#################### PYOTE 4.8.4 session started: Fri Aug 12 02:31:22 2022 #################### filename: /Volumes/MY PASSPORT/astro/occultations/20220809_50000_Quaoar/20220809_50000_Quaoar_Bender/20220809_50000_Quaoar_Bender.csv If the csv file came from PyMovie - columns with prefix: signal will be read. fourcc code of avi: dvsd fps: 29.97002997002997 avi contains 53893 frames ==================== file header lines ==================== # PyMovie Version 3.4.2 # source: /Volumes/MY PASSPORT/astro/occultations/20220809_50000_Quaoar/20220809_50000_Quaoar_Bender.avi # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 11 # ____ x,y: (356, 154) # ____ threshold: 99999 # ____ def mask radius: 4.0 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: tracking1 # ____ aperture size: 11 # ____ x,y: (460, 283) # ____ threshold: 46 # ____ def mask radius: 4.0 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: tracking2 # ____ aperture size: 11 # ____ x,y: (135, 219) # ____ threshold: 46 # ____ def mask radius: 4.0 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 3 # # aperture name: nostar # ____ aperture size: 11 # ____ x,y: (317, 182) # ____ threshold: 99999 # ____ def mask radius: 4.0 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 4 # ==================== end header lines ==================== timeDelta: 0.0333662 seconds per reading timestamp error rate: 0.0575% #################### PYOTE 4.8.4 session started: Fri Aug 12 02:31:37 2022 #################### filename: /Volumes/MY PASSPORT/astro/occultations/20220809_50000_Quaoar/20220809_50000_Quaoar_Bender/20220809_50000_Quaoar_Bender.csv If the csv file came from PyMovie - columns with prefix: appsum will be read. fourcc code of avi: dvsd fps: 29.97002997002997 avi contains 53893 frames ==================== file header lines ==================== # PyMovie Version 3.4.2 # source: /Volumes/MY PASSPORT/astro/occultations/20220809_50000_Quaoar/20220809_50000_Quaoar_Bender.avi # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 11 # ____ x,y: (356, 154) # ____ threshold: 99999 # ____ def mask radius: 4.0 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: tracking1 # ____ aperture size: 11 # ____ x,y: (460, 283) # ____ threshold: 46 # ____ def mask radius: 4.0 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: tracking2 # ____ aperture size: 11 # ____ x,y: (135, 219) # ____ threshold: 46 # ____ def mask radius: 4.0 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 3 # # aperture name: nostar # ____ aperture size: 11 # ____ x,y: (317, 182) # ____ threshold: 99999 # ____ def mask radius: 4.0 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 4 # ==================== end header lines ==================== timeDelta: 0.0333662 seconds per reading timestamp error rate: 0.0575% Block integration started at entry 14841 with block size of 16 readings timeDelta: 0.533859 seconds per block timestamp error rate: 0.089% nostar is selected as the reference curve for normalization. D zone selected: [2569, 2664] R zone selected: [2666, 2768] Locate a "D and R" event has been selected Number of candidate solutions: 9888 (using D/R region selections) New solver results... Integer (non-subframe) solution... sigB:95.23 sigA:91.04 B:6620.94 A:6529.53 in entryNum units: D: 2631 R: 2680 noise corr coefs: [1.00] (based on 3318 points) sigmaB: 91.64 Subframe adjusted solution... sigB:91.64 sigA:89.22 B:6620.94 A:6529.53 in entryNum units: D: 2631 R: 2680 D(subframe): 2631.0000 R(subframe): 2680.0000 in frameNum units: D: 42105 R: 42889 D(subframe): 42105.0000 R(subframe): 42889.