#################### PYOTE 5.1.0 session started: Wed Jan 1 09:39:01 2025 #################### filename: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2024_12_31_(137) Meliboea\Capture 2024-12-31T18_08_55Z\Meliboea_pymovie.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_12_31_(137) Meliboea\Capture 2024-12-31T18_08_55Z.adv # # Aperture photometry was used to extract the lightcurves # # lunar background: False # yellow mask = default: False # # aperture name: ref # ____ aperture size: 31 # ____ x,y: (126, 103) at frame 2100 # ____ threshold: 3201 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: target # ____ aperture size: 31 # ____ x,y: (383, 159) at frame 2100 # ____ threshold: 3097 # ____ def mask radius: 3.2 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: bg # ____ aperture size: 31 # ____ x,y: (327, 223) at frame 2100 # ____ threshold: 99999 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: True # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 3 # # date at frame 0: 2024-12-31 #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: 46.2314445 #LONGITUDE: 9.02407 #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: 0.100148 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 ... signal-target is the target curve. Use min/max event to locate a "D and R" event has been selected minEvent: 30 maxEvent: 80 Number of candidate solutions: 32895 (using event min/max entries) New solver results... Integer (non-subframe) solution... sigB:24538.66 sigA:15503.16 B:180798.20 A:72944.09 in entryNum units: D: 345 R: 392 noise corr coefs: [1.00] (based on 654 points) sigmaB: 24369.88 Subframe adjusted solution... sigB:24369.88 sigA:15501.29 B:180798.20 A:72944.09 in entryNum units: D: 345 R: 392 D(subframe): 345.0000 R(subframe): 392.0000 in frameNum units: D: 1745 R: 1792 D(subframe): 1745.0000 R(subframe): 1792.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.1944 hiDbar @ .68 ci: 0.2096 loDbar @ .95 ci: -0.5039 hiDbar @ .95 ci: 0.4718 loDbar @ .9973 ci: -0.9923 hiDbar @ .9973 ci: 0.9010 loDurBar @ .68 ci: -0.3050 hiDurBar @ .68 ci: 0.3055 loDurBar @ .95 ci: -0.6818 hiDurBar @ .95 ci: 0.6795 loDurBar @ .9973 ci: -1.2256 hiDurBar @ .9973 ci: 1.1895 Timestamp validity check ... From timestamps at D and R, calculated 47 reading blocks. From reading blocks, calculated 47 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 180798.20 {+/- 953.67} sigmaB: 24369.88 A: 72944.09 {+/- 2285.54} sigmaA: 15501.29 magDrop report: percentDrop: 59.7 magDrop: 0.986 +/- 0.034 (0.68 ci) snr: 4.43 D: 1745.00 {+0.21,-0.19} (frame number) D: [18:11:50.2049] {+0.0210,-0.0195} seconds R: 1792.00 {+0.19,-0.21} (frame number) R: [18:11:54.9119] {+0.0195,-0.0210} seconds Duration (R - D): 47.0000 {+0.3052,-0.3052} readings Duration (R - D): 4.7070 {+0.0306,-0.0306} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 180798.20 {+/- 1907.33} sigmaB: 24369.88 A: 72944.09 {+/- 4571.08} sigmaA: 15501.29 magDrop report: percentDrop: 59.7 magDrop: 0.986 +/- 0.069 (0.95 ci) snr: 4.43 D: 1745.00 {+0.47,-0.50} (frame number) D: [18:11:50.2049] {+0.0473,-0.0505} seconds R: 1792.00 {+0.50,-0.47} (frame number) R: [18:11:54.9119] {+0.0505,-0.0473} seconds Duration (R - D): 47.0000 {+0.6807,-0.6807} readings Duration (R - D): 4.7070 {+0.0682,-0.0682} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 180798.20 {+/- 2861.00} sigmaB: 24369.88 A: 72944.09 {+/- 6856.62} sigmaA: 15501.29 magDrop report: percentDrop: 59.7 magDrop: 0.986 +/- 0.103 (0.9973 ci) snr: 4.43 D: 1745.00 {+0.90,-0.99} (frame number) D: [18:11:50.2049] {+0.0902,-0.0994} seconds R: 1792.00 {+0.99,-0.90} (frame number) R: [18:11:54.9119] {+0.0994,-0.0902} seconds Duration (R - D): 47.0000 {+1.2076,-1.2076} readings Duration (R - D): 4.7070 {+0.1209,-0.1209} seconds =============== end 0.9973 containment interval report ============= D frame number: 1745.00 D: 0.6800 containment intervals: {+/- 0.21} (readings) D: 0.9500 containment intervals: {+/- 0.50} (readings) D: 0.9973 containment intervals: {+/- 0.99} (readings) R frame number: 1792.00 R: 0.6800 containment intervals: {+/- 0.21} (readings) R: 0.9500 containment intervals: {+/- 0.50} (readings) R: 0.9973 containment intervals: {+/- 0.99} (readings) Duration (R - D): 47.0000 readings Duration: 0.6800 containment intervals: {+/- 0.3052} (readings) Duration: 0.9500 containment intervals: {+/- 0.6807} (readings) Duration: 0.9973 containment intervals: {+/- 1.2076} (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: 59.7 magDrop: 0.986 +/- 0.069 (0.95 ci) snr: 4.43 D time: [18:11:50.2049] D: 0.6800 containment intervals: {+/- 0.0210} seconds D: 0.9500 containment intervals: {+/- 0.0505} seconds D: 0.9973 containment intervals: {+/- 0.0994} seconds R time: [18:11:54.9119] R: 0.6800 containment intervals: {+/- 0.0210} seconds R: 0.9500 containment intervals: {+/- 0.0505} seconds R: 0.9973 containment intervals: {+/- 0.0994} seconds Duration (R - D): 4.7070 seconds Duration: 0.6800 containment intervals: {+/- 0.0306} seconds Duration: 0.9500 containment intervals: {+/- 0.0682} seconds Duration: 0.9973 containment intervals: {+/- 0.1209} 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: Wed Jan 1 09:43:02 2025 ####################