#################### PYOTE 5.1.0 session started: Tue Nov 19 16:08:32 2024 #################### filename: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2024_11_18_(718) Erida\Capture 2024-11-18T00_59_56Z\6 nested apertures.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_11_18_(718) Erida\Capture 2024-11-18T00_59_56Z.adv # # Aperture photometry was used to extract the lightcurves # # lunar background: False # yellow mask = default: False # # aperture name: dynamic-nest1-thresh-1417 # ____ aperture size: 31 # ____ x,y: (320, 170) at frame 500 # ____ threshold: 1417 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: dynamic-nest1-thresh-1617 # ____ aperture size: 31 # ____ x,y: (320, 170) at frame 500 # ____ threshold: 1617 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # aperture name: dynamic-nest1-thresh-1817 # ____ aperture size: 31 # ____ x,y: (319, 170) at frame 500 # ____ threshold: 1817 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 3 # # aperture name: dynamic-nest1-thresh-2017 # ____ aperture size: 31 # ____ x,y: (320, 170) at frame 500 # ____ threshold: 2017 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 4 # # aperture name: dynamic-nest1-thresh-2217 # ____ aperture size: 31 # ____ x,y: (319, 170) at frame 500 # ____ threshold: 2217 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 5 # # aperture name: dynamic-nest1-thresh-2417 # ____ aperture size: 31 # ____ x,y: (319, 170) at frame 500 # ____ threshold: 2417 # ____ def mask radius: 3.2 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 6 # # aperture name: reference # ____ aperture size: 31 # ____ x,y: (93, 137) at frame 500 # ____ threshold: 2745 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: True # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 7 # # date at frame 0: 2024-11-18 #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: 46.231451166666666 #LONGITUDE: 9.024065 #POSITION-REFERENCE: WGS84 #RECORDER-SOFTWARE: SharpCap #RECORDER-SOFTWARE-VERSION: 4.1.12196.0 #WIDTH: 480 #TIME-SOURCE: Camera GPS # # Aperture photometry was used to extract the lightcurves ==================== end header lines ==================== No time step irregularities found. timeDelta: 0.400150 seconds per reading timestamp error rate: 0.00% 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 ... signal-dynamic-nest1-thresh-1617 is the target curve. signal-dynamic-nest1-thresh-1817 is the target curve. signal-dynamic-nest1-thresh-2417 is the target curve. 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: 6 maxEvent: 20 Number of candidate solutions: 3705 (using event min/max entries) New solver results... Integer (non-subframe) solution... sigB:29157.12 sigA:18289.52 B:111884.38 A:40117.50 in entryNum units: D: 108 R: 120 noise corr coefs: [1.00] (based on 249 points) sigmaB: 28219.17 Subframe adjusted solution... sigB:28219.17 sigA:16554.88 B:111884.38 A:40117.50 in entryNum units: D: 108 R: 120 D(subframe): 108.0000 R(subframe): 120.0000 in frameNum units: D: 348 R: 360 D(subframe): 348.0000 R(subframe): 360.