#################### PYOTE 3.9.4 session started: Sat Oct 30 07:01:46 2021 #################### filename: E:/Eurybates_Nolthenius/20211020_3548_Eurybates_Nolthenius_Moore.csv Unexpected file type of .fit found. Analyze light curve 1 selected. PyMovie aperture name: Target ==================== file header lines ==================== # PyMovie Version 3.2.4 # source: E:/Eurybates_Nolthenius/enhanced-image-19.fit # # lunar background: False # yellow mask = default: False # # aperture name: Target # ____ aperture size: 11 # ____ x,y: (298, 274) # ____ threshold: 99999 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: Track # ____ aperture size: 11 # ____ x,y: (124, 213) # ____ threshold: 36 # ____ def mask radius: 2.8 # ____ color: yellow # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 2 # ==================== end header lines ==================== timeDelta: 0.0333663 seconds per reading timestamp error rate: 0.00% Analyze light curve 1 selected. PyMovie aperture name: Target Block integration started at entry 244 with block size of 8 readings timeDelta: 0.266932 seconds per block timestamp error rate: 0.0% #################### Session ended: Sat Oct 30 07:02:38 2021 #################### #################### PYOTE 3.9.4 session started: Sat Oct 30 07:09:06 2021 #################### filename: E:/Eurybates_Nolthenius/20211020_3548_Eurybates_Nolthenius_Moore.csv Unexpected file type of .fit found. Analyze light curve 1 selected. PyMovie aperture name: Target ==================== file header lines ==================== # PyMovie Version 3.2.4 # source: E:/Eurybates_Nolthenius/enhanced-image-2449.fit # # lunar background: False # yellow mask = default: False # # aperture name: Target # ____ aperture size: 11 # ____ x,y: (297, 271) # ____ threshold: 99999 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: Track # ____ aperture size: 11 # ____ x,y: (124, 212) # ____ threshold: 34 # ____ def mask radius: 2.8 # ____ color: yellow # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 1 # ==================== end header lines ==================== timeDelta: 0.0333663 seconds per reading timestamp error rate: 17.3% Analyze light curve 1 selected. PyMovie aperture name: Target Block integration started at entry 220 with block size of 8 readings timeDelta: 0.266933 seconds per block timestamp error rate: 18% #################### Session ended: Sat Oct 30 07:10:43 2021 #################### #################### PYOTE 3.9.4 session started: Sun Oct 31 17:46:36 2021 #################### filename: E:/Eurybates_Nolthenius/20211020_3548_Eurybates_Nolthenius_Moore.csv Unexpected file type of .fit found. Analyze light curve 1 selected. PyMovie aperture name: Target ==================== file header lines ==================== # PyMovie Version 3.2.4 # source: E:/Eurybates_Nolthenius/enhanced-image-2449.fit # # lunar background: False # yellow mask = default: False # # aperture name: Target # ____ aperture size: 11 # ____ x,y: (297, 271) # ____ threshold: 99999 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: Track # ____ aperture size: 11 # ____ x,y: (124, 212) # ____ threshold: 34 # ____ def mask radius: 2.8 # ____ color: yellow # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 1 # ==================== end header lines ==================== timeDelta: 0.0333663 seconds per reading timestamp error rate: 17.3% Analyze light curve 1 selected. PyMovie aperture name: Target Block integration started at entry 228 with block size of 8 readings timeDelta: 0.266933 seconds per block timestamp error rate: 18% #################### Session ended: Sun Oct 31 17:58:23 2021 #################### #################### PYOTE 3.9.9 session started: Mon Nov 1 17:55:47 2021 #################### filename: E:/Eurybates_Nolthenius/20211020_3548_Eurybates_Nolthenius_Moore.csv Unexpected