#################### PYOTE 4.8.4  session started: Mon Feb 20 12:15:26 2023  ####################

filename: F:/OccvVideos/20230219Tomwhitney/RN-Tomwhitney-PyM.csv

If the csv file came from PyMovie - columns with prefix: signal will be read.

fourcc code of avi: dvvi
fps: 29.97002997002997
avi contains 4298 frames

==================== file header lines ====================
# PyMovie Version 3.6.6
# source: F:\OccvVideos\20230219Tomwhitney.avi
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: tracking1
# ____ aperture size: 31
# ____ x,y: (479, 293)
# ____ threshold: 8
# ____ def mask radius: 4.5
# ____ color: yellow
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 0
#
# aperture name: tracking2
# ____ aperture size: 31
# ____ x,y: (105, 168)
# ____ threshold: 12
# ____ def mask radius: 4.5
# ____ color: yellow
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# aperture name: sky
# ____ aperture size: 31
# ____ x,y: (294, 94)
# ____ threshold: 99999
# ____ def mask radius: 4.5
# ____ color: red
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 2
#
# aperture name: target
# ____ aperture size: 31
# ____ x,y: (247, 77)
# ____ threshold: 99999
# ____ def mask radius: 4.5
# ____ color: green
# ____ joggable: False
# ____ auto textOut: True
# ____ thumbnail source: True
# ____ csv output order: 4
#
==================== end header lines ====================

timeDelta: 0.0333665 seconds per reading
timestamp error rate: 0.00%

tracking1 is selected as the reference curve for normalization.

The reference curve has been deselected so normalization is disabled.

D zone selected: [1876, 1891]

R zone selected: [1916, 1933]

Locate a "D and R" event has been selected

Number of candidate solutions: 288 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:77.10  sigA:47.12 B:284.83 A:-5.40
in entryNum units: D: 1884  R: 1922

noise corr coefs: [1.00, 0.115]  (based on 4230 points)  sigmaB: 74.20

Subframe adjusted solution...
sigB:74.20  sigA:47.08 B:284.83 A:-5.40
in entryNum units: D: 1884  R: 1922  D(subframe): 1884.0000  R(subframe): 1922.0000

in frameNum units: D: 1914  R: 1952  D(subframe): 1914.0000  R(subframe): 1952.0000

... end New solver results

Error bar report based on 100,000 simulations (units are readings)...

loDbar   @ .68 ci:  -0.2269
hiDbar   @ .68 ci:   0.2344
loDbar   @ .95 ci:  -0.6203
hiDbar   @ .95 ci:   0.5185
loDbar   @ .9973 ci:  -1.2039
hiDbar   @ .9973 ci:   1.1072

loDurBar @ .68 ci:  -0.3538
hiDurBar @ .68 ci:   0.3488
loDurBar @ .95 ci:  -0.7861
hiDurBar @ .95 ci:   0.8040
loDurBar @ .9973 ci:  -1.6188
hiDurBar @ .9973 ci:   1.5083

Timestamp validity check ...

From timestamps at D and R, calculated 38 reading blocks.  From reading blocks, calculated 38 blocks.

Timestamps appear valid @ D and R

================= 0.68 containment interval report =================

B: 284.83  {+/- 1.14}  sigmaB: 74.20

A: -5.40  {+/- 7.74}  sigmaA: 47.08

magDrop: NA because 0 < A < B is not satisfied

snr: 3.91

D: 1914.00 {+0.23,-0.23} (frame number)
D: [08:35:13.4455]  {+0.0078,-0.0076} seconds

R: 1952.00 {+0.23,-0.23} (frame number)
R: [08:35:14.7134]  {+0.0076,-0.0078} seconds

Duration (R - D): 38.0000 {+0.3513,-0.3513} readings
Duration (R - D): 1.2679 {+0.0117,-0.0117} seconds

=============== end 0.68 containment interval report ===============

================= 0.95 containment interval report =================

B: 284.83  {+/- 2.28}  sigmaB: 74.20

A: -5.40  {+/- 15.48}  sigmaA: 47.08

magDrop: NA because 0 < A < B is not satisfied

snr: 3.91

D: 1914.00 {+0.52,-0.62} (frame number)
D: [08:35:13.4455]  {+0.0173,-0.0207} seconds

