

#################### PYOTE 4.1.2  session started: Sat Jan  8 00:32:42 2022  ####################

filename: F:/OccvVideos/2022010tolusa/RN-PyM-LC.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 5496 frames

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

==================== file header lines ====================
# PyMovie Version 3.3.0
# source: F:\OccvVideos\2022010tolusa.avi
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: tracking
# ____ aperture size: 51
# ____ x,y: (606, 142)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 0
#
# aperture name: target
# ____ aperture size: 51
# ____ x,y: (299, 154)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: red
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# aperture name: nostar
# ____ aperture size: 51
# ____ x,y: (415, 136)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: green
# ____ joggable: True
# ____ auto textOut: True
# ____ thumbnail source: True
# ____ csv output order: 2
#
==================== end header lines ====================

timeDelta: 0.0333665 seconds per reading
timestamp error rate: 0.0183%

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

There is no curve selected for analysis.

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

Analyze data 2 selected - PyMovie aperture name: target (signal)

D zone selected: [2199, 2430]

R zone selected: [2439, 2559]

Locate a "D and R" event triggered

minEvent: <blank>  maxEvent: <blank>

Number of candidate solutions: 28072 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:57.98  sigA:47.37 B:148.76 A:123.39
in entryNum units: D: 2343  R: 2459

noise corr coefs: [1.00, 0.0620]  (based on 5349 points)  sigmaB: 55.94

Subframe adjusted solution...
sigB:55.94  sigA:47.37 B:148.76 A:122.62
in entryNum units: D: 2344  R: 2460  D(subframe): 2344.0000  R(subframe): 2460.0000

in frameNum units: D: 2374  R: 2490  D(subframe): 2374.0000  R(subframe): 2490.0000

... end New solver results

Error bar report based on 100,000 simulations (units are readings)...

loDbar   @ .68 ci: -12.6983
hiDbar   @ .68 ci:   8.2517
loDbar   @ .95 ci: -43.4528
hiDbar   @ .95 ci:  34.1224
loDbar   @ .9973 ci: -100.7525
hiDbar   @ .9973 ci:  90.4729

loDurBar @ .68 ci: -18.6748
hiDurBar @ .68 ci:  18.6728
loDurBar @ .95 ci: -54.5368
hiDurBar @ .95 ci:  52.8378
loDurBar @ .9973 ci: -115.4479
hiDurBar @ .9973 ci: 118.4182

Timestamp validity check ...

From timestamps at D and R, calculated 116 reading blocks.  From reading blocks, calculated 116 blocks.

Timestamps appear valid @ D and R

================= 0.68 containment interval report =================

B: 148.76  {+/- 0.76}  sigmaB: 55.94

A: 122.62  {+/- 4.42}  sigmaA: 47.37

magDrop: 0.210  +/- 0.040  (0.68 ci)

snr: 0.47

D: 2374.00 {+10.47,-10.47} (frame number)
D: [06:02:48.4996]  {+0.3495,-0.3495} seconds

R: 2490.00 {+10.47,-10.47} (frame number)
R: [06:02:52.3702]  {+0.3495,-0.3495} seconds

Duration (R - D): 116.0000 {+18.6738,-18.6738} readings
Duration (R - D): 3.8706 {+0.6231,-0.6231} seconds

=============== end 0.68 containment interval report ===============

================= 0.95 containment interval report =================

B: 148.76  {+/- 1.53}  sigmaB: 55.94

A: 122.62  {+/- 8.83}  sigmaA: 47.37

magDrop: 0.210  +/- 0.079  (0.95 ci)

snr: 0.47

D: 2374.00 {+38.79,-38.79} (frame number)
D: [06:02:48.4996]  {+1.2942,-1.2942} seconds

R: 2490.00 {+38.79,-38.79} (frame number)
R: [06:02:52.3702]  {+1.2942,-1.2942} seconds

Duration (R - D): 116.0000 {+53.6873,-53.6873} readings
Duration (R - D): 3.8706 {+1.7914,-1.7914} seconds

