#################### PYOTE 4.9.2 session started: Sun Mar 5 13:15:34 2023 #################### filename: E:\ASTRONOMIA\Immagini CCD\Occultazioni\2023_02_28_(85) Io\Io con PYMOVIE\Io con pymovie.csv If the csv file came from PyMovie - columns with prefix: signal will be read. ==================== file header lines ==================== # PyMovie Version 3.6.6 # source: E:/ASTRONOMIA/Immagini CCD/Occultazioni/2023_02_28_(85) Io/Capture 2023-02-28T19_54_25Z.adv # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 31 # ____ x,y: (173, 73) # ____ threshold: 3263 # ____ def mask radius: 3.2 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: reference1 # ____ aperture size: 31 # ____ x,y: (304, 266) # ____ threshold: 3200 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: reference2 # ____ aperture size: 31 # ____ x,y: (246, 116) # ____ threshold: 3239 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: background # ____ aperture size: 31 # ____ x,y: (109, 208) # ____ threshold: 99999 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 5 # # date at frame 0: 2023-02-28 #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: 11.7200002670288 #EFFECTIVE-PIXEL-SIZE-Y: 11.7200002670288 #FSTF-TYPE: ADV #HEIGHT: 300 #LATITUDE: 46.2314013333333 #LONGITUDE: 9.02405666666667 #POSITION-REFERENCE: WGS84 #RECORDER-SOFTWARE: SharpCap #RECORDER-SOFTWARE-VERSION: 4.0.9478.0 #WIDTH: 480 ==================== end header lines ==================== timeDelta: 0.0401540 seconds per reading timestamp error rate: 0.00% #################### Session ended: Sun Mar 5 13:17:06 2023 #################### #################### PYOTE 4.9.2 session started: Sun Mar 5 13:19:17 2023 #################### filename: E:\ASTRONOMIA\Immagini CCD\Occultazioni\2023_02_28_(85) Io\Io con PYMOVIE\Io con pymovie.csv If the csv file came from PyMovie - columns with prefix: signal will be read. ==================== file header lines ==================== # PyMovie Version 3.6.6 # source: E:/ASTRONOMIA/Immagini CCD/Occultazioni/2023_02_28_(85) Io/Capture 2023-02-28T19_54_25Z.adv # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 31 # ____ x,y: (173, 74) # ____ threshold: 3263 # ____ def mask radius: 3.2 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: reference1 # ____ aperture size: 31 # ____ x,y: (304, 267) # ____ threshold: 3200 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: reference2 # ____ aperture size: 31 # ____ x,y: (246, 116) # ____ threshold: 3239 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: background # ____ aperture size: 31 # ____ x,y: (110, 207) # ____ threshold: 99999 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 5 # # date at frame 0: 2023-02-28 #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: 11.7200002670288 #EFFECTIVE-PIXEL-SIZE-Y: 11.7200002670288 #FSTF-TYPE: ADV #HEIGHT: 300 #LATITUDE: 46.2314013333333 #LONGITUDE: 9.02405666666667 #POSITION-REFERENCE: WGS84 #RECORDER-SOFTWARE: SharpCap #RECORDER-SOFTWARE-VERSION: 4.0.9478.0 #WIDTH: 480 ==================== end header lines ==================== timeDelta: 0.0401540 seconds per reading timestamp error rate: 0.00% D zone selected: [231, 308] R zone selected: [545, 586] Locate a "D and R" event has been selected Number of candidate solutions: 3276 (using D/R region selections) New solver results... Integer (non-subframe) solution... sigB:28471.39 sigA:21422.10 B:191807.77 A:100961.26 in entryNum units: D: 272 R: 565 noise corr coefs: [1.00, 0.127, 0.0776] (based on 559 points) sigmaB: 28271.23 Subframe adjusted solution... sigB:28437.54 sigA:21422.10 B:191885.51 A:100961.26 in entryNum units: D: 271 R: 565 D(subframe): 271.5230 R(subframe): 565.0000 in frameNum units: D: 4571 R: 4865 D(subframe): 4571.5230 R(subframe): 4865.