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Fig. 5


Chords of the occultation in the plane of the sky and elliptical fit to the chords. The color coding is the same as that in Figs. 3 and 4. The red segments at the chord extremities show the uncertainties from the ingress and egress fits. We note the asymmetry between ingress and egress timing uncertainties in tracks 1, 2, and 6. This is due to operational overheads of the detectors and if the ingress (or the egress) takes place during one of these periods, the uncertainty is larger than that solely due to the photometry noise. The near misses at Sabadell and Agerola are indicated as dashed red lines (easternmost and westernmost respectively).

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