file type of .fit found. Analyze light curve 1 selected. PyMovie aperture name: Target ==================== file header lines ==================== # PyMovie Version 3.2.4 # source: E:/Eurybates_Nolthenius/enhanced-image-2449.fit # # lunar background: False # yellow mask = default: False # # aperture name: Target # ____ aperture size: 11 # ____ x,y: (297, 271) # ____ threshold: 99999 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: Track # ____ aperture size: 11 # ____ x,y: (124, 212) # ____ threshold: 34 # ____ def mask radius: 2.8 # ____ color: yellow # ____ joggable: True # ____ auto textOut: True # ____ thumbnail source: True # ____ csv output order: 1 # ==================== end header lines ==================== timeDelta: 0.0333663 seconds per reading timestamp error rate: 17.3% Analyze light curve 1 selected. PyMovie aperture name: Target Block integration started at entry 268 with block size of 8 readings timeDelta: 0.266933 seconds per block timestamp error rate: 18% Data trimmed/selected using points: [0, 77] D zone selected: [64, 75] Locate a "D only" event triggered minEvent: maxEvent: Number of candidate solutions: 12 (using D/R region selections) New solver results... Integer (non-subframe) solution... sigB:110.28 sigA:92.58 B:380.01 A:-5.28 in entryNum units: D: 72 noise corr coefs: [1.00] (based on 72 points) sigmaB: 108.65 Subframe adjusted solution... sigB:108.65 sigA:108.65 B:380.01 A:-5.28 in entryNum units: D: 72 D(subframe): 72.5039 in frameNum units: D: 3029 D(subframe): 3033.0310 Unsupported file extension: .fit ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -2.6939 hiDbar @ .68 ci: 2.6436 loDbar @ .95 ci: -7.0119 hiDbar @ .95 ci: 6.9312 loDbar @ .9973 ci: -16.8999 hiDbar @ .9973 ci: 17.4266 loDurBar @ .68 ci: -4.1292 hiDurBar @ .68 ci: 4.1517 loDurBar @ .95 ci: -9.8089 hiDurBar @ .95 ci: 9.9357 loDurBar @ .9973 ci: -20.8253 hiDurBar @ .9973 ci: 20.9784 ================= 0.68 confidence interval report ================= B: 380.01 {+/- 12.76} sigmaB: 108.65 A: -5.28 {+/- 58.11} sigmaA: 108.65 minimum magDrop: > 2.00 nominal magDrop: > 2.04 maximum magDrop: > 2.07 snr: 3.55 D: 3033.03 {+2.67,-2.67} (frame number) D: [11:59:50.4940] {+0.0890,-0.0890} seconds =============== end 0.68 confidence interval report =============== ================= 0.95 confidence interval report ================= B: 380.01 {+/- 25.52} sigmaB: 108.65 A: -5.28 {+/- 116.22} sigmaA: 108.65 minimum magDrop: 1.26 nominal magDrop: > 2.04 maximum magDrop: > 2.11 snr: 3.55 D: 3033.03 {+6.97,-6.97} (frame number) D: [11:59:50.4940] {+0.2326,-0.2326} seconds =============== end 0.95 confidence interval report =============== ================= 0.9973 confidence interval report =============== B: 380.01 {+/- 38.28} sigmaB: 108.65 A: -5.28 {+/- 174.32} sigmaA: 108.65 minimum magDrop: 0.76 nominal magDrop: > 2.04 maximum magDrop: > 2.14 snr: 3.55 D: 3033.03 {+17.16,-17.16} (frame number) D: [11:59:50.4940] {+0.5727,-0.5727} seconds =============== end 0.9973 confidence interval report ============= D frame number: 3033.03 D: 0.6800 confidence intervals: {+/- 2.68} (readings) D: 0.9500 confidence intervals: {+/- 7.00} (readings) D: 0.9973 confidence intervals: {+/- 17.44} (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: 0.266933 This 'drop' has a 0.0000 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 timestamps are treated as being start-of-exposure times. 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. nominal magDrop: > 2.04 snr: 3.55 D time: [11:59:50.4940] D: 0.6800 confidence intervals: {+/- 0.0896} seconds D: 0.9500 confidence intervals: {+/- 0.2336} seconds D: 0.9973 confidence intervals: {+/- 0.5818} seconds Enter D and R error bars for each confidence 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 confidence interval error bars