#################### PYOTE 5.1.2  session started: Sun May 19 23:11:26 2024  ####################

filename: C:\Users\aschw\Desktop\DvtiData\20240519_210246_816x620_G33dBD_150.0ms\wet.csv

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

==================== file header lines ====================
# PyMovie Version 4.0.6
# source: C:\Users\aschw\Desktop\DvtiData\20240519_210246_816x620_G33dBD_150.0ms.adv
#
# Aperture photometry was used to extract the lightcurves
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: target
# ____ aperture size: 21
# ____ x,y: (504, 209) at frame 399
# ____ threshold: 1094
# ____ def mask radius: 3.2
# ____ color: red
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# aperture name: ref
# ____ aperture size: 21
# ____ x,y: (466, 225) at frame 399
# ____ threshold: 1092
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: True
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 2
#
# date at frame 0: 2024-05-19
#ACQUISITION-DELAY: 0.0
#ALTITUDE: 588.3
#AUTHOR: Andreas SCHWEIZER
#BINNING-X: 2
#BINNING-Y: 2
#CAMERA-DRIVER-NAME: UVC
#CAMERA-FIRMWARE-VERSION: 1.2.0
#CAMERA-MODEL: DVTI+CAM
#CAMERA-SENSOR-INFO: Sony IMX430LLJ-C (1.1" 1624x1240 4.5um CIS)
#CAMERA-SERIAL-NO: 13
#CAMERA-VENDOR-NAME: DVTI
#COMMENT: 
#DEC: 16.875039
#HEIGHT: 620
#INSTRUMENT: DVTI+CAM #13 FW 1.2.0, Sensor IMX430
#LATITUDE: 47.3418345
#LONGITUDE: 8.4728353
#OBJNAME: (12658) Peiraios occ. UCAC4 534-048547
#OBSERVER: Andreas SCHWEIZER
#RA: 9.309728
#RECORDER-SOFTWARE: DvtiCamControl
#RECORDER-SOFTWARE-VERSION: 5.8.1-49
#TELESCOPE: 25cm Boren Simon
#WIDTH: 816
#
# Aperture photometry was used to extract the lightcurves
==================== end header lines ====================

No time step irregularities found.

timeDelta: 0.150000 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: [176, 197]

R zone selected: [199, 220]

Locate a "D and R" event has been selected

Number of candidate solutions: 484 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:3690.97  sigA:3211.63 B:11509.86 A:2739.56
in entryNum units: D: 194  R: 203

noise corr coefs: [1.00]  (based on 391 points)  sigmaB: 3671.70

Subframe adjusted solution...
sigB:3671.70  sigA:3671.70 B:11509.86 A:2739.56
in entryNum units: D: 194  R: 203  D(subframe): 194.0000  R(subframe): 203.0000

in frameNum units: D: 194  R: 203  D(subframe): 194.0000  R(subframe): 203.0000

... end New solver results

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

loDbar   @ .68 ci:  -0.5543
hiDbar   @ .68 ci:   0.5648
loDbar   @ .95 ci:  -1.9032
hiDbar   @ .95 ci:   1.9579
loDbar   @ .9973 ci:  -4.7826
hiDbar   @ .9973 ci:   5.2289

loDurBar @ .68 ci:  -0.9577
hiDurBar @ .68 ci:   0.9258
loDurBar @ .95 ci:  -2.6747
hiDurBar @ .95 ci:   2.7680
loDurBar @ .9973 ci:  -6.0259
hiDurBar @ .9973 ci:   5.9339

Timestamp validity check ...

From timestamps at D and R, calculated 9 reading blocks.  From reading blocks, calculated 9 blocks.

Timestamps appear valid @ D and R

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

B: 11509.86  {+/- 185.92}  sigmaB: 3671.70

A: 2739.56  {+/- 1298.14}  sigmaA: 3671.70

magDrop report: percentDrop: 76.2  magDrop: 1.558  +/- 0.515  (0.68 ci)

snr: 2.39

D: 194.00 {+0.56,-0.56} (frame number)
D: [21:03:15.2990]  {+0.0839,-0.0839} seconds

R: 203.00 {+0.56,-0.56} (frame number)
R: [21:03:16.6490]  {+0.0839,-0.0839} seconds

Duration (R - D): 9.0000 {+0.9417,-0.9417} readings
Duration (R - D): 1.3500 {+0.1413,-0.1413} seconds

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

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

B: 11509.86  {+/- 371.85}  sigmaB: 3671.70

A: 2739.56  {+/- 2596.28}  sigmaA: 3671.70

magDrop report: percentDrop: 76.2  magDrop: 1.558  +/- 1.030  (0.95 ci)

snr: 2.39

D: 194.00 {+1.93,-1.93} (frame number)
D: [21:03:15.2990]  {+0.2896,-0.2896} seconds

R: 203.00 {+1.93,-1.93} (frame number)
R: [21:03:16.6490]  {+0.2896,-0.2896} seconds

Duration (R - D): 9.0000 {+2.7214,-2.7214} readings
Duration (R - D): 1.3500 {+0.4082,-0.4082} seconds

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

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

B: 11509.86  {+/- 557.77}  sigmaB: 3671.70

A: 2739.56  {+/- 3894.42}  sigmaA: 3671.70

magDrop report: percentDrop: 76.2  magDrop: 1.558  +/- 1.544  (0.9973 ci)

snr: 2.39

D: 194.00 {+5.01,-5.01} (frame number)
D: [21:03:15.2990]  {+0.7509,-0.7509} seconds

R: 203.00 {+5.01,-5.01} (frame number)
R: [21:03:16.6490]  {+0.7509,-0.7509} seconds

Duration (R - D): 9.0000 {+5.9799,-5.9799} readings
Duration (R - D): 1.3500 {+0.8970,-0.8970} seconds

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

D frame number: 194.00
D: 0.6800 containment intervals:  {+/- 0.56} (readings)
D: 0.9500 containment intervals:  {+/- 1.96} (readings)
D: 0.9973 containment intervals:  {+/- 5.23} (readings)

R frame number: 203.00
R: 0.6800 containment intervals:  {+/- 0.56} (readings)
R: 0.9500 containment intervals:  {+/- 1.96} (readings)
R: 0.9973 containment intervals:  {+/- 5.23} (readings)

Duration (R - D): 9.0000 readings
Duration: 0.6800 containment intervals:  {+/- 0.9417} (readings)
Duration: 0.9500 containment intervals:  {+/- 2.7214} (readings)
Duration: 0.9973 containment intervals:  {+/- 5.9799} (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: 76.2  magDrop: 1.558  +/- 1.030  (0.95 ci)

snr: 2.39

D time: [21:03:15.2990]
D: 0.6800 containment intervals:  {+/- 0.0839} seconds
D: 0.9500 containment intervals:  {+/- 0.2896} seconds
D: 0.9973 containment intervals:  {+/- 0.7509} seconds

R time: [21:03:16.6490]
R: 0.6800 containment intervals:  {+/- 0.0839} seconds
R: 0.9500 containment intervals:  {+/- 0.2896} seconds
R: 0.9973 containment intervals:  {+/- 0.7509} seconds

Duration (R - D): 1.3500 seconds
Duration: 0.6800 containment intervals:  {+/- 0.1413} seconds
Duration: 0.9500 containment intervals:  {+/- 0.4082} seconds
Duration: 0.9973 containment intervals:  {+/- 0.8970} 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