#################### PYOTE 4.8.4 session started: Sat Jul 30 16:37:31 2022 #################### filename: /Volumes/MY PASSPORT/astro/occultations/20220723_90_Antiope/20220723_90_Antiope_Bender/20220723_90_Antiope_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 8270 frames ==================== file header lines ==================== # PyMovie Version 3.4.2 # source: /Volumes/MY PASSPORT/astro/occultations/20220723_90_Antiope/20220723_90_Antiope_Bender.avi # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 21 # ____ x,y: (276, 192) # ____ threshold: 6 # ____ def mask radius: 6.8 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: nostar # ____ aperture size: 21 # ____ x,y: (313, 149) # ____ threshold: 99999 # ____ def mask radius: 6.8 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: tracking1 # ____ aperture size: 21 # ____ x,y: (55, 156) # ____ threshold: 9 # ____ def mask radius: 6.8 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: tracking2 # ____ aperture size: 21 # ____ x,y: (394, 283) # ____ threshold: 9 # ____ def mask radius: 6.8 # ____ color: yellow # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 3 # ==================== end header lines ==================== timeDelta: 0.0333662 seconds per reading timestamp error rate: 0.00% #################### PYOTE 4.8.4 session started: Sat Jul 30 16:37:37 2022 #################### filename: /Volumes/MY PASSPORT/astro/occultations/20220723_90_Antiope/20220723_90_Antiope_Bender/20220723_90_Antiope_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 8270 frames ==================== file header lines ==================== # PyMovie Version 3.4.2 # source: /Volumes/MY PASSPORT/astro/occultations/20220723_90_Antiope/20220723_90_Antiope_Bender.avi # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 21 # ____ x,y: (276, 192) # ____ threshold: 6 # ____ def mask radius: 6.8 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: nostar # ____ aperture size: 21 # ____ x,y: (313, 149) # ____ threshold: 99999 # ____ def mask radius: 6.8 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: tracking1 # ____ aperture size: 21 # ____ x,y: (55, 156) # ____ threshold: 9 # ____ def mask radius: 6.8 # ____ color: yellow # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: tracking2 # ____ aperture size: 21 # ____ x,y: (394, 283) # ____ threshold: 9 # ____ def mask radius: 6.8 # ____ color: yellow # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 3 # ==================== end header lines ==================== timeDelta: 0.0333662 seconds per reading timestamp error rate: 0.00% Block integration started at entry 417 with block size of 8 readings timeDelta: 0.266929 seconds per block timestamp error rate: 0.0% Data trimmed/selected using points: [0, 643] Use min/max event to locate a "D and R" event has been selected Use min/max event to locate a "D and R" event has been selected minEvent: 5 maxEvent: 100 Number of candidate solutions: 56688 (using event min/max entries) New solver results... Integer (non-subframe) solution... sigB:188.72 sigA:191.61 B:1572.97 A:1383.26 in entryNum units: D: 309 R: 344 noise corr coefs: [1.00] (based on 609 points) sigmaB: 187.05 Subframe adjusted solution... sigB:187.05 sigA:190.79 B:1572.97 A:1383.26 in entryNum units: D: 309 R: 344 D(subframe): 309.0000 R(subframe): 344.0000 in frameNum units: D: 2473 R: 2753 D(subframe): 2473.0000 R(subframe): 2753.