R: 1952.00 {+0.62,-0.52} (frame number)
R: [08:35:14.7134]  {+0.0207,-0.0173} seconds

Duration (R - D): 38.0000 {+0.7950,-0.7950} readings
Duration (R - D): 1.2679 {+0.0265,-0.0265} seconds

=============== end 0.95 containment interval report ===============

================= 0.9973 containment interval report ===============

B: 284.83  {+/- 3.42}  sigmaB: 74.20

A: -5.40  {+/- 23.22}  sigmaA: 47.08

magDrop: NA because 0 < A < B is not satisfied

snr: 3.91

D: 1914.00 {+1.11,-1.20} (frame number)
D: [08:35:13.4455]  {+0.0369,-0.0402} seconds

R: 1952.00 {+1.20,-1.11} (frame number)
R: [08:35:14.7134]  {+0.0402,-0.0369} seconds

Duration (R - D): 38.0000 {+1.5635,-1.5635} readings
Duration (R - D): 1.2679 {+0.0522,-0.0522} seconds

=============== end 0.9973 containment interval report =============

D frame number: 1914.00
D: 0.6800 containment intervals:  {+/- 0.23} (readings)
D: 0.9500 containment intervals:  {+/- 0.62} (readings)
D: 0.9973 containment intervals:  {+/- 1.20} (readings)

R frame number: 1952.00
R: 0.6800 containment intervals:  {+/- 0.23} (readings)
R: 0.9500 containment intervals:  {+/- 0.62} (readings)
R: 0.9973 containment intervals:  {+/- 1.20} (readings)

Duration (R - D): 38.0000 readings
Duration: 0.6800 containment intervals:  {+/- 0.3513} (readings)
Duration: 0.9500 containment intervals:  {+/- 0.7950} (readings)
Duration: 0.9973 containment intervals:  {+/- 1.5635} (readings)

=============== Summary report for Excel file =====================

This light curve has not been block integrated.

This light curve has been normalized against a reference star.

The following lightcurve parameters were utilized:

==== use diff: is checked
==== exp: 0.033367

This 'drop' has a zero probability of being an artifact of noise.
>>>> probability > 0.0000 indicates the 'drop' may be spurious (a noise artifact). Consult with an IOTA Regional Coordinator.
>>>> probability = 0.0000 indicates the 'drop' is unlikely to be a noise artifact, but does not prove that the 'drop' is due to an occultation
>>>> Consider 'drop' shape, timing, mag drop, duration and other positive observer chords before reporting the 'drop' as a positive.

All times are calculated/reported based on the assumption that timestamps are start-of-exposure times.

It is critical that you make appropriate time adjustments when timestamps are NOT start-of-exposure times.
If you use the North American Excel Spreadsheet report, all times will be properly corrected
for camera delay and reported start-of-exposure times.
For other users worldwide, use the appropriate corrections documented in the North American Spreadsheet report form - use
the documentation shown on the Corrections Tables tab.

magDrop: NA because 0 < A < B is not satisfied

snr: 3.91

D time: [08:35:13.4455]
D: 0.6800 containment intervals:  {+/- 0.0078} seconds
D: 0.9500 containment intervals:  {+/- 0.0207} seconds
D: 0.9973 containment intervals:  {+/- 0.0402} seconds

R time: [08:35:14.7134]
R: 0.6800 containment intervals:  {+/- 0.0078} seconds
R: 0.9500 containment intervals:  {+/- 0.0207} seconds
R: 0.9973 containment intervals:  {+/- 0.0402} seconds

Duration (R - D): 1.2679 seconds
Duration: 0.6800 containment intervals:  {+/- 0.0117} seconds
Duration: 0.9500 containment intervals:  {+/- 0.0265} seconds
Duration: 0.9973 containment intervals:  {+/- 0.0522} seconds

Enter D and R error bars for each containment interval in Excel spreadsheet without + or - sign (assumed to be +/-)

=========== end Summary report for Excel file =====================

Solution 'envelope' in the main plot drawn using 0.95 containment interval error bars



#################### Session ended: Mon Feb 20 12:25:28 2023  ####################