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.3704 hiDbar @ .68 ci: 0.3661 loDbar @ .95 ci: -1.1126 hiDbar @ .95 ci: 0.8855 loDbar @ .9973 ci: -2.6808 hiDbar @ .9973 ci: 2.3149 loDurBar @ .68 ci: -0.6023 hiDurBar @ .68 ci: 0.5600 loDurBar @ .95 ci: -1.4383 hiDurBar @ .95 ci: 1.4417 loDurBar @ .9973 ci: -3.1878 hiDurBar @ .9973 ci: 2.9502 Timestamp validity check ... From timestamps at D and R, calculated 12 reading blocks. From reading blocks, calculated 12 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 111884.38 {+/- 1791.92} sigmaB: 28219.17 A: 40117.50 {+/- 4991.48} sigmaA: 16554.88 magDrop report: percentDrop: 64.1 magDrop: 1.114 +/- 0.136 (0.68 ci) snr: 2.54 D: 348.00 {+0.37,-0.37} (frame number) D: [01:02:43.6205] {+0.1465,-0.1482} seconds R: 360.00 {+0.37,-0.37} (frame number) R: [01:02:48.4223] {+0.1482,-0.1465} seconds Duration (R - D): 12.0000 {+0.5811,-0.5811} readings Duration (R - D): 4.8019 {+0.2325,-0.2325} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 111884.38 {+/- 3583.84} sigmaB: 28219.17 A: 40117.50 {+/- 9982.97} sigmaA: 16554.88 magDrop report: percentDrop: 64.1 magDrop: 1.114 +/- 0.272 (0.95 ci) snr: 2.54 D: 348.00 {+0.89,-1.11} (frame number) D: [01:02:43.6205] {+0.3543,-0.4452} seconds R: 360.00 {+1.11,-0.89} (frame number) R: [01:02:48.4223] {+0.4452,-0.3543} seconds Duration (R - D): 12.0000 {+1.4400,-1.4400} readings Duration (R - D): 4.8019 {+0.5762,-0.5762} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 111884.38 {+/- 5375.76} sigmaB: 28219.17 A: 40117.50 {+/- 14974.45} sigmaA: 16554.88 magDrop report: percentDrop: 64.1 magDrop: 1.114 +/- 0.409 (0.9973 ci) snr: 2.54 D: 348.00 {+2.31,-2.68} (frame number) D: [01:02:43.6205] {+0.9263,-1.0727} seconds R: 360.00 {+2.68,-2.31} (frame number) R: [01:02:48.4223] {+1.0727,-0.9263} seconds Duration (R - D): 12.0000 {+3.0690,-3.0690} readings Duration (R - D): 4.8019 {+1.2281,-1.2281} seconds =============== end 0.9973 containment interval report ============= D frame number: 348.00 D: 0.6800 containment intervals: {+/- 0.37} (readings) D: 0.9500 containment intervals: {+/- 1.11} (readings) D: 0.9973 containment intervals: {+/- 2.68} (readings) R frame number: 360.00 R: 0.6800 containment intervals: {+/- 0.37} (readings) R: 0.9500 containment intervals: {+/- 1.11} (readings) R: 0.9973 containment intervals: {+/- 2.68} (readings) Duration (R - D): 12.0000 readings Duration: 0.6800 containment intervals: {+/- 0.5811} (readings) Duration: 0.9500 containment intervals: {+/- 1.4400} (readings) Duration: 0.9973 containment intervals: {+/- 3.0690} (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: 64.1 magDrop: 1.114 +/- 0.272 (0.95 ci) snr: 2.54 D time: [01:02:43.6205] D: 0.6800 containment intervals: {+/- 0.1482} seconds D: 0.9500 containment intervals: {+/- 0.4452} seconds D: 0.9973 containment intervals: {+/- 1.0727} seconds R time: [01:02:48.4223] R: 0.6800 containment intervals: {+/- 0.1482} seconds R: 0.9500 containment intervals: {+/- 0.4452} seconds R: 0.9973 containment intervals: {+/- 1.0727} seconds Duration (R - D): 4.8019 seconds Duration: 0.6800 containment intervals: {+/- 0.2325} seconds Duration: 0.9500 containment intervals: {+/- 0.5762} seconds Duration: 0.9973 containment intervals: {+/- 1.2281} 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 signal-dynamic-nest1-thresh-1417 is the target curve. signal-dynamic-nest1-thresh-2417 is the target curve. signal-dynamic-nest1-thresh-1417 is the target curve. signal-dynamic-nest1-thresh-2417 is the target curve. signal-dynamic-nest1-thresh-1417 is the target curve. Use min/max event to locate a "D and R" event has been selected minEvent: 