A high probability event recorded under windy and partrly cloudy conditions using ADVS and a Flea3 video camera running at 15 fps fps with Gamma of 4.000



Light curve. A timing correction of -1 frame (-67 ms) hasn't been applied to the times given below.



Light curve of the occulted star (blue) and a comparison star (green) normalized on the comparison star.



The stars before, during and after the occultation.



The ADVS settings used in the recording during the occultation.



Catalog comparison. Observation indicates a small left shift which seems to be closer to the UCAC2 and UCAC3 positions.






Tangra-2 light curve file

Original prediction from IOTAUpdates