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5. The observations

In Tables 6-9, we give the observed positions of the satellites in the form of pixel coordinates, as described in the previous section. These are apparent topocentric data; no correction has been made for the effects of refraction, stellar aberration or parallax. The date and time of the middle of the exposure are given in Universal Time. The exposure time is also given.. The satellites are listed in the conventional order of increasing semi-major axis.

Table 6: Observations made in 1990

Table 7: Observations made in 1991

Table 8: Observations made in 1993

Table 9: Observations made in 1994

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