Pl. VILight curve · one night

Transit of WASP-52 b

Light curve of the WASP-52 b transit: the star dims while the planet passes in front
Fig. 1Relative flux against time, with the fitted model.
Fig. 2The whole night on video.
Star field with the target and comparison stars marked
Fig. 3The field: target and comparison stars.
Notes

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

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