Contents.
planet: 6 - Saturn
satellites: S3-Tethys : 1,
S4-Dione : 1,
total number: 2
type: relative
dates: 2009-2010
observatory: 286 - Yunnan Observatory
Reference.
Zhang X., Liu Z., Tang Z. (2013)
Astrometric results of the mutual events between the Saturn's satellites observed at Yunnan Observatory.
Planetary and Space Science. Vol. 76. P. 83-86.
2013P&SS___76___83Z
Informations.
relative to: reference body (an occulted or eclipsed satellite)
S3-Tethys : 1,
S4-Dione : 1
reference frame: astrometric
centre of frame: heliocentric for mutual eclipse, geocentric for mutual occultation
epoch of equinox: J2000
time scale: UTC
reduction: from mutual occultations and eclipses
coordinates: X, Y (heliocentric for mutual eclipse, geocentric for mutual occultation)
diff. refraction: no information
receptor: CCD
telescope: 1-m telescope (first observation), 60-cm telescope (second observation)
observers: no information
data included in standard data file: no
Comments.
Format.
1. Year of observation
2. Month of observation
3. Day of observation
4. The type of the phenomenon (eclipse or occultation) including the
satellite numbers. The type of phenomenon is coded as n_a o n_p
or n_a e n_p for a mutual occultation or eclipse, respectively
Here $n_a$ is the number of the occulting or eclipsing satellite
and $n_p$ is that of the occulted or eclipsed satellite
5. Hour of the midtime of the event (UTC)
6. Minute of the midtime of the event (UTC)
7. Second of the midtime of the event with decimals (UTC)
9. X coordinate in arcseconds (heliocentric for mutual eclipse, geocentric for mutual occultation)
10. Y coordinate in arcseconds (heliocentric for mutual eclipse, geocentric for mutual occultation)
11. sigma of X in arcseconds
12. sigma of Y in arcseconds
13. Position angle A (in degrees) corresponding to X, Y
14. Impact parameter I in arcseconds
15. Flux drop at the minimum of the event (F, %)
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Year Date Type Midtime X Y sigma X sigma Y A I F
Month h m s arcsec arcsec arcsec arcsec deg arcsec %
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