#################### PYOTE 5.1.0  session started: Sun Dec  1 09:24:13 2024  ####################

filename: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2024_11_29_(368) Haidea\Capture 2024-11-29T21_43_29Z\1 dynamic.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_29_(368) Haidea\Capture 2024-11-29T21_43_29Z.adv
#
# Aperture photometry was used to extract the lightcurves
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: target
# ____ aperture size: 31
# ____ x,y: (280, 193) at frame 924
# ____ threshold: 3845
# ____ def mask radius: 3.2
# ____ color: green
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 2
#
# aperture name: ref
# ____ aperture size: 31
# ____ x,y: (178, 195) at frame 924
# ____ threshold: 4010
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: True
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 3
#
# date at frame 0: 2024-11-29
#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: 46.231427
#LONGITUDE: 9.024058333333333
#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 ...
Use min/max event to locate a "D and R" event has been selected

minEvent: 10  maxEvent: 40

Number of candidate solutions: 27683 (using event min/max entries)

New solver results...

Integer (non-subframe) solution...
sigB:47553.46  sigA:37634.00 B:341565.21 A:117641.47
in entryNum units: D: 418  R: 433

noise corr coefs: [1.00]  (based on 904 points)  sigmaB: 46989.29

Subframe adjusted solution...
sigB:47444.39  sigA:37634.00 B:341749.62 A:117641.47
in entryNum units: D: 417  R: 433  D(subframe): 417.6353  R(subframe): 433.3784

in frameNum units: D: 423  R: 439  D(subframe): 423.6353  R(subframe): 439.3784

... end New solver results

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

loDbar   @ .68 ci:  -0.2092
hiDbar   @ .68 ci:   0.2092
loDbar   @ .95 ci:  -0.5163
hiDbar   @ .95 ci:   0.4863
loDbar   @ .9973 ci:  -0.9919
hiDbar   @ .9973 ci:   0.9847

loDurBar @ .68 ci:  -0.3205
hiDurBar @ .68 ci:   0.3126
loDurBar @ .95 ci:  -0.7008
hiDurBar @ .95 ci:   0.7146
loDurBar @ .9973 ci:  -1.2262
hiDurBar @ .9973 ci:   1.2551

Timestamp validity check ...

From timestamps at D and R, calculated 16 reading blocks.  From reading blocks, calculated 16 blocks.

Timestamps appear valid @ D and R

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

B: 341749.62  {+/- 1579.50}  sigmaB: 47444.39

A: 117641.47  {+/- 9801.35}  sigmaA: 37634.00

magDrop report: percentDrop: 65.6  magDrop: 1.158  +/- 0.091  (0.68 ci)

snr: 4.72

D: 423.64 {+0.21,-0.21} (frame number)
D: [21:46:18.3093]  {+0.0837,-0.0837} seconds

R: 439.38 {+0.21,-0.21} (frame number)
R: [21:46:24.6089]  {+0.0837,-0.0837} seconds

Duration (R - D): 15.7431 {+0.3165,-0.3165} readings
Duration (R - D): 6.2997 {+0.1267,-0.1267} seconds

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

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

B: 341749.62  {+/- 3159.00}  sigmaB: 47444.39

A: 117641.47  {+/- 19602.71}  sigmaA: 37634.00

magDrop report: percentDrop: 65.6  magDrop: 1.158  +/- 0.181  (0.95 ci)

snr: 4.72

D: 423.64 {+0.50,-0.50} (frame number)
D: [21:46:18.3093]  {+0.2006,-0.2006} seconds

R: 439.38 {+0.50,-0.50} (frame number)
R: [21:46:24.6089]  {+0.2006,-0.2006} seconds

Duration (R - D): 15.7431 {+0.7077,-0.7077} readings
Duration (R - D): 6.2997 {+0.2832,-0.2832} seconds

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

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

B: 341749.62  {+/- 4738.50}  sigmaB: 47444.39

A: 117641.47  {+/- 29404.06}  sigmaA: 37634.00

magDrop report: percentDrop: 65.6  magDrop: 1.158  +/- 0.272  (0.9973 ci)

snr: 4.72

D: 423.64 {+0.99,-0.99} (frame number)
D: [21:46:18.3093]  {+0.3955,-0.3955} seconds

R: 439.38 {+0.99,-0.99} (frame number)
R: [21:46:24.6089]  {+0.3955,-0.3955} seconds

Duration (R - D): 15.7431 {+1.2406,-1.2406} readings
Duration (R - D): 6.2997 {+0.4964,-0.4964} seconds

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

D frame number: 423.64
D: 0.6800 containment intervals:  {+/- 0.21} (readings)
D: 0.9500 containment intervals:  {+/- 0.52} (readings)
D: 0.9973 containment intervals:  {+/- 0.99} (readings)

R frame number: 439.38
R: 0.6800 containment intervals:  {+/- 0.21} (readings)
R: 0.9500 containment intervals:  {+/- 0.52} (readings)
R: 0.9973 containment intervals:  {+/- 0.99} (readings)

Duration (R - D): 15.7431 readings
Duration: 0.6800 containment intervals:  {+/- 0.3165} (readings)
Duration: 0.9500 containment intervals:  {+/- 0.7077} (readings)
Duration: 0.9973 containment intervals:  {+/- 1.2406} (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: 65.6  magDrop: 1.158  +/- 0.181  (0.95 ci)

snr: 4.72

D time: [21:46:18.3093]
D: 0.6800 containment intervals:  {+/- 0.0837} seconds
D: 0.9500 containment intervals:  {+/- 0.2006} seconds
D: 0.9973 containment intervals:  {+/- 0.3955} seconds

R time: [21:46:24.6089]
R: 0.6800 containment intervals:  {+/- 0.0837} seconds
R: 0.9500 containment intervals:  {+/- 0.2006} seconds
R: 0.9973 containment intervals:  {+/- 0.3955} seconds

Duration (R - D): 6.2997 seconds
Duration: 0.6800 containment intervals:  {+/- 0.1267} seconds
Duration: 0.9500 containment intervals:  {+/- 0.2832} seconds
Duration: 0.9973 containment intervals:  {+/- 0.4964} 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: Sun Dec  1 09:27:56 2024  ####################