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

        

Discussion:

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.

Observational Data:

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