Contents.
planet: 6 - Saturn
satellites: S12-Helene : 131,
S13-Telesto : 46,
S14-Calypso : 93
total number: 270
type: relative
dates: 1981-1985
observatory: 809 - La Silla (ESO, Chile)
568 - Mauna Kea (CFH, Hawaii)
Reference.
Oberti P., Veillet C., and Catullo V. (1989) Lagrangian
satellites of Tethys and Dione. I - Reduction of
observations.
Astronomy and Astrophysics Supplement Series.
V.80. N.3. P.289-297.
1989A&AS___80__289O
Informations.
relative to: planet
reference frame: astrometric
centre of frame: topocentre
epoch of equinox: 1 - date,
2 - B1950
time scale: UTC
reduction: no information
coordinates: X, Y
diff. refraction: no information
receptor: photographic
telescope: Observatory ESO (Chile) -
Danish reflector, D=1.54 m
Observatory Mauna Kea (CFH, Hawaii) -
D=3.60 m
observers: Oberti P., Veillet C., Catullo V.
data included in standard data file: no
Comments.
evaluation: The differences O-C(X)e, O-C(Y)e were also
calculated by N.Emelianov with the theory by
P. Oberty
With these O-C one have
X Y
M. (mean) -0.035" 0.072"
R.M.S. (root mean square) 0.432" 0.658"
Format.
1. Number of satellite (N sat)
2. JD of the moment of observation (UT)
3. X=Delta(alpha)*cos(delta), arcsec
4. Y=Delta(delta), arcsec
5. epoch of equinox (N sys): 1 - date, 2 - B1950
6. O-C(X)e for X, arcsec
7. O-C(Y)e for Y, arcsec
8. Number of observatory (N obs)
(809 - La Silla, 568 - Mauna Kea)
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N JD (UT) N O-C(X)e O-C(Y)e
sat X Y sys N
arcsec arcsec arcsec arcsec obs
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