=============== end 0.95 containment interval report ===============

================= 0.9973 containment interval report ===============

B: 148.76  {+/- 2.29}  sigmaB: 55.94

A: 122.62  {+/- 13.25}  sigmaA: 47.37

magDrop: 0.210  +/- 0.119  (0.9973 ci)

snr: 0.47

D: 2374.00 {+95.61,-95.61} (frame number)
D: [06:02:48.4996]  {+3.1903,-3.1903} seconds

R: 2490.00 {+95.61,-95.61} (frame number)
R: [06:02:52.3702]  {+3.1903,-3.1903} seconds

Duration (R - D): 116.0000 {+116.9330,-116.9330} readings
Duration (R - D): 3.8706 {+3.9016,-3.9016} seconds

=============== end 0.9973 containment interval report =============

D frame number: 2374.00
D: 0.6800 containment intervals:  {+/- 12.70} (readings)
D: 0.9500 containment intervals:  {+/- 43.45} (readings)
D: 0.9973 containment intervals:  {+/- 100.75} (readings)

R frame number: 2490.00
R: 0.6800 containment intervals:  {+/- 12.70} (readings)
R: 0.9500 containment intervals:  {+/- 43.45} (readings)
R: 0.9973 containment intervals:  {+/- 100.75} (readings)

Duration (R - D): 116.0000 readings
Duration: 0.6800 containment intervals:  {+/- 18.6738} (readings)
Duration: 0.9500 containment intervals:  {+/- 53.6873} (readings)
Duration: 0.9973 containment intervals:  {+/- 116.9330} (readings)

=============== Summary report for Excel file =====================

This light curve has not been block integrated.

The following lightcurve parameters were utilized:

==== use diff: is checked
==== exp: 0.033367

This 'drop' has a 0.0011 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: 0.210  +/- 0.079  (0.95 ci)

snr: 0.47

D time: [06:02:48.4996]
D: 0.6800 containment intervals:  {+/- 0.4237} seconds
D: 0.9500 containment intervals:  {+/- 1.4499} seconds
D: 0.9973 containment intervals:  {+/- 3.3618} seconds

R time: [06:02:52.3702]
R: 0.6800 containment intervals:  {+/- 0.4237} seconds
R: 0.9500 containment intervals:  {+/- 1.4499} seconds
R: 0.9973 containment intervals:  {+/- 3.3618} seconds

Duration (R - D): 3.8706 seconds
Duration: 0.6800 containment intervals:  {+/- 0.6231} seconds
Duration: 0.9500 containment intervals:  {+/- 1.7914} seconds
Duration: 0.9973 containment intervals:  {+/- 3.9016} 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

Secondary reference 1 selected - PyMovie aperture name: tracking (signal)

******************** starting over ********************



#################### PYOTE 4.1.2  session started: Sat Jan  8 00:41:51 2022  ####################

filename: F:/OccvVideos/2022010tolusa/RN-PyM-LC.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 5496 frames

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

==================== file header lines ====================
# PyMovie Version 3.3.0
# source: F:\OccvVideos\2022010tolusa.avi
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: tracking
# ____ aperture size: 51
# ____ x,y: (606, 142)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 0
#
# aperture name: target
# ____ aperture size: 51
# ____ x,y: (299, 154)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: red
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# aperture name: nostar
# ____ aperture size: 51
# ____ x,y: (415, 136)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: green
# ____ joggable: True
# ____ auto textOut: True
# ____ thumbnail source: True
# ____ csv output order: 2
#
==================== end header lines ====================

timeDelta: 0.0333665 seconds per reading
timestamp error rate: 0.0183%

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

There is no secondary reference selected.

Secondary reference 1 selected - PyMovie aperture name: tracking (signal)

There is no curve selected for analysis.

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

Analyze data 2 selected - PyMovie aperture name: target (signal)

Data trimmed/selected using points: [16, 5449]

Smoothing of secondary star light curve performed with window size: 33

******************** starting over ********************

******************** starting over ********************

Data trimmed/selected using points: [16, 5449]

Smoothing of secondary star light curve performed with window size: 33

Light curve normalized to secondary around point 2531

D zone selected: [2164, 2374]

R zone selected: [2408, 2645]

