AOTAsteroidal Occultation Time Analyser: Alternative Tool for Asteroidal Occultation Analysis

 
AOTA
 
Asteroidal   Occultation
Time   Analyser
 
AOTA is in Occult 4.1.0.14
 
2
 
and looks like:
 
3
 
Aim
 
Create an alternative tool to analyse asteroidal
occultation light curves
Focus on measuring the D and R events
independently
Handle Limovie & Tangra files
Handle output from integrating cameras
Clear presentation of what is ‘going on’
User friendliness & simplicity – as much as
possible!
 
4
 
Basic methodology
 
Integrity check, for timing inconsistencies
Putative events identified using cross-correlation
analysis
D and R events analysed by fitting a test light
curve of varying transition duration, using a 
χ
2
best fit analysis
Uncertainties determined using a Monte Carlo
analysis, with noise applied to the test light curve
Apply camera-based corrections to the times
 
5
 
If no time stamps, set manually
 
6
 
If start and end time stamps, can fill
with calculated rate. 
But treat with care
 
7
 
Integrity Check
 
Highly desirable to have OCR reading of time
stamp
Looks for irregularities in time stamp
sequence, and for identity in sequential
measurements
For integrating cameras, checks that the
recorded #frames in each integration interval
is constant
 
8
 
Example video with duplicated frames
 
9
 
Can check for systematic problems
with a Fourier Analysis plot
 
Bad
 
Good
 
10
 
Set integration/binning/normalisation
 
11
 
Event identification
 
Test signal extends for the entire recording
duration
Sets a minimum cross-correlation level for a
possible event
Look for symmetric triangle, straight sides,
sharp apex, peak above orange region at
bottom, and light curve flat across the
bottom.
 
12
 
Symmetric triangle with straight sides,
sharp apex, flat light curve at bottom
(see 5 orange bars)
 
13
 
Cloud event – asymmetric, non-straight
sides, no sharp apex, light curve at
bottom not flat (see orange bars)
 
14
 
Can overlay comparison stars
 
Note how the green line drops at the same
time as the cloud event, but not for the
occultation
 
15
 
Can identify up to 5 putative events
 
Each event can be separately analysed
 
16
 
Final plot showing fitted light curve
and uncertainties
 
17
 
Some events have two discrete
possibilities
 
Dunham-Agamemnon
 
18
 
Accuracy visible via 
χ
2
 curves
 
Well-defined
event
 
Poorly-defined
event
 
Small uncertainty
on the ‘-’ side, large
on the 
‘+’ 
side
 
19
 
True gradual
events have a rise
and fall in the
plot of  
χ
2
 
20
 
Disregard anomalous points
 
21
 
Applies corrections based on camera
used
 
22
 
Can view/save measurement report
 
AOTA analysis of the file D:\Videos\ofOthers\Metis\20140307-Metis_Pierrefontaines.csv
- analysed on Wednesday, 26 March 2014 at 3:29 AM UTC
- using AOTA v4.1.0.27
 
Event #1
 
  Event location in video frame ID's
   D: 601.0  +1.0/-0.5
   R: 914.0  +0.5/-0.5
 
  Event time in UTC
   D:  3  8 19.40 ± 0.03
   R:  3  8 31.92 ± 0.02
 
  Duration of transition in frames
   D: 0
   R: 0
 
  SN at event locations
   D: 3.0
   R: 3.3
 
===== Camera details =====
Camera                 : WAT-910BD
Frames integrated      : 0
Video system           : PAL
 
==== Measurement info ====
Measurement tool       : Limovie
Measured at Field level: False
# Measurements binned  : 1
Normalisation          : None
Time scale from tool   : False
 
===== end of report ======
 
23
 
Save plots for sending to others
 
24
 
Detailed Help file provided, with
step-by-step instructions and
guidance on interpretation
 
25
 
Questions?
 
26
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Create an alternative tool for analyzing asteroidal occultation light curves independently, focusing on D and R events. The methodology involves integrity checks, fitting test light curves, and applying camera-based corrections. Manual time stamp setting, calculating time stamps, and integrity checks are crucial steps in the analysis process. Check for systematic problems using Fourier Analysis plots and set integration parameters for accurate analysis.

  • Asteroidal Occultation
  • Light Curve Analysis
  • Alternative Tool
  • Camera-Based Corrections
  • Fourier Analysis

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  1. AOTA Asteroidal Occultation Time Analyser

  2. AOTA is in Occult 4.1.0.14 2

  3. and looks like: 3

  4. Aim Create an alternative tool to analyse asteroidal occultation light curves Focus on measuring the D and R events independently Handle Limovie & Tangra files Handle output from integrating cameras Clear presentation of what is going on User friendliness & simplicity as much as possible! 4

  5. Basic methodology Integrity check, for timing inconsistencies Putative events identified using cross-correlation analysis D and R events analysed by fitting a test light curve of varying transition duration, using a 2 best fit analysis Uncertainties determined using a Monte Carlo analysis, with noise applied to the test light curve Apply camera-based corrections to the times 5

  6. If no time stamps, set manually 6

  7. If start and end time stamps, can fill with calculated rate. But treat with care 7

  8. Integrity Check Highly desirable to have OCR reading of time stamp Looks for irregularities in time stamp sequence, and for identity in sequential measurements For integrating cameras, checks that the recorded #frames in each integration interval is constant 8

  9. Example video with duplicated frames 9

  10. Can check for systematic problems with a Fourier Analysis plot Good Bad 10

  11. Set integration/binning/normalisation 11

  12. Event identification Test signal extends for the entire recording duration Sets a minimum cross-correlation level for a possible event Look for symmetric triangle, straight sides, sharp apex, peak above orange region at bottom, and light curve flat across the bottom. 12

  13. Symmetric triangle with straight sides, sharp apex, flat light curve at bottom (see 5 orange bars) 13

  14. Cloud event asymmetric, non-straight sides, no sharp apex, light curve at bottom not flat (see orange bars) 14

  15. Can overlay comparison stars Note how the green line drops at the same time as the cloud event, but not for the occultation 15

  16. Can identify up to 5 putative events Each event can be separately analysed 16

  17. Final plot showing fitted light curve and uncertainties 17

  18. Some events have two discrete possibilities Dunham-Agamemnon 18

  19. Accuracy visible via 2 curves Well-defined event Small uncertainty on the - side, large on the + side Poorly-defined event 19

  20. True gradual events have a rise and fall in the plot of 2 20

  21. Disregard anomalous points 21

  22. Applies corrections based on camera used 22

  23. Can view/save measurement report AOTA analysis of the file D:\Videos\ofOthers\Metis\20140307-Metis_Pierrefontaines.csv - analysed on Wednesday, 26 March 2014 at 3:29 AM UTC - using AOTA v4.1.0.27 Event #1 Event location in video frame ID's D: 601.0 +1.0/-0.5 R: 914.0 +0.5/-0.5 Event time in UTC D: 3 8 19.40 0.03 R: 3 8 31.92 0.02 Duration of transition in frames D: 0 R: 0 SN at event locations D: 3.0 R: 3.3 ===== Camera details ===== Camera : WAT-910BD Frames integrated : 0 Video system : PAL ==== Measurement info ==== Measurement tool : Limovie Measured at Field level: False # Measurements binned : 1 Normalisation : None Time scale from tool : False ===== end of report ====== 23

  24. Save plots for sending to others 24

  25. Detailed Help file provided, with step-by-step instructions and guidance on interpretation 25

  26. Questions? 26

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