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A Three chords were recorded , using Video OSD technique.
One clearly observed miss was recorded for this event.
View the updated prediction.
Observers:
1(M) G Hudson,Porirua, New Zealand
2 M Forbes,Lower Hutt
3 M Unwin,Wanaka, New Zealand
4 A Pennell, Dunedin, New Zealand
5(P) Prediction, 01 April
Discussion:
The ellipse above is plotted at the best fit axis ratio as determined by Occult. With 3 chords we can be confident of the path of Aspasia and that it was north of the predicted line. The Damit/ISAM 3D model has been overlaid on the measured ellipse and shows poor fit. This has turned out to be quite a difficult event to sort out and even now the result is only partially satisfactory. The main problem is that the star was faint (mag 12.7) and the mag drop was small (0.2 m) All observers were using long integration times (x32 to x64 frames = 1.28 to 2.56 secs) so the time resolution is poor even when measured using AOTA and R-OTE. I have checked and rechecked Gordon's data and cannot find anything that is a convincing dip. The other 3 observers have dips that are consistent with the expected mag drop but all seem to show slow D and R. It seems that the major source of noise is in the Analogue cables and the A to D converter. All observers are to be congratulated in end up with data that is of sufficient accuracy to get a reasonable match with the DAMIT model.
The figure below shows the Tangra light curve of Martin's occultation as analysed by AOTA for the main event.
Observational Data:
Observation details for MP ( 409 ) Aspasia
By Star UCAC4 492-144257
On 2014-08-30 at 14:50:37.0
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Observer Murray Forbes
Location Lower Hutt
Longitude +174:58
Latitude -41:09
Altitude 25 m
Datum WGS84
Telescope SCT including Cass and Mak
Aperture 20 cm
Seeing Slight flickering Clear
Camera Type WAT120N+ PAL/CCIR
Camera Delay -0.19
Timing GPS - time inserted Video with frame analysis
Disappearance 14:50:35.89
Reappearance 14:50:42.53
Comments: Lightcurve generated by Limovie. Occult's AOTA used to analyse event,
giving the large uncertainties in the times.
Report prepopulated by IOTA Reporting Add-in for OW ver.1.8
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Observer G Hudson
Location Porirua, New Zealand
Longitude +174:50
Latitude -41:06
Altitude 52 m
Datum WGS84
Telescope SCT including Cass and Mak
Aperture 30 cm
Seeing Steady Clear
Camera Type WAT120N+ PAL/CCIR
Camera Delay -0.05
Timing GPS - time inserted Video with frame analysis
Missed
Comments: Video scan by Limovie Time analysis by AOTA
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Observer Martin Unwin
Location Wanaka, New Zealand
Longitude +169:06
Latitude -44:41
Altitude 300 m
Datum WGS84
Telescope Newtonian
Aperture 15 cm
Seeing Steady Clear
Camera Type WAT120N PAL/CCIR
Camera Delay -0.67
Timing GPS - time inserted Video with frame analysis
Disappearance 14:51:26.06
Reappearance 14:51:41.74
Comments: Video scanned with Limovie and times extracted using AOTA.
Line of sight just above roof of house, seeing affected by thermals.
Report prepopulated by IOTA Reporting Add-in for OW ver.1.8
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Observer Ash Pennell
Location Dunedin NZ
Longitude +170:29
Latitude -45:52
Altitude 136 m
Datum WGS84
Telescope SCT including Cass and Mak
Aperture 35 cm
Seeing Slight flickering Clear
Camera Type WAT120N+ PAL/CCIR
Camera Delay -1.31
Timing GPS - time inserted Video with frame analysis
Disappearance 14:51:26.30
Reappearance 14:51:36.82
Comments: Times by Aota Tangra scan