A Two positive occultations were recorded by , using the ADVS video technique.
View the updated prediction.
Observers: 1 D Gault,Hawkesbury Heights, NSW, AU 2 T Barry,Werrington Downs,NSW,AU 3(P) Prediction, TT14 29 March
The circle above is plotted at the expected 62 km diameter of Pafuri.
With two nearby chords it is not possible to determine whether Dave and Tony were north
or south of the central line of the event.
Tony's long integration (2 sec per sample) means that there is high uncetainty in the times and the error bars overlap. The plot has been adjusted to centre between Dave's times. This was the first event with two ADVS units being used and has led to a number of suggestions for recording.
The figure below shows Dave's Tangra light curve of the occultation.
The figure below shows Tony's Tangra light curve of the occultation.
Observation details for MP ( 1032 ) Pafuri By Star UCAC4 329-177069 On 2013-04-28 at 16:01:19.0 _______________________________ Observer Dave Gault Location Hawkesbury Heights, NSW, AU Longitude +150:38 Latitude -33:39 Altitude 286 m Datum WGS84 Telescope SCT including Cass and Mak Aperture 30 cm Seeing Steady Clear Camera Type ADVS ADVS Camera Delay 0 0.27 Sec Integration Timing GPS - time inserted Video with frame analysis Disappearance 16:01:39.702 Reappearance 16:01:47.435 Comments: Light Curve plot attached. Temperature = 14C _______________________________ Observer Tony Barry Location Werrington Downs Longitude +150:43 Latitude -33:44 Altitude 35 m Datum WGS84 Telescope SCT including Cass and Mak Aperture 25 cm Seeing Steady Clear Camera Type ADVS ADVS Camera Delay 0 2 sec integration Timing GPS - time inserted Video with frame analysis Disappearance 16:01:42.29 Reappearance 16:01:50.29 Comments: Report prepopulated by IOTA Reporting Add-in for OW ver.1.7