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -23.2315 hiDbar @ .68 ci: 23.5131 loDbar @ .95 ci: -87.0247 hiDbar @ .95 ci: 89.2065 loDbar @ .9973 ci: -223.5883 hiDbar @ .9973 ci: 213.7191 loDurBar @ .68 ci: -41.7456 hiDurBar @ .68 ci: 42.1286 loDurBar @ .95 ci: -123.8630 hiDurBar @ .95 ci: 123.4137 loDurBar @ .9973 ci: -269.9060 hiDurBar @ .9973 ci: 260.3540 Timestamp validity check ... From timestamps at D and R, calculated 35 reading blocks. From reading blocks, calculated 35 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 1572.97 {+/- 7.59} sigmaB: 187.05 A: 1383.26 {+/- 32.72} sigmaA: 190.79 magDrop: 0.140 +/- 0.026 (0.68 ci) snr: 1.01 D: 2473.00 {+23.37,-23.37} (frame number) D: [09:49:21.9810] {+0.7798,-0.7798} seconds R: 2753.00 {+23.37,-23.37} (frame number) R: [09:49:31.3235] {+0.7798,-0.7798} seconds Duration (R - D): 280.0000 {+41.9371,-41.9371} readings Duration (R - D): 9.3425 {+1.3993,-1.3993} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 1572.97 {+/- 15.17} sigmaB: 187.05 A: 1383.26 {+/- 65.44} sigmaA: 190.79 magDrop: 0.140 +/- 0.052 (0.95 ci) snr: 1.01 D: 2473.00 {+88.12,-88.12} (frame number) D: [09:49:21.9810] {+2.9401,-2.9401} seconds R: 2753.00 {+88.12,-88.12} (frame number) R: [09:49:31.3235] {+2.9401,-2.9401} seconds Duration (R - D): 280.0000 {+123.6384,-123.6384} readings Duration (R - D): 9.3425 {+4.1253,-4.1253} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 1572.97 {+/- 22.76} sigmaB: 187.05 A: 1383.26 {+/- 98.16} sigmaA: 190.79 magDrop: 0.140 +/- 0.079 (0.9973 ci) snr: 1.01 D: 2473.00 {+218.65,-218.65} (frame number) D: [09:49:21.9810] {+7.2956,-7.2956} seconds R: 2753.00 {+218.65,-218.65} (frame number) R: [09:49:31.3235] {+7.2956,-7.2956} seconds Duration (R - D): 280.0000 {+265.1300,-265.1300} readings Duration (R - D): 9.3425 {+8.8464,-8.8464} seconds =============== end 0.9973 containment interval report ============= D frame number: 2473.00 D: 0.6800 containment intervals: {+/- 23.51} (readings) D: 0.9500 containment intervals: {+/- 89.21} (readings) D: 0.9973 containment intervals: {+/- 223.59} (readings) R frame number: 2753.00 R: 0.6800 containment intervals: {+/- 23.51} (readings) R: 0.9500 containment intervals: {+/- 89.21} (readings) R: 0.9973 containment intervals: {+/- 223.59} (readings) Duration (R - D): 280.0000 readings Duration: 0.6800 containment intervals: {+/- 41.9371} (readings) Duration: 0.9500 containment intervals: {+/- 123.6384} (readings) Duration: 0.9973 containment intervals: {+/- 265.1300} (readings) =============== Summary report for Excel file ===================== Block integration of size 8 has been applied to this light curve. This light curve has been trimmed. The following lightcurve parameters were utilized: ==== use diff: is checked ==== exp: 0.266929 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: 0.140 +/- 0.052 (0.95 ci) snr: 1.01 D time: [09:49:21.9810] D: 0.6800 containment intervals: {+/- 0.7798} seconds D: 0.9500 containment intervals: {+/- 2.9401} seconds D: 0.9973 containment intervals: {+/- 7.2956} seconds R time: [09:49:31.3235] R: 0.6800 containment intervals: {+/- 0.7798} seconds R: 0.9500 containment intervals: {+/- 2.9401} seconds R: 0.9973 containment intervals: {+/- 7.2956} seconds Duration (R - D): 9.3425 seconds Duration: 0.6800 containment intervals: {+/- 1.3993} seconds Duration: 0.9500 containment intervals: {+/- 4.1253} seconds Duration: 0.9973 containment intervals: {+/- 8.8464} 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 Excel spreadsheet Asteroid Report Form entries made successfully. #################### Session ended: Sat Jul 30 16:55:59 2022 ####################