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I.Kulyk, K.Jockers, N.Karpov, A.Sergeev
Positions of the inner Jovian moons.
Description:
The catalogue includes 303 intersatellite positions of the inner
Jovian moons Thebe, Amalthea, Adrastea and Metis derived from
the observations made with the 2-m Zeiss RCC telescope
of Terskol Observatory (Terskol peak, Northern Caucasus, long=42.50083
deg, lat= 43.27427 deg, h=3100m) in 1999-2001.
The Two-Channel Focal Reducer of the Max-Planck Institute
for Aeronomy (MPAe,Germany) was used for acquisition
of the images. The optical arrangement of this device and the
main parameters of the optical system are published in [1].
We provide delta(alpha) and delta(delta) of Thebe and Amalthea with respect
to the Galilean satellites, while the positions of Adrastea and Metis
are referred to either the Galilean moons or to Thebe or to Amalthea.
Since our frames cover the field of the Galilean moons,they
were used as the reference points forming the reference direction on the
frames.
Astrometric topocentric coordinates J2000.0 of the Galilean satellites
were used for scale and orientation angle determination.
The array scale was corrected for differential refraction
and differential aberration to ferst-order.
All observed positions are compared with theoretical ones.
Residual statistics show the inner accuracy of our observations in the range
from about 0.1 to 0.9 arcsec. The slight dependence of the differences
of the observed and calculated positions on the distances from Jupiter
has been found for our observations of Metis and Adrastea.
[1] Jockers K., Credner T., Bonev T., et al.,
KFNT , 2000,Suppl. Ser. 3, 13 .
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File Summary:
File Name Lrec Records Explanations
c4_dese.htm 80 . This file
File c4_dat.htm: 43 303 Observed astrometric positions
of inner Jovian satellites
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Bytes Format Units Label Explanations
1-4 I4 year OBSy Date of observation (year)
5-7 I3 month OBSm Date of observation (month)
8-10 I3 day OBSd Day of observation (day)
11-13 I3 hour OBSh Time of observation in UT (hour)
14-16 I3 min OBSm Time of observation in UT (min)
17-19 I3 sec OBSs Time of observation in UT (sec)
20-27 F8.2 arcsec X X=15*delta(alpha)*cos(del)
28-35 F8.2 arcsec Y Y=delta(delta)
36-39 I4 --- Ns Number of satellite (1)
40-43 I4 --- Nrs Number of reference satellite (1)
=============================================================================
Note(1): Satellite number 505:Amalthea, 514:Thebe, 515: Adrastea, 516: Metis,
501:Io , 502:Europa, 503: Ganymede, 504: Callisto
Data (32.2Kb)
Data byte to byte description
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of 2.5 Million Stars (ASCC-2.5, 2-nd version).
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S. P. Rybka & A. I. Yatsenko
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identified from 2MASS photometry in 10 sky areas.
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Catalogue of 2.2 million
candidates for Red Clump giants selected from the 2MASS down to Ks = 11 magnitude
at galacic latidudes 5° < |b| < 30°.
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stellar proper motions at the South Galactic Pole.
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and infrared photometry of stars at the North Galactic Pole.
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Photometric survey near
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| L.Pakuliak. Questions, remarks and propositions are welcome. |
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