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A 5 second occultation was recorded by Brian Loader, using an SCT Telescope and Watec 910BD camera.
View the IOTA update.
Observers: 1 B Loader, Darfield, Canterbury, New Zealand 2(P) Prediction- IOTA Feed
Discussion:
The circle above is plotted at the expected diameter of Agamemnon. With only one chord, it is not possible to tell if Brian was east or west of the centre line of the event. The circle has been plotted centred on the observed chord.
The event appears to have been west of the predicted path.
The figure below shows the Tangra light curve of the occultation.
Name:
Observational Data:
Observation details for MP ( 911 ) Agamemnon By Star UCAC4 224-143520 On 2017-08-17 at 15:26:54.0 _______________________________ Observer B. Loader Location Darfield Longitude +172:06 Latitude -43:28 Altitude 210 m Datum WGS84 Telescope SCT including Cass and Mak Aperture 25 cm Seeing Strong flickering Thin cloud < 2 Camera Type WAT910BD AAV-PAL Camera Delay Timing GPS - time inserted Video with frame analysis Disappearance 15:26:17.49 Reappearance 15:26:22.77 Comments: Lightcurve from 15:25:31 to 15:27:15 by Tangra v3.6.7 using AperturePhotometry/AverageBackground. Analysis by AOTA v4.3.2.0. Report prepopulated by IOTA Reporting Add-in for OW ver.1.8