Pl. VLight curve · one night

Transit of TrES-2 b

Light curve of the TrES-2 b transit: the star dims while the planet passes in front
Fig. 1Relative flux against time, with the fitted model.
Star field with the target and comparison stars marked
Fig. 2The field: target and comparison stars.
Notes

Partial result. The mid-transit time is valid for O−C; the depth is not, because part of the transit is missing or there was a meridian flip in the middle.

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