#################### PYOTE 5.1.0 session started: Sat Apr 13 16:50:03 2024 #################### filename: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2024_04_12_(4446) Carolyn\Capture 2024-04-12T03_42_56Z\CarolynWithPymovie.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_04_12_(4446) Carolyn\Capture 2024-04-12T03_42_56Z.adv # # Aperture photometry was used to extract the lightcurves # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 31 # ____ x,y: (167, 118) at frame 820 # ____ threshold: 1458 # ____ 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: (278, 275) at frame 820 # ____ threshold: 1489 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: True # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # date at frame 0: 2024-04-12 #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: 46.23143816666666 #LONGITUDE: 9.024051666666667 #POSITION-REFERENCE: WGS84 #RECORDER-SOFTWARE: SharpCap #RECORDER-SOFTWARE-VERSION: 4.1.11351.0 #WIDTH: 480 # # Aperture photometry was used to extract the lightcurves ==================== end header lines ==================== At reading 00305: time delta to next reading = 0.6003 : likely 1 dropped readings At reading 00639: time delta to next reading = 0.6003 : likely 1 dropped readings ========== Total dropped readings..... 2 ========== Num duplicated readings.... 0 ========== Number timestamp errors.... 0 ========== Number of cadence errors... 2 timeDelta: 0.300144 seconds per reading timestamp error rate: 0.244% 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: 2 maxEvent: 9 Number of candidate solutions: 6516 (using event min/max entries) New solver results... Integer (non-subframe) solution... sigB:14112.20 sigA:15652.58 B:63734.56 A:10719.00 in entryNum units: D: 458 R: 463 noise corr coefs: [1.00, 0.0873, 0.103, 0.0560, 0.0516] (based on 816 points) sigmaB: 12456.43 Subframe adjusted solution... sigB:14112.20 sigA:11796.36 B:63734.56 A:4938.00 in entryNum units: D: 458 R: 462 D(subframe): 458.0000 R(subframe): 462.5638 in frameNum units: D: 458 R: 462 D(subframe): 458.0000 R(subframe): 462.5638 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.2422 hiDbar @ .68 ci: 0.2534 loDbar @ .95 ci: -0.6320 hiDbar @ .95 ci: 0.5966 loDbar @ .9973 ci: -1.2993 hiDbar @ .9973 ci: 1.2508 loDurBar @ .68 ci: -0.3820 hiDurBar @ .68 ci: 0.3722 loDurBar @ .95 ci: -0.8597 hiDurBar @ .95 ci: 0.8515 loDurBar @ .9973 ci: -1.7845 hiDurBar @ .9973 ci: 1.6230 Timestamp validity check ... From timestamps at D and R, calculated 4 reading blocks. From reading blocks, calculated 4 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 63734.56 {+/- 494.20} sigmaB: 14112.20 A: 4938.00 {+/- 6248.72} sigmaA: 11796.36 magDrop report: percentDrop: 92.3 magDrop: 2.777 +/- 1.374 (0.68 ci) snr: 4.17 D: 458.00 {+0.25,-0.25} (frame number) D: [03:45:13.6892] {+0.0744,-0.0744} seconds R: 462.56 {+0.25,-0.25} (frame number) R: [03:45:15.0590] {+0.0744,-0.0744} seconds Duration (R - D): 4.5638 {+0.3771,-0.3771} readings Duration (R - D): 1.3698 {+0.1132,-0.1132} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 63734.56 {+/- 988.39} sigmaB: 14112.20 A: 4938.00 {+/- 12497.45} sigmaA: 11796.36 magDrop report: percentDrop: 92.3 magDrop: 2.777 +/- 2.748 (0.95 ci) snr: 4.17 D: 458.00 {+0.61,-0.61} (frame number) D: [03:45:13.6892] {+0.1844,-0.1844} seconds R: 462.56 {+0.61,-0.61} (frame number) R: [03:45:15.0590] {+0.1844,-0.1844} seconds Duration (R - D): 4.5638 {+0.8556,-0.8556} readings Duration (R - D): 1.3698 {+0.2568,-0.2568} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 63734.56 {+/- 1482.59} sigmaB: 14112.20 A: 4938.00 {+/- 18746.17} sigmaA: 11796.36 magDrop report: percentDrop: 92.3 magDrop: 2.777 too much noise; cannot calculate error bars snr: 4.17 D: 458.00 {+1.28,-1.28} (frame number) D: [03:45:13.6892] {+0.3827,-0.3827} seconds R: 462.56 {+1.28,-1.28} (frame number) R: [03:45:15.0590] {+0.3827,-0.3827} seconds Duration (R - D): 4.5638 {+1.7038,-1.7038} readings Duration (R - D): 1.3698 {+0.5114,-0.5114} seconds =============== end 0.9973 containment interval report ============= D frame number: 458.00 D: 0.6800 containment intervals: {+/- 0.25} (readings) D: 0.9500 containment intervals: {+/- 0.63} (readings) D: 0.9973 containment intervals: {+/- 1.30} (readings) R frame number: 462.56 R: 0.6800 containment intervals: {+/- 0.25} (readings) R: 0.9500 containment intervals: {+/- 0.63} (readings) R: 0.9973 containment intervals: {+/- 1.30} (readings) Duration (R - D): 4.5638 readings Duration: 0.6800 containment intervals: {+/- 0.3771} (readings) Duration: 0.9500 containment intervals: {+/- 0.8556} (readings) Duration: 0.9973 containment intervals: {+/- 1.7038} (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: 92.3 magDrop: 2.777 +/- 2.748 (0.95 ci) snr: 4.17 D time: [03:45:13.6892] D: 0.6800 containment intervals: {+/- 0.0744} seconds D: 0.9500 containment intervals: {+/- 0.1844} seconds D: 0.9973 containment intervals: {+/- 0.3827} seconds R time: [03:45:15.0590] R: 0.6800 containment intervals: {+/- 0.0744} seconds R: 0.9500 containment intervals: {+/- 0.1844} seconds R: 0.9973 containment intervals: {+/- 0.3827} seconds Duration (R - D): 1.3698 seconds Duration: 0.6800 containment intervals: {+/- 0.1132} seconds Duration: 0.9500 containment intervals: {+/- 0.2568} seconds Duration: 0.9973 containment intervals: {+/- 0.5114} 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: Sat Apr 13 16:52:26 2024 ####################