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -47.5548 hiDbar @ .68 ci: 45.1391 loDbar @ .95 ci: -176.2800 hiDbar @ .95 ci: 173.2374 loDbar @ .9973 ci: -423.6799 hiDbar @ .9973 ci: 440.5112 loDurBar @ .68 ci: -81.9018 hiDurBar @ .68 ci: 83.8882 loDurBar @ .95 ci: -240.0877 hiDurBar @ .95 ci: 248.6103 loDurBar @ .9973 ci: -544.3103 hiDurBar @ .9973 ci: 517.2005 Timestamp validity check ... From timestamps at D and R, calculated 49 reading blocks. From reading blocks, calculated 49 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 6620.94 {+/- 1.59} sigmaB: 91.64 A: 6529.53 {+/- 12.88} sigmaA: 89.22 magDrop: 0.015 +/- 0.002 (0.68 ci) snr: 1.00 D: 42105.00 {+46.35,-46.35} (frame number) D: [06:45:34.2882] {+1.5464,-1.5464} seconds R: 42889.00 {+46.35,-46.35} (frame number) R: [06:46:00.4472] {+1.5464,-1.5464} seconds Duration (R - D): 784.0000 {+82.8950,-82.8950} readings Duration (R - D): 26.1590 {+2.7659,-2.7659} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 6620.94 {+/- 3.18} sigmaB: 91.64 A: 6529.53 {+/- 25.75} sigmaA: 89.22 magDrop: 0.015 +/- 0.004 (0.95 ci) snr: 1.00 D: 42105.00 {+174.76,-174.76} (frame number) D: [06:45:34.2882] {+5.8310,-5.8310} seconds R: 42889.00 {+174.76,-174.76} (frame number) R: [06:46:00.4472] {+5.8310,-5.8310} seconds Duration (R - D): 784.0000 {+244.3490,-244.3490} readings Duration (R - D): 26.1590 {+8.1530,-8.1530} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 6620.94 {+/- 4.77} sigmaB: 91.64 A: 6529.53 {+/- 38.63} sigmaA: 89.22 magDrop: 0.015 +/- 0.006 (0.9973 ci) snr: 1.00 D: 42105.00 {+432.10,-432.10} (frame number) D: [06:45:34.2882] {+14.4174,-14.4174} seconds R: 42889.00 {+432.10,-432.10} (frame number) R: [06:46:00.4472] {+14.4174,-14.4174} seconds Duration (R - D): 784.0000 {+530.7554,-530.7554} readings Duration (R - D): 26.1590 {+17.7093,-17.7093} seconds =============== end 0.9973 containment interval report ============= D frame number: 42105.00 D: 0.6800 containment intervals: {+/- 47.55} (readings) D: 0.9500 containment intervals: {+/- 176.28} (readings) D: 0.9973 containment intervals: {+/- 440.51} (readings) R frame number: 42889.00 R: 0.6800 containment intervals: {+/- 47.55} (readings) R: 0.9500 containment intervals: {+/- 176.28} (readings) R: 0.9973 containment intervals: {+/- 440.51} (readings) Duration (R - D): 784.0000 readings Duration: 0.6800 containment intervals: {+/- 82.8950} (readings) Duration: 0.9500 containment intervals: {+/- 244.3490} (readings) Duration: 0.9973 containment intervals: {+/- 530.7554} (readings) =============== Summary report for Excel file ===================== Block integration of size 16 has been applied to this light curve. This light curve has been normalized against a reference star. ... nostar was used for normalization with X offset: 0 ... 45 readings were used for smoothing The following lightcurve parameters were utilized: ==== use diff: is checked ==== exp: 0.533859 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: 0.015 +/- 0.004 (0.95 ci) snr: 1.00 D time: [06:45:34.2882] D: 0.6800 containment intervals: {+/- 1.5464} seconds D: 0.9500 containment intervals: {+/- 5.8310} seconds D: 0.9973 containment intervals: {+/- 14.4174} seconds R time: [06:46:00.4472] R: 0.6800 containment intervals: {+/- 1.5464} seconds R: 0.9500 containment intervals: {+/- 5.8310} seconds R: 0.9973 containment intervals: {+/- 14.4174} seconds Duration (R - D): 26.1590 seconds Duration: 0.6800 containment intervals: {+/- 2.7659} seconds Duration: 0.9500 containment intervals: {+/- 8.1530} seconds Duration: 0.9973 containment intervals: {+/- 17.7093} 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