#################### PYOTE 4.9.2 session started: Sun Jan 14 10:07:01 2024 #################### filename: E:\ASTRONOMIA\Immagini CCD\Occultazioni\2024_01_13_(510) Mabella\per pymovie\Capture 2024-01-13T22_35_55Z\mabella_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\2024_01_13_(510) Mabella\Capture 2024-01-13T22_35_55Z.adv # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 31 # ____ x,y: (186, 211) # ____ threshold: 3281 # ____ def mask radius: 3.2 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: ref # ____ aperture size: 31 # ____ x,y: (255, 215) # ____ threshold: 3202 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 1 # # date at frame 0: 2024-01-13 #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: 46.231487333333334 #LONGITUDE: 9.024128333333334 #POSITION-REFERENCE: WGS84 #RECORDER-SOFTWARE: SharpCap #RECORDER-SOFTWARE-VERSION: 4.1.11351.0 #WIDTH: 480 ==================== end header lines ==================== timeDelta: 0.100149 seconds per reading timestamp error rate: 0.00% Use min/max event to locate a "D and R" event has been selected minEvent: 4 maxEvent: 30 Number of candidate solutions: 17091 (using event min/max entries) New solver results... Integer (non-subframe) solution... sigB:26264.80 sigA:24534.85 B:195026.93 A:54053.60 in entryNum units: D: 320 R: 340 noise corr coefs: [1.00, 0.0954] (based on 631 points) sigmaB: 25977.68 Subframe adjusted solution... sigB:26107.50 sigA:24534.85 B:195203.76 A:54053.60 in entryNum units: D: 319 R: 340 D(subframe): 319.6990 R(subframe): 340.4893 in frameNum units: D: 1819 R: 1840 D(subframe): 1819.6990 R(subframe): 1840.4893 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.1893 hiDbar @ .68 ci: 0.2078 loDbar @ .95 ci: -0.4657 hiDbar @ .95 ci: 0.4830 loDbar @ .9973 ci: -0.9229 hiDbar @ .9973 ci: 0.9459 loDurBar @ .68 ci: -0.3075 hiDurBar @ .68 ci: 0.2905 loDurBar @ .95 ci: -0.6698 hiDurBar @ .95 ci: 0.6641 loDurBar @ .9973 ci: -1.2249 hiDurBar @ .9973 ci: 1.1701 Timestamp validity check ... From timestamps at D and R, calculated 21 reading blocks. From reading blocks, calculated 21 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 195203.76 {+/- 1040.80} sigmaB: 26107.50 A: 54053.60 {+/- 5515.15} sigmaA: 24534.85 magDrop: 1.394 +/- 0.111 (0.68 ci) snr: 5.41 D: 1819.70 {+0.20,-0.20} (frame number) D: [22:38:57.4487] {+0.0199,-0.0199} seconds R: 1840.49 {+0.20,-0.20} (frame number) R: [22:38:59.5308] {+0.0199,-0.0199} seconds Duration (R - D): 20.7903 {+0.2990,-0.2990} readings Duration (R - D): 2.0821 {+0.0299,-0.0299} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 195203.76 {+/- 2081.60} sigmaB: 26107.50 A: 54053.60 {+/- 11030.30} sigmaA: 24534.85 magDrop: 1.394 +/- 0.222 (0.95 ci) snr: 5.41 D: 1819.70 {+0.47,-0.47} (frame number) D: [22:38:57.4487] {+0.0475,-0.0475} seconds R: 1840.49 {+0.47,-0.47} (frame number) R: [22:38:59.5308] {+0.0475,-0.0475} seconds Duration (R - D): 20.7903 {+0.6670,-0.6670} readings Duration (R - D): 2.0821 {+0.0668,-0.0668} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 195203.76 {+/- 3122.40} sigmaB: 26107.50 A: 54053.60 {+/- 16545.45} sigmaA: 24534.85 magDrop: 1.394 +/- 0.333 (0.9973 ci) snr: 5.41 D: 1819.70 {+0.93,-0.93} (frame number) D: [22:38:57.4487] {+0.0936,-0.0936} seconds R: 1840.49 {+0.93,-0.93} (frame number) R: [22:38:59.5308] {+0.0936,-0.0936} seconds Duration (R - D): 20.7903 {+1.1975,-1.1975} readings Duration (R - D): 2.0821 {+0.1199,-0.1199} seconds =============== end 0.9973 containment interval report ============= D frame number: 1819.70 D: 0.6800 containment intervals: {+/- 0.21} (readings) D: 0.9500 containment intervals: {+/- 0.48} (readings) D: 0.9973 containment intervals: {+/- 0.95} (readings) R frame number: 1840.49 R: 0.6800 containment intervals: {+/- 0.21} (readings) R: 0.9500 containment intervals: {+/- 0.48} (readings) R: 0.9973 containment intervals: {+/- 0.95} (readings) Duration (R - D): 20.7903 readings Duration: 0.6800 containment intervals: {+/- 0.2990} (readings) Duration: 0.9500 containment intervals: {+/- 0.6670} (readings) Duration: 0.9973 containment intervals: {+/- 1.1975} (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: 0.100149 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: 1.394 +/- 0.222 (0.95 ci) snr: 5.41 D time: [22:38:57.4487] D: 0.6800 containment intervals: {+/- 0.0199} seconds D: 0.9500 containment intervals: {+/- 0.0475} seconds D: 0.9973 containment intervals: {+/- 0.0936} seconds R time: [22:38:59.5308] R: 0.6800 containment intervals: {+/- 0.0199} seconds R: 0.9500 containment intervals: {+/- 0.0475} seconds R: 0.9973 containment intervals: {+/- 0.0936} seconds Duration (R - D): 2.0821 seconds Duration: 0.6800 containment intervals: {+/- 0.0299} seconds Duration: 0.9500 containment intervals: {+/- 0.0668} seconds Duration: 0.9973 containment intervals: {+/- 0.1199} 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