Locate a "D and R" event triggered

minEvent: <blank>  maxEvent: <blank>

Number of candidate solutions: 50218 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:56.98  sigA:47.21 B:145.37 A:121.34
in entryNum units: D: 2346  R: 2459

noise corr coefs: [1.00, 0.0660]  (based on 5320 points)  sigmaB: 54.74

Subframe adjusted solution...
sigB:54.74  sigA:47.21 B:145.36 A:120.50
in entryNum units: D: 2346  R: 2460  D(subframe): 2346.0000  R(subframe): 2460.0000

in frameNum units: D: 2376  R: 2490  D(subframe): 2376.0000  R(subframe): 2490.0000

... end New solver results

Error bar report based on 100,000 simulations (units are readings)...

loDbar   @ .68 ci: -13.6843
hiDbar   @ .68 ci:   9.6969
loDbar   @ .95 ci: -45.9959
hiDbar   @ .95 ci:  41.0419
loDbar   @ .9973 ci: -104.5118
hiDbar   @ .9973 ci: 112.2247

loDurBar @ .68 ci: -20.0862
hiDurBar @ .68 ci:  21.6370
loDurBar @ .95 ci: -62.1459
hiDurBar @ .95 ci:  60.3158
loDurBar @ .9973 ci: -134.0691
hiDurBar @ .9973 ci: 131.8968

Timestamp validity check ...

From timestamps at D and R, calculated 114 reading blocks.  From reading blocks, calculated 114 blocks.

Timestamps appear valid @ D and R

================= 0.68 containment interval report =================

B: 145.36  {+/- 0.75}  sigmaB: 54.74

A: 120.50  {+/- 4.44}  sigmaA: 47.21

magDrop: 0.204  +/- 0.040  (0.68 ci)

snr: 0.45

D: 2376.00 {+11.69,-11.69} (frame number)
D: [06:02:48.5664]  {+0.3901,-0.3901} seconds

R: 2490.00 {+11.69,-11.69} (frame number)
R: [06:02:52.3702]  {+0.3901,-0.3901} seconds

Duration (R - D): 114.0000 {+20.8616,-20.8616} readings
Duration (R - D): 3.8038 {+0.6961,-0.6961} seconds

=============== end 0.68 containment interval report ===============

================= 0.95 containment interval report =================

B: 145.36  {+/- 1.50}  sigmaB: 54.74

A: 120.50  {+/- 8.88}  sigmaA: 47.21

magDrop: 0.204  +/- 0.081  (0.95 ci)

snr: 0.45

D: 2376.00 {+43.52,-43.52} (frame number)
D: [06:02:48.5664]  {+1.4521,-1.4521} seconds

R: 2490.00 {+43.52,-43.52} (frame number)
R: [06:02:52.3702]  {+1.4521,-1.4521} seconds

Duration (R - D): 114.0000 {+61.2309,-61.2309} readings
Duration (R - D): 3.8038 {+2.0431,-2.0431} seconds

=============== end 0.95 containment interval report ===============

================= 0.9973 containment interval report ===============

B: 145.36  {+/- 2.25}  sigmaB: 54.74

A: 120.50  {+/- 13.32}  sigmaA: 47.21

magDrop: 0.204  +/- 0.121  (0.9973 ci)

snr: 0.45

D: 2376.00 {+108.37,-108.37} (frame number)
D: [06:02:48.5664]  {+3.6159,-3.6159} seconds

R: 2490.00 {+108.37,-108.37} (frame number)
R: [06:02:52.3702]  {+3.6159,-3.6159} seconds

Duration (R - D): 114.0000 {+132.9830,-132.9830} readings
Duration (R - D): 3.8038 {+4.4372,-4.4372} seconds

=============== end 0.9973 containment interval report =============

D frame number: 2376.00
D: 0.6800 containment intervals:  {+/- 13.68} (readings)
D: 0.9500 containment intervals:  {+/- 46.00} (readings)
D: 0.9973 containment intervals:  {+/- 112.22} (readings)

R frame number: 2490.00
R: 0.6800 containment intervals:  {+/- 13.68} (readings)
R: 0.9500 containment intervals:  {+/- 46.00} (readings)
R: 0.9973 containment intervals:  {+/- 112.22} (readings)

Duration (R - D): 114.0000 readings
Duration: 0.6800 containment intervals:  {+/- 20.8616} (readings)
Duration: 0.9500 containment intervals:  {+/- 61.2309} (readings)
Duration: 0.9973 containment intervals:  {+/- 132.9830} (readings)

=============== Summary report for Excel file =====================

This light curve has not been block integrated.
This light curve has been normalized against a reference star.
This light curve has been trimmed.

