#################### PYOTE 5.1.0  session started: Sun Nov  3 16:07:25 2024  ####################

filename: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2024_11_02_(501) Urhixidur\Capture 2024-11-02T19_25_53Z\501_con pyote.csv

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

==================== file header lines ====================
# PyMovie Version 4.0.5
# source: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2024_11_02_(501) Urhixidur\Capture 2024-11-02T19_25_53Z.adv
#
# Aperture photometry was used to extract the lightcurves
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: target
# ____ aperture size: 31
# ____ x,y: (217, 129) at frame 1219
# ____ threshold: 1729
# ____ def mask radius: 3.2
# ____ color: green
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 0
#
# aperture name: reference
# ____ aperture size: 31
# ____ x,y: (310, 130) at frame 1219
# ____ threshold: 1614
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: True
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# date at frame 0: 2024-11-02
#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: 46.23141783333333
#LONGITUDE: 9.024031666666666
#POSITION-REFERENCE: WGS84
#RECORDER-SOFTWARE: SharpCap
#RECORDER-SOFTWARE-VERSION: 4.1.12196.0
#WIDTH: 480
#TIME-SOURCE: Camera GPS
#
# Aperture photometry was used to extract the lightcurves
==================== end header lines ====================

No time step irregularities found.

timeDelta: 0.500141 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 ...
Use min/max event to locate a "D and R" event has been selected

minEvent: 5  maxEvent: 50

Number of candidate solutions: 54809 (using event min/max entries)

New solver results...

Integer (non-subframe) solution...
sigB:14777.60  sigA:11971.85 B:164168.89 A:127225.65
in entryNum units: D: 580  R: 600

noise corr coefs: [1.00, 0.0599]  (based on 1200 points)  sigmaB: 14712.75

Subframe adjusted solution...
sigB:14712.75  sigA:11873.76 B:164168.89 A:127225.65
in entryNum units: D: 580  R: 600  D(subframe): 580.0000  R(subframe): 600.0000

in frameNum units: D: 580  R: 600  D(subframe): 580.0000  R(subframe): 600.0000

... end New solver results

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

loDbar   @ .68 ci:  -0.4385
hiDbar   @ .68 ci:   0.4638
loDbar   @ .95 ci:  -1.4822
hiDbar   @ .95 ci:   1.3334
loDbar   @ .9973 ci:  -3.9235
hiDbar   @ .9973 ci:   3.7950

loDurBar @ .68 ci:  -0.7463
hiDurBar @ .68 ci:   0.7232
loDurBar @ .95 ci:  -2.0414
hiDurBar @ .95 ci:   2.1404
loDurBar @ .9973 ci:  -4.7657
hiDurBar @ .9973 ci:   4.6716

Timestamp validity check ...

From timestamps at D and R, calculated 20 reading blocks.  From reading blocks, calculated 20 blocks.

Timestamps appear valid @ D and R

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

B: 164168.89  {+/- 424.90}  sigmaB: 14712.75

A: 127225.65  {+/- 2724.03}  sigmaA: 11873.76

magDrop report: percentDrop: 22.5  magDrop: 0.277  +/- 0.023  (0.68 ci)

snr: 2.51

D: 580.00 {+0.45,-0.45} (frame number)
D: [19:30:42.9276]  {+0.2256,-0.2256} seconds

R: 600.00 {+0.45,-0.45} (frame number)
R: [19:30:52.9305]  {+0.2256,-0.2256} seconds

Duration (R - D): 20.0000 {+0.7347,-0.7347} readings
Duration (R - D): 10.0029 {+0.3675,-0.3675} seconds

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

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

B: 164168.89  {+/- 849.80}  sigmaB: 14712.75

A: 127225.65  {+/- 5448.06}  sigmaA: 11873.76

magDrop report: percentDrop: 22.5  magDrop: 0.277  +/- 0.047  (0.95 ci)

snr: 2.51

D: 580.00 {+1.41,-1.41} (frame number)
D: [19:30:42.9276]  {+0.7041,-0.7041} seconds

R: 600.00 {+1.41,-1.41} (frame number)
R: [19:30:52.9305]  {+0.7041,-0.7041} seconds

Duration (R - D): 20.0000 {+2.0909,-2.0909} readings
Duration (R - D): 10.0029 {+1.0458,-1.0458} seconds

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

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

B: 164168.89  {+/- 1274.69}  sigmaB: 14712.75

A: 127225.65  {+/- 8172.08}  sigmaA: 11873.76

magDrop report: percentDrop: 22.5  magDrop: 0.277  +/- 0.070  (0.9973 ci)

snr: 2.51

D: 580.00 {+3.86,-3.86} (frame number)
D: [19:30:42.9276]  {+1.9302,-1.9302} seconds

R: 600.00 {+3.86,-3.86} (frame number)
R: [19:30:52.9305]  {+1.9302,-1.9302} seconds

Duration (R - D): 20.0000 {+4.7187,-4.7187} readings
Duration (R - D): 10.0029 {+2.3600,-2.3600} seconds

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

D frame number: 580.00
D: 0.6800 containment intervals:  {+/- 0.46} (readings)
D: 0.9500 containment intervals:  {+/- 1.48} (readings)
D: 0.9973 containment intervals:  {+/- 3.92} (readings)

R frame number: 600.00
R: 0.6800 containment intervals:  {+/- 0.46} (readings)
R: 0.9500 containment intervals:  {+/- 1.48} (readings)
R: 0.9973 containment intervals:  {+/- 3.92} (readings)

Duration (R - D): 20.0000 readings
Duration: 0.6800 containment intervals:  {+/- 0.7347} (readings)
Duration: 0.9500 containment intervals:  {+/- 2.0909} (readings)
Duration: 0.9973 containment intervals:  {+/- 4.7187} (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: 22.5  magDrop: 0.277  +/- 0.047  (0.95 ci)

snr: 2.51

D time: [19:30:42.9276]
D: 0.6800 containment intervals:  {+/- 0.2256} seconds
D: 0.9500 containment intervals:  {+/- 0.7041} seconds
D: 0.9973 containment intervals:  {+/- 1.9302} seconds

R time: [19:30:52.9305]
R: 0.6800 containment intervals:  {+/- 0.2256} seconds
R: 0.9500 containment intervals:  {+/- 0.7041} seconds
R: 0.9973 containment intervals:  {+/- 1.9302} seconds

Duration (R - D): 10.0029 seconds
Duration: 0.6800 containment intervals:  {+/- 0.3675} seconds
Duration: 0.9500 containment intervals:  {+/- 1.0458} seconds
Duration: 0.9973 containment intervals:  {+/- 2.3600} 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