#################### PYOTE 5.1.0  session started: Tue Mar 25 21:05:23 2025  ####################

filename: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2025_03_25_(83613) 2001 SR286\20250325_194203_816x620_G24dB_0050ms\dynamic170.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\2025_03_25_(83613) 2001 SR286\20250325_194203_816x620_G24dB_0050ms.adv
#
# Aperture photometry was used to extract the lightcurves
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: ref
# ____ aperture size: 31
# ____ x,y: (62, 389) at frame 2625
# ____ threshold: 99999
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 1
#
# aperture name: target_dynamic
# ____ aperture size: 31
# ____ x,y: (550, 442) at frame 2625
# ____ threshold: 170
# ____ def mask radius: 3.2
# ____ color: green
# ____ joggable: True
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 5
#
# date at frame 0: 2025-03-25
#ACQUISITION-DELAY: 0.0
#ALTITUDE: 258.1
#AUTHOR: Stefano Sposetti
#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: 96
#CAMERA-VENDOR-NAME: DVTI
#COMMENT: 
#HEIGHT: 620
#INSTRUMENT: DVTI+CAM #96 FW 1.2.0, Sensor IMX430
#LATITUDE: 46.2313579
#LONGITUDE: 9.0239556
#OBJNAME: 
#OBSERVER: Stefano Sposetti
#RECORDER-SOFTWARE: DvtiCamControl
#RECORDER-SOFTWARE-VERSION: 5.8.1-51
#TELESCOPE: N420
#WIDTH: 816
#
# Aperture photometry was used to extract the lightcurves
==================== end header lines ====================

No time step irregularities found.

timeDelta: 0.0500000 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 ...
Background regions cleared.

signal-target_dynamic is the target curve.

Use min/max event to locate a "D and R" event has been selected

minEvent: 6  maxEvent: 20

Number of candidate solutions: 39165 (using event min/max entries)

New solver results...

Integer (non-subframe) solution...
sigB:3032.14  sigA:1304.54 B:12681.51 A:835.78
in entryNum units: D: 1247  R: 1256

noise corr coefs: [1.00, 0.184]  (based on 2616 points)  sigmaB: 3001.01

Subframe adjusted solution...
sigB:3001.01  sigA:3001.01 B:12681.51 A:835.78
in entryNum units: D: 1247  R: 1256  D(subframe): 1247.0000  R(subframe): 1256.0000

in frameNum units: D: 1248  R: 1257  D(subframe): 1248.0000  R(subframe): 1257.0000

... end New solver results

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

loDbar   @ .68 ci:  -0.2966
hiDbar   @ .68 ci:   0.2896
loDbar   @ .95 ci:  -0.7412
hiDbar   @ .95 ci:   0.7610
loDbar   @ .9973 ci:  -2.0923
hiDbar   @ .9973 ci:   1.9595

loDurBar @ .68 ci:  -0.4537
hiDurBar @ .68 ci:   0.4456
loDurBar @ .95 ci:  -1.0662
hiDurBar @ .95 ci:   1.0442
loDurBar @ .9973 ci:  -2.5655
hiDurBar @ .9973 ci:   2.4264

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: 12681.51  {+/- 58.69}  sigmaB: 3001.01

A: 835.78  {+/- 1061.02}  sigmaA: 3001.01

magDrop report: percentDrop: 93.4  magDrop: 2.953  +/- 1.378  (0.68 ci)

snr: 3.95

D: 1248.00 {+0.29,-0.29} (frame number)
D: [19:43:05.9260]  {+0.0147,-0.0147} seconds

R: 1257.00 {+0.29,-0.29} (frame number)
R: [19:43:06.3760]  {+0.0147,-0.0147} seconds

Duration (R - D): 9.0000 {+0.4497,-0.4497} readings
Duration (R - D): 0.4500 {+0.0225,-0.0225} seconds

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

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

B: 12681.51  {+/- 117.37}  sigmaB: 3001.01

A: 835.78  {+/- 2122.04}  sigmaA: 3001.01

magDrop report: percentDrop: 93.4  magDrop: 2.953  +/- 2.757  (0.95 ci)

snr: 3.95

D: 1248.00 {+0.75,-0.75} (frame number)
D: [19:43:05.9260]  {+0.0376,-0.0376} seconds

R: 1257.00 {+0.75,-0.75} (frame number)
R: [19:43:06.3760]  {+0.0376,-0.0376} seconds

Duration (R - D): 9.0000 {+1.0552,-1.0552} readings
Duration (R - D): 0.4500 {+0.0528,-0.0528} seconds

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

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

B: 12681.51  {+/- 176.06}  sigmaB: 3001.01

A: 835.78  {+/- 3183.05}  sigmaA: 3001.01

magDrop report: percentDrop: 93.4  magDrop: 2.953  too much noise; cannot calculate error bars

snr: 3.95

D: 1248.00 {+2.03,-2.03} (frame number)
D: [19:43:05.9260]  {+0.1013,-0.1013} seconds

R: 1257.00 {+2.03,-2.03} (frame number)
R: [19:43:06.3760]  {+0.1013,-0.1013} seconds

Duration (R - D): 9.0000 {+2.4960,-2.4960} readings
Duration (R - D): 0.4500 {+0.1248,-0.1248} seconds

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

D frame number: 1248.00
D: 0.6800 containment intervals:  {+/- 0.30} (readings)
D: 0.9500 containment intervals:  {+/- 0.76} (readings)
D: 0.9973 containment intervals:  {+/- 2.09} (readings)

R frame number: 1257.00
R: 0.6800 containment intervals:  {+/- 0.30} (readings)
R: 0.9500 containment intervals:  {+/- 0.76} (readings)
R: 0.9973 containment intervals:  {+/- 2.09} (readings)

Duration (R - D): 9.0000 readings
Duration: 0.6800 containment intervals:  {+/- 0.4497} (readings)
Duration: 0.9500 containment intervals:  {+/- 1.0552} (readings)
Duration: 0.9973 containment intervals:  {+/- 2.4960} (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: 93.4  magDrop: 2.953  +/- 2.757  (0.95 ci)

snr: 3.95

D time: [19:43:05.9260]
D: 0.6800 containment intervals:  {+/- 0.0147} seconds
D: 0.9500 containment intervals:  {+/- 0.0376} seconds
D: 0.9973 containment intervals:  {+/- 0.1013} seconds

R time: [19:43:06.3760]
R: 0.6800 containment intervals:  {+/- 0.0147} seconds
R: 0.9500 containment intervals:  {+/- 0.0376} seconds
R: 0.9973 containment intervals:  {+/- 0.1013} seconds

Duration (R - D): 0.4500 seconds
Duration: 0.6800 containment intervals:  {+/- 0.0225} seconds
Duration: 0.9500 containment intervals:  {+/- 0.0528} seconds
Duration: 0.9973 containment intervals:  {+/- 0.1248} 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