The following lightcurve parameters were utilized:

==== use diff: is checked
==== exp: 0.033367

This 'drop' has a 0.0027 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: 0.204  +/- 0.081  (0.95 ci)

snr: 0.45

D time: [06:02:48.5664]
D: 0.6800 containment intervals:  {+/- 0.4566} seconds
D: 0.9500 containment intervals:  {+/- 1.5347} seconds
D: 0.9973 containment intervals:  {+/- 3.7445} seconds

R time: [06:02:52.3702]
R: 0.6800 containment intervals:  {+/- 0.4566} seconds
R: 0.9500 containment intervals:  {+/- 1.5347} seconds
R: 0.9973 containment intervals:  {+/- 3.7445} seconds

Duration (R - D): 3.8038 seconds
Duration: 0.6800 containment intervals:  {+/- 0.6961} seconds
Duration: 0.9500 containment intervals:  {+/- 2.0431} seconds
Duration: 0.9973 containment intervals:  {+/- 4.4372} 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

******************** starting over ********************



#################### PYOTE 4.1.2  session started: Sat Jan  8 00:57:31 2022  ####################

filename: F:/OccvVideos/2022010tolusa/RN-PyM-LC.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 5496 frames

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

==================== file header lines ====================
# PyMovie Version 3.3.0
# source: F:\OccvVideos\2022010tolusa.avi
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: tracking
# ____ aperture size: 51
# ____ x,y: (606, 142)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 0
#
# aperture name: target
# ____ aperture size: 51
# ____ x,y: (299, 154)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: red
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# aperture name: nostar
# ____ aperture size: 51
# ____ x,y: (415, 136)
# ____ threshold: 8
# ____ def mask radius: 3.2
# ____ color: green
# ____ joggable: True
# ____ auto textOut: True
# ____ thumbnail source: True
# ____ csv output order: 2
#
==================== end header lines ====================

timeDelta: 0.0333665 seconds per reading
timestamp error rate: 0.0183%

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

There is no curve selected for analysis.

Analyze data 1 selected - PyMovie aperture name: tracking (signal)

Analyze data 2 selected - PyMovie aperture name: target (signal)

Secondary reference 2 selected - PyMovie aperture name: target (signal)

Secondary reference 1 selected - PyMovie aperture name: tracking (signal)

Data trimmed/selected using points: [16, 5449]

Smoothing of secondary star light curve performed with window size: 33

Data trimmed/selected using points: [65, 5400]

Smoothing of secondary star light curve performed with window size: 99

Light curve normalized to secondary around point 1826

D zone selected: [2236, 2414]

R zone selected: [2420, 2614]

Locate a "D and R" event triggered

minEvent: <blank>  maxEvent: <blank>

Number of candidate solutions: 34905 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:58.46  sigA:48.43 B:149.92 A:124.90
in entryNum units: D: 2346  R: 2459

noise corr coefs: [1.00, 0.0664]  (based on 5222 points)  sigmaB: 56.05

Subframe adjusted solution...
sigB:56.05  sigA:48.43 B:149.90 A:124.02
in entryNum units: D: 2346  R: 2460  D(subframe): 2346.0000  R(subframe): 2460.0000

in frameNum units: D: 2376  R: 2490  D(subframe): 2376.0000  R(subframe): 2490.0000

... end New solver results

Error bar report based on 100,000 simulations (units are readings)...

loDbar   @ .68 ci: -13.4952
hiDbar   @ .68 ci:   9.4364
loDbar   @ .95 ci: -46.7275
hiDbar   @ .95 ci:  38.2532
loDbar   @ .9973 ci: -111.7832
hiDbar   @ .9973 ci: 101.0988

loDurBar @ .68 ci: -19.4792
hiDurBar @ .68 ci:  21.1575
loDurBar @ .95 ci: -60.4998
hiDurBar @ .95 ci:  59.1821
loDurBar @ .9973 ci: -130.9622
hiDurBar @ .9973 ci: 126.4286

Timestamp validity check ...

From timestamps at D and R, calculated 114 reading blocks.  From reading blocks, calculated 114 blocks.

