#################### PYOTE 5.1.2  session started: Sun Apr  9 22:22:40 2023  ####################

filename: C:\Users\aschw\Desktop\DvtiData\20230409_201041.csv

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

==================== file header lines ====================
# PyMovie Version 3.7.0
# source: C:/Users/aschw/Desktop/DvtiData/20230409_201041_1624x1240_G36dBD_0100ms.adv
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: target
# ____ aperture size: 31
# ____ x,y: (805, 638)
# ____ threshold: 1410
# ____ def mask radius: 3.2
# ____ color: red
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 0
#
# aperture name: ref1
# ____ aperture size: 31
# ____ x,y: (1058, 817)
# ____ threshold: 1504
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# aperture name: ref2
# ____ aperture size: 31
# ____ x,y: (940, 558)
# ____ threshold: 1496
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: True
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 2
#
# date at frame 0: 2023-04-09
#ACQUISITION-DELAY: 0.0
#ALTITUDE: 567.4
#AUTHOR: Andreas SCHWEIZER
#BINNING-X: 1
#BINNING-Y: 1
#CAMERA-DRIVER-NAME: UVC
#CAMERA-FIRMWARE-VERSION: 1.0.3
#CAMERA-MODEL: DVTI+CAM
#CAMERA-SENSOR-INFO: Sony IMX430LLJ-C (1.1" 1624x1240 4.5um CIS)
#CAMERA-SERIAL-NO: 17
#CAMERA-VENDOR-NAME: DVTI
#COMMENT: 
#DEC: -9.129531
#HEIGHT: 1240
#INSTRUMENT: DVTI+CAM #17 FW 1.0.3, Sensor IMX430
#LATITUDE: 47.3418587
#LONGITUDE: 8.4731581
#OBJNAME: (439) Ohio occ. UCAC4 408-057811
#OBSERVER: Andreas SCHWEIZER
#RA: 13.225049
#RECORDER-SOFTWARE: DvtiCamControl
#RECORDER-SOFTWARE-VERSION: 5.6.0-14
#TELESCOPE: Borg 107FL
#WIDTH: 1624
==================== end header lines ====================

No time step irregularities found.

timeDelta: 0.100000 seconds per reading
timestamp error rate: 0.00%

Home directory: C:\Users\aschw\AppData\Local\Packages\PythonSoftwareFoundation.Python.3.10_qbz5n2kfra8p0\LocalCache\local-packages\Python310\site-packages\pyoteapp

We found C:\Users\aschw\Documents\model-examples already present. Adding any new examples ...
D zone selected: [327, 360]

R zone selected: [362, 397]

Locate a "D and R" event has been selected

Number of candidate solutions: 1224 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:11611.03  sigA:6285.70 B:39368.13 A:3730.23
in entryNum units: D: 356  R: 369

noise corr coefs: [1.00, 0.111]  (based on 589 points)  sigmaB: 11456.69

Subframe adjusted solution...
sigB:11611.03  sigA:5323.58 B:39368.13 A:2675.50
in entryNum units: D: 356  R: 368  D(subframe): 356.0000  R(subframe): 368.6449

in frameNum units: D: 356  R: 368  D(subframe): 356.0000  R(subframe): 368.6449

... end New solver results

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

loDbar   @ .68 ci:  -0.2333
hiDbar   @ .68 ci:   0.2677
loDbar   @ .95 ci:  -0.6942
hiDbar   @ .95 ci:   0.5751
loDbar   @ .9973 ci:  -1.6265
hiDbar   @ .9973 ci:   1.2707

loDurBar @ .68 ci:  -0.3900
hiDurBar @ .68 ci:   0.3834
loDurBar @ .95 ci:  -0.9014
hiDurBar @ .95 ci:   0.8879
loDurBar @ .9973 ci:  -1.9068
hiDurBar @ .9973 ci:   1.9044

Timestamp validity check ...

From timestamps at D and R, calculated 12 reading blocks.  From reading blocks, calculated 12 blocks.