6 maxEvent: 20 Number of candidate solutions: 3705 (using event min/max entries) New solver results... Integer (non-subframe) solution... sigB:38663.52 sigA:20945.63 B:154792.98 A:42933.30 in entryNum units: D: 110 R: 120 noise corr coefs: [1.00] (based on 251 points) sigmaB: 38006.37 Subframe adjusted solution... sigB:38598.75 sigA:20945.63 B:155002.16 A:42933.30 in entryNum units: D: 109 R: 120 D(subframe): 109.5325 R(subframe): 120.0000 in frameNum units: D: 349 R: 360 D(subframe): 349.5325 R(subframe): 360.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.2955 hiDbar @ .68 ci: 0.3022 loDbar @ .95 ci: -0.8680 hiDbar @ .95 ci: 0.6938 loDbar @ .9973 ci: -2.1282 hiDbar @ .9973 ci: 1.3886 loDurBar @ .68 ci: -0.4639 hiDurBar @ .68 ci: 0.4610 loDurBar @ .95 ci: -1.0879 hiDurBar @ .95 ci: 1.1130 loDurBar @ .9973 ci: -2.3164 hiDurBar @ .9973 ci: 2.2275 Timestamp validity check ... From timestamps at D and R, calculated 11 reading blocks. From reading blocks, calculated 11 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 155002.16 {+/- 2443.49} sigmaB: 38598.75 A: 42933.30 {+/- 6807.31} sigmaA: 20945.63 magDrop report: percentDrop: 72.3 magDrop: 1.394 +/- 0.173 (0.68 ci) snr: 2.90 D: 349.53 {+0.30,-0.30} (frame number) D: [01:02:44.2337] {+0.1209,-0.1183} seconds R: 360.00 {+0.30,-0.30} (frame number) R: [01:02:48.4223] {+0.1183,-0.1209} seconds Duration (R - D): 10.4675 {+0.4624,-0.4624} readings Duration (R - D): 4.1886 {+0.1850,-0.1850} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 155002.16 {+/- 4886.97} sigmaB: 38598.75 A: 42933.30 {+/- 13614.63} sigmaA: 20945.63 magDrop report: percentDrop: 72.3 magDrop: 1.394 +/- 0.346 (0.95 ci) snr: 2.90 D: 349.53 {+0.69,-0.87} (frame number) D: [01:02:44.2337] {+0.2776,-0.3473} seconds R: 360.00 {+0.87,-0.69} (frame number) R: [01:02:48.4223] {+0.3473,-0.2776} seconds Duration (R - D): 10.4675 {+1.1005,-1.1005} readings Duration (R - D): 4.1886 {+0.4404,-0.4404} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 155002.16 {+/- 7330.46} sigmaB: 38598.75 A: 42933.30 {+/- 20421.94} sigmaA: 20945.63 magDrop report: percentDrop: 72.3 magDrop: 1.394 +/- 0.519 (0.9973 ci) snr: 2.90 D: 349.53 {+1.39,-2.13} (frame number) D: [01:02:44.2337] {+0.5557,-0.8516} seconds R: 360.00 {+2.13,-1.39} (frame number) R: [01:02:48.4223] {+0.8516,-0.5557} seconds Duration (R - D): 10.4675 {+2.2720,-2.2720} readings Duration (R - D): 4.1886 {+0.9091,-0.9091} seconds =============== end 0.9973 containment interval report ============= D frame number: 349.53 D: 0.6800 containment intervals: {+/- 0.30} (readings) D: 0.9500 containment intervals: {+/- 0.87} (readings) D: 0.9973 containment intervals: {+/- 2.13} (readings) R frame number: 360.00 R: 0.6800 containment intervals: {+/- 0.30} (readings) R: 0.9500 containment intervals: {+/- 0.87} (readings) R: 0.9973 containment intervals: {+/- 2.13} (readings) Duration (R - D): 10.4675 readings Duration: 0.6800 containment intervals: {+/- 0.4624} (readings) Duration: 0.9500 containment intervals: {+/- 1.1005} (readings) Duration: 0.9973 containment intervals: {+/- 2.2720} (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: 72.3 magDrop: 1.394 +/- 0.346 (0.95 ci) snr: 2.90 D time: [01:02:44.2337] D: 0.6800 containment intervals: {+/- 0.1209} seconds D: 0.9500 containment intervals: {+/- 0.3473} seconds D: 0.9973 containment intervals: {+/- 0.8516} seconds R time: [01:02:48.4223] R: 0.6800 containment intervals: {+/- 0.1209} seconds R: 0.9500 containment intervals: {+/- 0.3473} seconds R: 0.9973 containment intervals: {+/- 0.8516} seconds Duration (R - D): 4.1886 seconds Duration: 0.6800 containment intervals: {+/- 0.1850} seconds Duration: 0.9500 containment intervals: {+/- 0.4404} seconds Duration: 0.9973 containment intervals: {+/- 0.9091} 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: Tue Nov 19 16:17:11 2024 #################### #################### PYOTE 5.1.0 session started: Tue Nov 19 17:29:00 2024 #################### filename: E:\ASTRONOMIA\1-Immagini CCD\Occultazioni\2024_11_18_(718) Erida\Capture 2024-11-18T00_59_56Z\6 nested apertures.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_11_18_(718) Erida\Capture 2024-11-18T00_59_56Z.adv # # Aperture photometry was used to extract the lightcurves # # lunar background: False # yellow mask = default: False # # aperture name: dynamic-nest1-thresh-1424 # ____ aperture size: 31 # ____ x,y: (323, 171) at frame 530 # ____ threshold: 1424 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 17 # # aperture name: dynamic-nest1-thresh-1724 # ____ aperture size: 31 # ____ x,y: (323, 171) at frame 530 # ____ threshold: 1724 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 18 # # aperture name: dynamic-nest1-thresh-2024 # ____ aperture size: 31 # ____ x,y: (323, 171) at frame 530 # ____ threshold: 2024 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 19 # # aperture name: dynamic-nest1-thresh-2324 # ____ aperture size: 31 # ____ x,y: (323, 171) at frame 530 # ____ threshold: 2324 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 20 # # aperture name: dynamic-nest1-thresh-2624 # ____ aperture size: 31 # ____ x,y: (323, 171) at frame 530 # ____ threshold: 2624 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 21 # # aperture name: dynamic-nest1-thresh-2924 # ____ aperture size: 31 # ____ x,y: (323, 171) at frame 530 # ____ threshold: 2924 # ____ def mask radius: 3.2 # ____ color: green # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 22 # # aperture name: reference # ____ aperture size: 31 # ____ x,y: (54, 118) at frame 530 # ____ threshold: 2862 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: True # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 23 # # date at frame 0: 2024-11-18 #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: 46.231451166666666 #LONGITUDE: 9.024065 #POSITION-REFERENCE: WGS84 #RECORDER-SOFTWARE: SharpCap #RECORDER-SOFTWARE-VERSION: 4.1.12196.0 #WIDTH: 480 #TIME-SOURCE: Camera GPS # # Aperture photometry was used to extract the lightcurves ==================== end header lines ==================== No time step irregularities found. timeDelta: 0.400150 seconds per reading timestamp error rate: 0.00% 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: 5 maxEvent: 20 Number of candidate solutions: 5384 (using event min/max entries) New solver results... Integer (non-subframe) solution... sigB:39101.16 sigA:20255.84 B:156934.26 A:43463.90 in entryNum units: D: 169 R: 179 noise corr coefs: [1.00] (based on 340 points) sigmaB: 37799.13 Subframe adjusted solution... sigB:39066.98 sigA:20255.84 B:157079.60 A:43463.90 in entryNum units: D: 168 R: 179 D(subframe): 168.5658 R(subframe): 179.0000 in frameNum units: D: 349 R: 360 D(subframe): 349.5658 R(subframe): 360.