We adopt two theories, G5 (Arlot 1982) and the newest JUP204 (Jacobson 2002), for the four Galilean satellites. In order to compute equatorial coordinates for the satellites, we also use JPL DE405 (Standish 1998) for the Jupiter. While calibrating the CCD field of view, we calculate topocentric positions for the Jupiter and Galilean satellites. Besides, both atmospheric refractions and the central projection (projection of the celestial sphere on the tangential plane of the focal point) are also taken into account. However, no phase effect is corrected for the observations of Galilean satellites since they are made very close to the opposition.
As well known, a small field of view of a CCD
(
)
has no enough reference stars
chosen for calibrating the CCD device. We prefer to use a specific
technique ("Brighter Moon Calibration'' method), which has been
used in the previous works (Harper et al. 1997; Shen
et al. 2001; Vienne et al. 2001; and Paper I) for the calibration in our reduction. Strictly, the "Brighter
Moon Calibration'' method should only be used to obtain
observations of inner faint satellites whose observational errors
are large enough not to be affected by systematic errors in the
scale and orientation caused by errors in the ephemerides of the
bright satellites. Here, this method is used only to test our
image-processing techniques and to assess the internal precision.
Table 1 gives results for the CCD calibration derived by using the four Galilean satellites. We see almost the same parameters for different exp-time subsets when the same ephemeris is used. Besides, for the same exp-time subset a very small difference exists when JUP204 and G5 are used respectively. The scales and orientations solved from all 133 frames of CCD images are adopted in the following reduction.
JUP204 | N | Scale | Orientation |
Subset | (arcsec/pixel) | (degree) | |
1 s exp-time | 43 | 0.373633 | 179.527 |
2 s exp-time | 46 | 0.373631 | 179.529 |
3 s exp-time | 44 | 0.373630 | 179.528 |
Total | 133 | 0.373631 | 179.528 |
G5 | N | Scale | Orientation |
Subset | (arcsec/pixel) | (degree) | |
1 s exp-time | 43 | 0.373657 | 179.521 |
2 s exp-time | 46 | 0.373655 | 179.522 |
3 s exp-time | 44 | 0.373654 | 179.522 |
Total | 133 | 0.373655 | 179.522 |
Calibrated by | JUP204 | ||||||||||
referred theory | JUP204 | G5 | |||||||||
Subset | N | object | mean | s.e. | mean | s.e. | mean | s.e. | mean | s.e. | |
![]() ![]() ![]() |
![]() ![]() |
![]() ![]() ![]() |
![]() ![]() |
||||||||
1 s exp-time | 43 | JI | -47 | 13 | -2 | 11 | 50 | 9 | -4 | 12 | |
43 | JII | 41 | 33 | -30 | 38 | 152 | 33 | -31 | 37 | ||
43 | JIV | 61 | 26 | -49 | 23 | 198 | 26 | -93 | 23 | ||
43 | Jupiter | -49 | 26 | -62 | 33 | 48 | 26 | -81 | 33 | ||
2 s exp-time | 46 | JI | -46 | 13 | -3 | 12 | 50 | 8 | -4 | 13 | |
46 | JII | 42 | 26 | -33 | 31 | 153 | 26 | -34 | 31 | ||
46 | JIV | 61 | 16 | -44 | 23 | 198 | 16 | -88 | 23 | ||
46 | Jupiter | -46 | 24 | -63 | 30 | 52 | 24 | -83 | 30 | ||
3 s exp-time | 44 | JI | -46 | 12 | -3 | 10 | 52 | 6 | -4 | 10 | |
44 | JII | 47 | 21 | -34 | 20 | 158 | 21 | -34 | 19 | ||
44 | JIV | 67 | 12 | -47 | 19 | 204 | 12 | -91 | 19 | ||
44 | Jupiter | -45 | 18 | -63 | 17 | 53 | 18 | -82 | 17 | ||
Total | 133 | JI | -46 | 13 | -2 | 11 | 51 | 8 | -4 | 11 | |
133 | JII | 44 | 27 | -32 | 30 | 154 | 27 | -33 | 30 | ||
133 | JIV | 63 | 19 | -46 | 22 | 200 | 19 | -91 | 22 | ||
133 | Jupiter | -47 | 23 | -63 | 27 | 51 | 23 | -82 | 27 | ||
Calibrated by | G5 | ||||||||||
referred theory | JUP204 | G5 | |||||||||
Subset | N | object | mean | s.e. | mean | s.e. | mean | s.e. | mean | s.e. | |
![]() ![]() ![]() |
![]() ![]() |
![]() ![]() ![]() |
![]() ![]() |
||||||||
1 s exp-time | 43 | JI | -49 | 14 | 0 | 11 | 48 | 9 | -2 | 11 | |
43 | JII | 50 | 33 | -52 | 38 | 169 | 33 | -53 | 37 | ||
43 | JIV | 55 | 26 | -33 | 23 | 192 | 26 | -77 | 23 | ||
43 | Jupiter | -44 | 26 | -77 | 32 | 53 | 26 | -96 | 32 | ||
2 s exp-time | 46 | JI | -49 | 13 | -1 | 12 | 48 | 8 | -2 | 12 | |
46 | JII | 51 | 26 | -56 | 31 | 162 | 26 | -56 | 31 | ||
46 | JIV | 54 | 16 | -27 | 23 | 192 | 16 | -72 | 23 | ||
46 | Jupiter | -41 | 24 | -78 | 30 | 57 | 24 | -98 | 30 | ||
3 s exp-time | 44 | JI | -48 | 12 | -1 | 9 | 49 | 7 | -3 | 10 | |
44 | JII | 57 | 21 | -56 | 20 | 167 | 21 | -57 | 19 | ||
44 | JIV | 60 | 12 | -30 | 19 | 198 | 12 | -75 | 19 | ||
44 | Jupiter | -40 | 18 | -78 | 17 | 58 | 18 | -97 | 17 | ||
Total | 133 | JI | -49 | 13 | -1 | 11 | 48 | 8 | -2 | 11 | |
133 | JII | 53 | 27 | -55 | 30 | 163 | 27 | -56 | 30 | ||
133 | JIV | 56 | 19 | -30 | 22 | 194 | 19 | -75 | 22 | ||
133 | Jupiter | -42 | 23 | -78 | 27 | 56 | 23 | -97 | 27 |
Copyright ESO 2003