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.3048 hiDbar @ .68 ci: 0.3363 loDbar @ .95 ci: -0.8833 hiDbar @ .95 ci: 0.8071 loDbar @ .9973 ci: -2.5290 hiDbar @ .9973 ci: 2.2387 loDurBar @ .68 ci: -0.5110 hiDurBar @ .68 ci: 0.4920 loDurBar @ .95 ci: -1.2472 hiDurBar @ .95 ci: 1.2028 loDurBar @ .9973 ci: -3.0488 hiDurBar @ .9973 ci: 3.0518 Timestamp validity check ... From timestamps at D and R, calculated 294 reading blocks. From reading blocks, calculated 294 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 191885.51 {+/- 1204.37} sigmaB: 28437.54 A: 100961.26 {+/- 1252.61} sigmaA: 21422.10 magDrop: 0.697 +/- 0.015 (0.68 ci) snr: 3.20 D: 4571.52 {+0.34,-0.30} (frame number) D: [19:57:29.0599] {+0.0135,-0.0122} seconds R: 4865.00 {+0.30,-0.34} (frame number) R: [19:57:40.8442] {+0.0122,-0.0135} seconds Duration (R - D): 293.4770 {+0.5015,-0.5015} readings Duration (R - D): 11.7843 {+0.0201,-0.0201} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 191885.51 {+/- 2408.74} sigmaB: 28437.54 A: 100961.26 {+/- 2505.22} sigmaA: 21422.10 magDrop: 0.697 +/- 0.030 (0.95 ci) snr: 3.20 D: 4571.52 {+0.81,-0.88} (frame number) D: [19:57:29.0599] {+0.0324,-0.0355} seconds R: 4865.00 {+0.88,-0.81} (frame number) R: [19:57:40.8442] {+0.0355,-0.0324} seconds Duration (R - D): 293.4770 {+1.2250,-1.2250} readings Duration (R - D): 11.7843 {+0.0492,-0.0492} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 191885.51 {+/- 3613.12} sigmaB: 28437.54 A: 100961.26 {+/- 3757.83} sigmaA: 21422.10 magDrop: 0.697 +/- 0.045 (0.9973 ci) snr: 3.20 D: 4571.52 {+2.24,-2.53} (frame number) D: [19:57:29.0599] {+0.0899,-0.1015} seconds R: 4865.00 {+2.53,-2.24} (frame number) R: [19:57:40.8442] {+0.1015,-0.0899} seconds Duration (R - D): 293.4770 {+3.0503,-3.0503} readings Duration (R - D): 11.7843 {+0.1225,-0.1225} seconds =============== end 0.9973 containment interval report ============= D frame number: 4571.52 D: 0.6800 containment intervals: {+/- 0.34} (readings) D: 0.9500 containment intervals: {+/- 0.88} (readings) D: 0.9973 containment intervals: {+/- 2.53} (readings) R frame number: 4865.00 R: 0.6800 containment intervals: {+/- 0.34} (readings) R: 0.9500 containment intervals: {+/- 0.88} (readings) R: 0.9973 containment intervals: {+/- 2.53} (readings) Duration (R - D): 293.4770 readings Duration: 0.6800 containment intervals: {+/- 0.5015} (readings) Duration: 0.9500 containment intervals: {+/- 1.2250} (readings) Duration: 0.9973 containment intervals: {+/- 3.0503} (readings) =============== Summary report for Excel file ===================== This light curve has not been block integrated. The following lightcurve parameters were utilized: ==== use diff: is checked ==== exp: 0.040154 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: 0.697 +/- 0.030 (0.95 ci) snr: 3.20 D time: [19:57:29.0599] D: 0.6800 containment intervals: {+/- 0.0135} seconds D: 0.9500 containment intervals: {+/- 0.0355} seconds D: 0.9973 containment intervals: {+/- 0.1015} seconds R time: [19:57:40.8442] R: 0.6800 containment intervals: {+/- 0.0135} seconds R: 0.9500 containment intervals: {+/- 0.0355} seconds R: 0.9973 containment intervals: {+/- 0.1015} seconds Duration (R - D): 11.7843 seconds Duration: 0.6800 containment intervals: {+/- 0.0201} seconds Duration: 0.9500 containment intervals: {+/- 0.0492} seconds Duration: 0.9973 containment intervals: {+/- 0.1225} 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 Mar 5 13:25:05 2023 ####################