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.2829 hiDbar @ .68 ci: 0.3055 loDbar @ .95 ci: -0.8462 hiDbar @ .95 ci: 0.6839 loDbar @ .9973 ci: -2.0094 hiDbar @ .9973 ci: 1.3498 loDurBar @ .68 ci: -0.4436 hiDurBar @ .68 ci: 0.4691 loDurBar @ .95 ci: -1.0844 hiDurBar @ .95 ci: 1.0648 loDurBar @ .9973 ci: -2.2289 hiDurBar @ .9973 ci: 2.2258 Timestamp validity check ... From timestamps at D and R, calculated 11 reading blocks. From reading blocks, calculated 11 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 157079.60 {+/- 2123.19} sigmaB: 39066.98 A: 43463.90 {+/- 6594.74} sigmaA: 20255.84 magDrop report: percentDrop: 72.3 magDrop: 1.395 +/- 0.165 (0.68 ci) snr: 2.91 D: 349.57 {+0.31,-0.28} (frame number) D: [01:02:44.2470] {+0.1223,-0.1132} seconds R: 360.00 {+0.28,-0.31} (frame number) R: [01:02:48.4223] {+0.1132,-0.1223} seconds Duration (R - D): 10.4342 {+0.4564,-0.4564} readings Duration (R - D): 4.1753 {+0.1826,-0.1826} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 157079.60 {+/- 4246.37} sigmaB: 39066.98 A: 43463.90 {+/- 13189.48} sigmaA: 20255.84 magDrop report: percentDrop: 72.3 magDrop: 1.395 +/- 0.331 (0.95 ci) snr: 2.91 D: 349.57 {+0.68,-0.85} (frame number) D: [01:02:44.2470] {+0.2737,-0.3386} seconds R: 360.00 {+0.85,-0.68} (frame number) R: [01:02:48.4223] {+0.3386,-0.2737} seconds Duration (R - D): 10.4342 {+1.0746,-1.0746} readings Duration (R - D): 4.1753 {+0.4300,-0.4300} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 157079.60 {+/- 6369.56} sigmaB: 39066.98 A: 43463.90 {+/- 19784.23} sigmaA: 20255.84 magDrop report: percentDrop: 72.3 magDrop: 1.395 +/- 0.496 (0.9973 ci) snr: 2.91 D: 349.57 {+1.35,-2.01} (frame number) D: [01:02:44.2470] {+0.5401,-0.8041} seconds R: 360.00 {+2.01,-1.35} (frame number) R: [01:02:48.4223] {+0.8041,-0.5401} seconds Duration (R - D): 10.4342 {+2.2273,-2.2273} readings Duration (R - D): 4.1753 {+0.8913,-0.8913} seconds =============== end 0.9973 containment interval report ============= D frame number: 349.57 D: 0.6800 containment intervals: {+/- 0.31} (readings) D: 0.9500 containment intervals: {+/- 0.85} (readings) D: 0.9973 containment intervals: {+/- 2.01} (readings) R frame number: 360.00 R: 0.6800 containment intervals: {+/- 0.31} (readings) R: 0.9500 containment intervals: {+/- 0.85} (readings) R: 0.9973 containment intervals: {+/- 2.01} (readings) Duration (R - D): 10.4342 readings Duration: 0.6800 containment intervals: {+/- 0.4564} (readings) Duration: 0.9500 containment intervals: {+/- 1.0746} (readings) Duration: 0.9973 containment intervals: {+/- 2.2273} (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: 72.3 magDrop: 1.395 +/- 0.331 (0.95 ci) snr: 2.91 D time: [01:02:44.2470] D: 0.6800 containment intervals: {+/- 0.1223} seconds D: 0.9500 containment intervals: {+/- 0.3386} seconds D: 0.9973 containment intervals: {+/- 0.8041} seconds R time: [01:02:48.4223] R: 0.6800 containment intervals: {+/- 0.1223} seconds R: 0.9500 containment intervals: {+/- 0.3386} seconds R: 0.9973 containment intervals: {+/- 0.8041} seconds Duration (R - D): 4.1753 seconds Duration: 0.6800 containment intervals: {+/- 0.1826} seconds Duration: 0.9500 containment intervals: {+/- 0.4300} seconds Duration: 0.9973 containment intervals: {+/- 0.8913} 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