Timestamps appear valid @ D and R

================= 0.68 containment interval report =================

B: 149.90  {+/- 0.78}  sigmaB: 56.05

A: 124.02  {+/- 4.56}  sigmaA: 48.43

magDrop: 0.206  +/- 0.040  (0.68 ci)

snr: 0.46

D: 2376.00 {+11.47,-11.47} (frame number)
D: [06:02:48.5664]  {+0.3826,-0.3826} seconds

R: 2490.00 {+11.47,-11.47} (frame number)
R: [06:02:52.3702]  {+0.3826,-0.3826} seconds

Duration (R - D): 114.0000 {+20.3184,-20.3184} readings
Duration (R - D): 3.8038 {+0.6780,-0.6780} seconds

=============== end 0.68 containment interval report ===============

================= 0.95 containment interval report =================

B: 149.90  {+/- 1.55}  sigmaB: 56.05

A: 124.02  {+/- 9.11}  sigmaA: 48.43

magDrop: 0.206  +/- 0.081  (0.95 ci)

snr: 0.46

D: 2376.00 {+42.49,-42.49} (frame number)
D: [06:02:48.5664]  {+1.4178,-1.4178} seconds

R: 2490.00 {+42.49,-42.49} (frame number)
R: [06:02:52.3702]  {+1.4178,-1.4178} seconds

Duration (R - D): 114.0000 {+59.8409,-59.8409} readings
Duration (R - D): 3.8038 {+1.9967,-1.9967} seconds

=============== end 0.95 containment interval report ===============

================= 0.9973 containment interval report ===============

B: 149.90  {+/- 2.33}  sigmaB: 56.05

A: 124.02  {+/- 13.67}  sigmaA: 48.43

magDrop: 0.206  +/- 0.121  (0.9973 ci)

snr: 0.46

D: 2376.00 {+106.44,-106.44} (frame number)
D: [06:02:48.5664]  {+3.5516,-3.5516} seconds

R: 2490.00 {+106.44,-106.44} (frame number)
R: [06:02:52.3702]  {+3.5516,-3.5516} seconds

Duration (R - D): 114.0000 {+128.6954,-128.6954} readings
Duration (R - D): 3.8038 {+4.2941,-4.2941} seconds

=============== end 0.9973 containment interval report =============

D frame number: 2376.00
D: 0.6800 containment intervals:  {+/- 13.50} (readings)
D: 0.9500 containment intervals:  {+/- 46.73} (readings)
D: 0.9973 containment intervals:  {+/- 111.78} (readings)

R frame number: 2490.00
R: 0.6800 containment intervals:  {+/- 13.50} (readings)
R: 0.9500 containment intervals:  {+/- 46.73} (readings)
R: 0.9973 containment intervals:  {+/- 111.78} (readings)

Duration (R - D): 114.0000 readings
Duration: 0.6800 containment intervals:  {+/- 20.3184} (readings)
Duration: 0.9500 containment intervals:  {+/- 59.8409} (readings)
Duration: 0.9973 containment intervals:  {+/- 128.6954} (readings)

=============== Summary report for Excel file =====================

This light curve has not been block integrated.
This light curve has been normalized against a reference star.
This light curve has been trimmed.

The following lightcurve parameters were utilized:

==== use diff: is checked
==== exp: 0.033367

This 'drop' has a 0.0018 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: 0.206  +/- 0.081  (0.95 ci)

snr: 0.46

D time: [06:02:48.5664]
D: 0.6800 containment intervals:  {+/- 0.4503} seconds
D: 0.9500 containment intervals:  {+/- 1.5591} seconds
D: 0.9973 containment intervals:  {+/- 3.7298} seconds

R time: [06:02:52.3702]
R: 0.6800 containment intervals:  {+/- 0.4503} seconds
R: 0.9500 containment intervals:  {+/- 1.5591} seconds
R: 0.9973 containment intervals:  {+/- 3.7298} seconds

Duration (R - D): 3.8038 seconds
Duration: 0.6800 containment intervals:  {+/- 0.6780} seconds
Duration: 0.9500 containment intervals:  {+/- 1.9967} seconds
Duration: 0.9973 containment intervals:  {+/- 4.2941} 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

