#################### PYOTE 5.1.2 session started: Sun Jun 11 00:05:01 2023 ####################



#################### PYOTE 5.1.2 session started: Sun Jun 11 00:05:01 2023 ####################



#################### PYOTE 5.1.2 session started: Sun Jun 11 00:05:01 2023 ####################

filename: C:\Users\aschw\Desktop\kaliope.csv

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

==================== file header lines ====================
# PyMovie Version 3.7.0
# source: C:/Users/aschw/Desktop/DvtiData/20230610_214317_1624x1240_G36dBD_1000ms.adv
#
# lunar background: False
# yellow mask = default: False
#
# aperture name: target
# ____ aperture size: 21
# ____ x,y: (827, 589)
# ____ threshold: 2000
# ____ def mask radius: 3.2
# ____ color: red
# ____ joggable: False
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 10
#
# aperture name: ref
# ____ aperture size: 21
# ____ x,y: (814, 684)
# ____ threshold: 2000
# ____ def mask radius: 3.2
# ____ color: yellow
# ____ joggable: True
# ____ auto textOut: False
# ____ thumbnail source: False
# ____ csv output order: 11
#
# date at frame 0: 2023-06-10
#ACQUISITION-DELAY: 0.0
#ALTITUDE: 597.8
#AUTHOR: Andreas SCHWEIZER
#BINNING-X: 1
#BINNING-Y: 1
#CAMERA-DRIVER-NAME: UVC
#CAMERA-FIRMWARE-VERSION: 1.0.3
#CAMERA-MODEL: DVTI+CAM
#CAMERA-SENSOR-INFO: Sony IMX430LLJ-C (1.1" 1624x1240 4.5um CIS)
#CAMERA-SERIAL-NO: 17
#CAMERA-VENDOR-NAME: DVTI
#COMMENT: 
#DEC: -24.811992
#HEIGHT: 1240
#INSTRUMENT: DVTI+CAM #17 FW 1.0.3, Sensor IMX430
#LATITUDE: 47.3418275
#LONGITUDE: 8.4728547
#OBJNAME: (104) Klymene occ. UCAC4 326-089169
#OBSERVER: Andreas SCHWEIZER
#RA: 16.924962
#RECORDER-SOFTWARE: DvtiCamControl
#RECORDER-SOFTWARE-VERSION: 5.6.1-15
#TELESCOPE: Borg 107FL
#WIDTH: 1624
==================== end header lines ====================

No time step irregularities found.

timeDelta: 1.00000 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: [18, 34]

R zone selected: [36, 50]

Locate a "D and R" event has been selected

Number of candidate solutions: 255 (using D/R region selections)

New solver results...

Integer (non-subframe) solution...
sigB:22174.24 sigA:13525.28 B:126972.74 A:58918.75
in entryNum units: D: 31 R: 39

noise corr coefs: [1.00] (based on 57 points) sigmaB: 21646.40

Subframe adjusted solution...
sigB:21646.40 sigA:21646.40 B:126972.74 A:58918.75
in entryNum units: D: 31 R: 39 D(subframe): 31.0000 R(subframe): 39.0000

in frameNum units: D: 32 R: 40 D(subframe): 32.0000 R(subframe): 40.0000

... end New solver results

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

loDbar @ .68 ci: -0.3922
hiDbar @ .68 ci: 0.3861
loDbar @ .95 ci: -1.0562
hiDbar @ .95 ci: 1.0747
loDbar @ .9973 ci: -2.7302
hiDbar @ .9973 ci: 2.6666

loDurBar @ .68 ci: -0.6251
hiDurBar @ .68 ci: 0.6072
loDurBar @ .95 ci: -1.5296
hiDurBar @ .95 ci: 1.5478
loDurBar @ .9973 ci: -3.3449
hiDurBar @ .9973 ci: 3.4311

Timestamp validity check ...

From timestamps at D and R, calculated 8 reading blocks. From reading blocks, calculated 8 blocks.

Timestamps appear valid @ D and R

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

B: 126972.74 {+/- 2892.62} sigmaB: 21646.40

A: 58918.75 {+/- 8181.57} sigmaA: 21646.40

magDrop report: percentDrop: 53.6 magDrop: 0.834 +/- 0.153 (0.68 ci)

snr: 3.14

D: 32.00 {+0.39,-0.39} (frame number)
D: [21:43:50.2680] {+0.3892,-0.3892} seconds

R: 40.00 {+0.39,-0.39} (frame number)
R: [21:43:58.2680] {+0.3892,-0.3892} seconds

Duration (R - D): 8.0000 {+0.6161,-0.6161} readings
Duration (R - D): 8.0000 {+0.6161,-0.6161} seconds

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

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

B: 126972.74 {+/- 5785.24} sigmaB: 21646.40

A: 58918.75 {+/- 16363.14} sigmaA: 21646.40

magDrop report: percentDrop: 53.6 magDrop: 0.834 +/- 0.306 (0.95 ci)

snr: 3.14

D: 32.00 {+1.07,-1.07} (frame number)
D: [21:43:50.2680] {+1.0654,-1.0654} seconds

R: 40.00 {+1.07,-1.07} (frame number)
R: [21:43:58.2680] {+1.0654,-1.0654} seconds

Duration (R - D): 8.0000 {+1.5387,-1.5387} readings
Duration (R - D): 8.0000 {+1.5387,-1.5387} seconds

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

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

B: 126972.74 {+/- 8677.86} sigmaB: 21646.40

A: 58918.75 {+/- 24544.71} sigmaA: 21646.40

magDrop report: percentDrop: 53.6 magDrop: 0.834 +/- 0.458 (0.9973 ci)

snr: 3.14

D: 32.00 {+2.70,-2.70} (frame number)
D: [21:43:50.2680] {+2.6984,-2.6984} seconds

R: 40.00 {+2.70,-2.70} (frame number)
R: [21:43:58.2680] {+2.6984,-2.6984} seconds

Duration (R - D): 8.0000 {+3.3880,-3.3880} readings
Duration (R - D): 8.0000 {+3.3880,-3.3880} seconds

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

D frame number: 32.00
D: 0.6800 containment intervals: {+/- 0.39} (readings)
D: 0.9500 containment intervals: {+/- 1.07} (readings)
D: 0.9973 containment intervals: {+/- 2.73} (readings)

R frame number: 40.00
R: 0.6800 containment intervals: {+/- 0.39} (readings)
R: 0.9500 containment intervals: {+/- 1.07} (readings)
R: 0.9973 containment intervals: {+/- 2.73} (readings)

Duration (R - D): 8.0000 readings
Duration: 0.6800 containment intervals: {+/- 0.6161} (readings)
Duration: 0.9500 containment intervals: {+/- 1.5387} (readings)
Duration: 0.9973 containment intervals: {+/- 3.3880} (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: 53.6 magDrop: 0.834 +/- 0.306 (0.95 ci)

snr: 3.14

D time: [21:43:50.2680]
D: 0.6800 containment intervals: {+/- 0.3892} seconds
D: 0.9500 containment intervals: {+/- 1.0654} seconds
D: 0.9973 containment intervals: {+/- 2.6984} seconds

R time: [21:43:58.2680]
R: 0.6800 containment intervals: {+/- 0.3892} seconds
R: 0.9500 containment intervals: {+/- 1.0654} seconds
R: 0.9973 containment intervals: {+/- 2.6984} seconds

Duration (R - D): 8.0000 seconds
Duration: 0.6800 containment intervals: {+/- 0.6161} seconds
Duration: 0.9500 containment intervals: {+/- 1.5387} seconds
Duration: 0.9973 containment intervals: {+/- 3.3880} 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