#################### PYOTE 5.1.0  session started: Tue Dec 24 14:56:28 2024  ####################

filename: \\bequiet\DATA\DATI\OCCULTAZIONI\Capture 2024-12-23T21_14_54Z\Bertholda_Gnosca_dynamic_mask.csv

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

==================== file header lines ====================
# PyMovie Version 4.0.5
# source: //bequiet/DATA/DATI/OCCULTAZIONI/Capture 2024-12-23T21_14_54Z.adv
#
# Aperture photometry was used to extract the lightcurves
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: target
# ____ aperture size: 31
# ____ x,y: (258, 148) at frame 700
# ____ threshold: 3924
# ____ def mask radius: 3.2
# ____ color: green
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 0
#
# aperture name: ref
# ____ aperture size: 31
# ____ x,y: (397, 153) at frame 700
# ____ threshold: 3740
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: True
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# date at frame 0: 2024-12-23
#ADV-VERSION: 2
#ADVLIB-VERSION: 2.0
#ALTITUDE: 0
#BINNING-X: 2
#BINNING-Y: 2
#BITPIX: 16
#CAMERA-MODEL: QHY174M
#CAMERA-SENSOR-INFO: ADC bit depth : 12
#EFFECTIVE-PIXEL-SIZE-X: 11.720000267028809
#EFFECTIVE-PIXEL-SIZE-Y: 11.720000267028809
#FSTF-TYPE: ADV
#HEIGHT: 300
#LATITUDE: 46.2314505
#LONGITUDE: 9.024086666666667
#POSITION-REFERENCE: WGS84
#RECORDER-SOFTWARE: SharpCap
#RECORDER-SOFTWARE-VERSION: 4.1.9418.0
#WIDTH: 480
#TIME-SOURCE: Camera GPS
#
# Aperture photometry was used to extract the lightcurves
==================== end header lines ====================

No time step irregularities found.

timeDelta: 0.400150 seconds per reading
timestamp error rate: 0.00%

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

We found C:\Users\stefa\Documents\model-examples already present. Adding any new examples ...
D zone selected: [126, 132]

R zone selected: [146, 159]

Locate a "D and R" event has been selected

Number of candidate solutions: 98 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:115613.15  sigA:104819.24 B:808969.58 A:274988.27
in entryNum units: D: 130  R: 152

noise corr coefs: [1.00, 0.334, 0.200]  (based on 279 points)  sigmaB: 104858.98

Subframe adjusted solution...
sigB:115286.42  sigA:104819.24 B:809634.96 A:274988.27
in entryNum units: D: 130  R: 152  D(subframe): 130.0000  R(subframe): 152.3464

in frameNum units: D: 530  R: 552  D(subframe): 530.0000  R(subframe): 552.3464

... end New solver results

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

loDbar   @ .68 ci:  -0.2319
hiDbar   @ .68 ci:   0.2316
loDbar   @ .95 ci:  -0.5854
hiDbar   @ .95 ci:   0.5561
loDbar   @ .9973 ci:  -1.2596
hiDbar   @ .9973 ci:   1.2444

loDurBar @ .68 ci:  -0.3440
hiDurBar @ .68 ci:   0.3582
loDurBar @ .95 ci:  -0.8004
hiDurBar @ .95 ci:   0.7872
loDurBar @ .9973 ci:  -1.8378
hiDurBar @ .9973 ci:   1.8635

Timestamp validity check ...

From timestamps at D and R, calculated 22 reading blocks.  From reading blocks, calculated 22 blocks.

Timestamps appear valid @ D and R

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

B: 809634.96  {+/- 6918.73}  sigmaB: 115286.42

A: 274988.27  {+/- 22687.08}  sigmaA: 104819.24

magDrop report: percentDrop: 66.0  magDrop: 1.172  +/- 0.090  (0.68 ci)

snr: 4.64

D: 530.00 {+0.23,-0.23} (frame number)
D: [21:18:05.2256]  {+0.0927,-0.0927} seconds

R: 552.35 {+0.23,-0.23} (frame number)
R: [21:18:14.1676]  {+0.0927,-0.0927} seconds

Duration (R - D): 22.3464 {+0.3511,-0.3511} readings
Duration (R - D): 8.9420 {+0.1405,-0.1405} seconds

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

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

B: 809634.96  {+/- 13837.46}  sigmaB: 115286.42

A: 274988.27  {+/- 45374.17}  sigmaA: 104819.24

magDrop report: percentDrop: 66.0  magDrop: 1.172  +/- 0.180  (0.95 ci)

snr: 4.64

D: 530.00 {+0.57,-0.57} (frame number)
D: [21:18:05.2256]  {+0.2284,-0.2284} seconds

R: 552.35 {+0.57,-0.57} (frame number)
R: [21:18:14.1676]  {+0.2284,-0.2284} seconds

Duration (R - D): 22.3464 {+0.7938,-0.7938} readings
Duration (R - D): 8.9420 {+0.3176,-0.3176} seconds

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

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

B: 809634.96  {+/- 20756.20}  sigmaB: 115286.42

A: 274988.27  {+/- 68061.25}  sigmaA: 104819.24

magDrop report: percentDrop: 66.0  magDrop: 1.172  +/- 0.270  (0.9973 ci)

snr: 4.64

D: 530.00 {+1.25,-1.25} (frame number)
D: [21:18:05.2256]  {+0.5010,-0.5010} seconds

R: 552.35 {+1.25,-1.25} (frame number)
R: [21:18:14.1676]  {+0.5010,-0.5010} seconds

Duration (R - D): 22.3464 {+1.8507,-1.8507} readings
Duration (R - D): 8.9420 {+0.7405,-0.7405} seconds

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

D frame number: 530.00
D: 0.6800 containment intervals:  {+/- 0.23} (readings)
D: 0.9500 containment intervals:  {+/- 0.59} (readings)
D: 0.9973 containment intervals:  {+/- 1.26} (readings)

R frame number: 552.35
R: 0.6800 containment intervals:  {+/- 0.23} (readings)
R: 0.9500 containment intervals:  {+/- 0.59} (readings)
R: 0.9973 containment intervals:  {+/- 1.26} (readings)

Duration (R - D): 22.3464 readings
Duration: 0.6800 containment intervals:  {+/- 0.3511} (readings)
Duration: 0.9500 containment intervals:  {+/- 0.7938} (readings)
Duration: 0.9973 containment intervals:  {+/- 1.8507} (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: 66.0  magDrop: 1.172  +/- 0.180  (0.95 ci)

snr: 4.64

D time: [21:18:05.2256]
D: 0.6800 containment intervals:  {+/- 0.0927} seconds
D: 0.9500 containment intervals:  {+/- 0.2284} seconds
D: 0.9973 containment intervals:  {+/- 0.5010} seconds

R time: [21:18:14.1676]
R: 0.6800 containment intervals:  {+/- 0.0927} seconds
R: 0.9500 containment intervals:  {+/- 0.2284} seconds
R: 0.9973 containment intervals:  {+/- 0.5010} seconds

Duration (R - D): 8.9420 seconds
Duration: 0.6800 containment intervals:  {+/- 0.1405} seconds
Duration: 0.9500 containment intervals:  {+/- 0.3176} seconds
Duration: 0.9973 containment intervals:  {+/- 0.7405} 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: Tue Dec 24 14:59:38 2024  ####################