Timestamps appear valid @ D and R

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

B: 39368.13  {+/- 478.69}  sigmaB: 11611.03

A: 2675.50  {+/- 1560.04}  sigmaA: 5323.58

magDrop report: percentDrop: 93.2  magDrop: 2.919  +/- 0.633  (0.68 ci)

snr: 3.16

D: 356.00 {+0.27,-0.23} (frame number)
D: [20:11:09.3240]  {+0.0268,-0.0233} seconds

R: 368.64 {+0.23,-0.27} (frame number)
R: [20:11:10.5885]  {+0.0233,-0.0268} seconds

Duration (R - D): 12.6449 {+0.3867,-0.3867} readings
Duration (R - D): 1.2645 {+0.0387,-0.0387} seconds

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

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

B: 39368.13  {+/- 957.37}  sigmaB: 11611.03

A: 2675.50  {+/- 3120.08}  sigmaA: 5323.58

magDrop report: percentDrop: 93.2  magDrop: 2.919  +/- 1.266  (0.95 ci)

snr: 3.16

D: 356.00 {+0.58,-0.69} (frame number)
D: [20:11:09.3240]  {+0.0575,-0.0694} seconds

R: 368.64 {+0.69,-0.58} (frame number)
R: [20:11:10.5885]  {+0.0694,-0.0575} seconds

Duration (R - D): 12.6449 {+0.8947,-0.8947} readings
Duration (R - D): 1.2645 {+0.0895,-0.0895} seconds

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

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

B: 39368.13  {+/- 1436.06}  sigmaB: 11611.03

A: 2675.50  {+/- 4680.13}  sigmaA: 5323.58

magDrop report: percentDrop: 93.2  magDrop: 2.919  +/- 1.900  (0.9973 ci)

snr: 3.16

D: 356.00 {+1.27,-1.63} (frame number)
D: [20:11:09.3240]  {+0.1271,-0.1626} seconds

R: 368.64 {+1.63,-1.27} (frame number)
R: [20:11:10.5885]  {+0.1626,-0.1271} seconds

Duration (R - D): 12.6449 {+1.9056,-1.9056} readings
Duration (R - D): 1.2645 {+0.1906,-0.1906} seconds

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

D frame number: 356.00
D: 0.6800 containment intervals:  {+/- 0.27} (readings)
D: 0.9500 containment intervals:  {+/- 0.69} (readings)
D: 0.9973 containment intervals:  {+/- 1.63} (readings)

R frame number: 368.64
R: 0.6800 containment intervals:  {+/- 0.27} (readings)
R: 0.9500 containment intervals:  {+/- 0.69} (readings)
R: 0.9973 containment intervals:  {+/- 1.63} (readings)

Duration (R - D): 12.6449 readings
Duration: 0.6800 containment intervals:  {+/- 0.3867} (readings)
Duration: 0.9500 containment intervals:  {+/- 0.8947} (readings)
Duration: 0.9973 containment intervals:  {+/- 1.9056} (readings)

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

This light curve has not been block integrated.


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 report: percentDrop: 93.2  magDrop: 2.919  +/- 1.266  (0.95 ci)

snr: 3.16

D time: [20:11:09.3240]
D: 0.6800 containment intervals:  {+/- 0.0268} seconds
D: 0.9500 containment intervals:  {+/- 0.0694} seconds
D: 0.9973 containment intervals:  {+/- 0.1626} seconds

R time: [20:11:10.5885]
R: 0.6800 containment intervals:  {+/- 0.0268} seconds
R: 0.9500 containment intervals:  {+/- 0.0694} seconds
R: 0.9973 containment intervals:  {+/- 0.1626} seconds

Duration (R - D): 1.2645 seconds
Duration: 0.6800 containment intervals:  {+/- 0.0387} seconds
Duration: 0.9500 containment intervals:  {+/- 0.0895} seconds
Duration: 0.9973 containment intervals:  {+/- 0.1906} 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