940 
-------------------------------------------------------------------------------------

Format.
  1. Year   of the moment of observation
  2. Month  of the moment of observation
  3  Day    of the moment of observation with decimals
  4. Type - the type of the phenomenon (eclipse or occultation)
     including the satellite numbers in the form 
     "nem" (eclipse) or "nom" (occultation),
     where n is the number of the occulting or eclipsing satellite
     and m - is the number of the occulted or eclipsed satellite. 
  5. Observatory code (Code)
  6. Hour of the moment of observation
  7. Minute of the moment of observation
  8. Secondes of the moment of observation with decimals
  9. X, arcsec
 10. Y, arcsec
 11. sigma X, arcsec
 12. sigma Y, arcsec
 13. Q - index of the result quality, following from processing:
     Q=0 - normal result,
     Q=2 - result following from low quality photometry. 

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Year    Day   Code  Moment, UTC     X      Y      sigma X  sigma Y
   Month  Type      h  m  s      arcsec   arcsec   arcsec   arcsec  Q 
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