#################### PYOTE 5.1.2 session started: Sat May 18 20:21:03 2024 #################### filename: C:\Users\aschw\Desktop\DvtiData\20240517_220939_408x310_G30dBD_0050ms\pymovie_oc.csv If the csv file came from PyMovie - columns with prefix: signal will be read. ==================== file header lines ==================== # PyMovie Version 4.0.6 # source: C:\Users\aschw\Desktop\DvtiData\20240517_220939_408x310_G30dBD_0050ms.adv # # Aperture photometry was used to extract the lightcurves # # lunar background: False # yellow mask = default: False # # aperture name: target # ____ aperture size: 31 # ____ x,y: (194, 160) at frame 1199 # ____ threshold: 250 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 0 # # aperture name: ref1 # ____ aperture size: 31 # ____ x,y: (155, 193) at frame 1199 # ____ threshold: 252 # ____ def mask radius: 3.2 # ____ color: red # ____ joggable: False # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 1 # # aperture name: ref2 # ____ aperture size: 31 # ____ x,y: (81, 138) at frame 1199 # ____ threshold: 252 # ____ def mask radius: 3.2 # ____ color: yellow # ____ joggable: True # ____ auto textOut: False # ____ thumbnail source: False # ____ csv output order: 2 # # date at frame 0: 2024-05-17 #ACQUISITION-DELAY: 0.0 #ALTITUDE: 545.9 #AUTHOR: Andreas SCHWEIZER #BINNING-X: 4 #BINNING-Y: 4 #CAMERA-DRIVER-NAME: UVC #CAMERA-FIRMWARE-VERSION: 1.2.0 #CAMERA-MODEL: DVTI+CAM #CAMERA-SENSOR-INFO: Sony IMX430LLJ-C (1.1" 1624x1240 4.5um CIS) #CAMERA-SERIAL-NO: 61 #CAMERA-VENDOR-NAME: DVTI #COMMENT: #HEIGHT: 310 #INSTRUMENT: DVTI+CAM #61 FW 1.2.0, Sensor IMX430 #LATITUDE: 47.5195973 #LONGITUDE: 8.5707320 #OBJNAME: #OBSERVER: Andreas SCHWEIZER #RECORDER-SOFTWARE: DvtiCamControl #RECORDER-SOFTWARE-VERSION: 5.8.1-51 #TELESCOPE: 50cm Newton #WIDTH: 408 # # Aperture photometry was used to extract the lightcurves ==================== end header lines ==================== No time step irregularities found. timeDelta: 0.0500000 seconds per reading timestamp error rate: 0.00% Home directory: C:\Users\aschw\AppData\Local\Packages\PythonSoftwareFoundation.Python.3.10_qbz5n2kfra8p0\LocalCache\local-packages\Python310\site-packages\pyoteapp We found C:\Users\aschw\Documents\model-examples already present. Adding any new examples ... D zone selected: [522, 591] R zone selected: [593, 671] Locate a "D and R" event has been selected Number of candidate solutions: 5530 (using D/R region selections) New solver results... Integer (non-subframe) solution... sigB:1783.85 sigA:1009.75 B:6129.34 A:362.56 in entryNum units: D: 588 R: 597 noise corr coefs: [1.00, 0.188] (based on 1191 points) sigmaB: 1767.19 Subframe adjusted solution... sigB:1767.19 sigA:1767.19 B:6129.34 A:362.56 in entryNum units: D: 588 R: 597 D(subframe): 588.0000 R(subframe): 597.0000 in frameNum units: D: 588 R: 597 D(subframe): 588.0000 R(subframe): 597.0000 ... end New solver results Error bar report based on 100,000 simulations (units are readings)... loDbar @ .68 ci: -0.3748 hiDbar @ .68 ci: 0.3730 loDbar @ .95 ci: -1.0380 hiDbar @ .95 ci: 1.1044 loDbar @ .9973 ci: -3.4511 hiDbar @ .9973 ci: 3.3169 loDurBar @ .68 ci: -0.6087 hiDurBar @ .68 ci: 0.5824 loDurBar @ .95 ci: -1.6408 hiDurBar @ .95 ci: 1.6734 loDurBar @ .9973 ci: -4.2403 hiDurBar @ .9973 ci: 3.8980 Timestamp validity check ... From timestamps at D and R, calculated 9 reading blocks. From reading blocks, calculated 9 blocks. Timestamps appear valid @ D and R ================= 0.68 containment interval report ================= B: 6129.34 {+/- 51.23} sigmaB: 1767.19 A: 362.56 {+/- 624.79} sigmaA: 1767.19 magDrop report: percentDrop: 94.1 magDrop: 3.070 +/- 1.871 (0.68 ci) snr: 3.26 D: 588.00 {+0.37,-0.37} (frame number) D: [22:10:08.7980] {+0.0187,-0.0187} seconds R: 597.00 {+0.37,-0.37} (frame number) R: [22:10:09.2480] {+0.0187,-0.0187} seconds Duration (R - D): 9.0000 {+0.5955,-0.5955} readings Duration (R - D): 0.4500 {+0.0298,-0.0298} seconds =============== end 0.68 containment interval report =============== ================= 0.95 containment interval report ================= B: 6129.34 {+/- 102.46} sigmaB: 1767.19 A: 362.56 {+/- 1249.59} sigmaA: 1767.19 magDrop report: percentDrop: 94.1 magDrop: 3.070 too much noise; cannot calculate error bars snr: 3.26 D: 588.00 {+1.07,-1.07} (frame number) D: [22:10:08.7980] {+0.0536,-0.0536} seconds R: 597.00 {+1.07,-1.07} (frame number) R: [22:10:09.2480] {+0.0536,-0.0536} seconds Duration (R - D): 9.0000 {+1.6571,-1.6571} readings Duration (R - D): 0.4500 {+0.0829,-0.0829} seconds =============== end 0.95 containment interval report =============== ================= 0.9973 containment interval report =============== B: 6129.34 {+/- 153.68} sigmaB: 1767.19 A: 362.56 {+/- 1874.38} sigmaA: 1767.19 magDrop report: percentDrop: 94.1 magDrop: 3.070 too much noise; cannot calculate error bars snr: 3.26 D: 588.00 {+3.38,-3.38} (frame number) D: [22:10:08.7980] {+0.1692,-0.1692} seconds R: 597.00 {+3.38,-3.38} (frame number) R: [22:10:09.2480] {+0.1692,-0.1692} seconds Duration (R - D): 9.0000 {+4.0692,-4.0692} readings Duration (R - D): 0.4500 {+0.2035,-0.2035} seconds =============== end 0.9973 containment interval report ============= D frame number: 588.00 D: 0.6800 containment intervals: {+/- 0.37} (readings) D: 0.9500 containment intervals: {+/- 1.10} (readings) D: 0.9973 containment intervals: {+/- 3.45} (readings) R frame number: 597.00 R: 0.6800 containment intervals: {+/- 0.37} (readings) R: 0.9500 containment intervals: {+/- 1.10} (readings) R: 0.9973 containment intervals: {+/- 3.45} (readings) Duration (R - D): 9.0000 readings Duration: 0.6800 containment intervals: {+/- 0.5955} (readings) Duration: 0.9500 containment intervals: {+/- 1.6571} (readings) Duration: 0.9973 containment intervals: {+/- 4.0692} (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: 94.1 magDrop: 3.070 too much noise; cannot calculate error bars snr: 3.26 D time: [22:10:08.7980] D: 0.6800 containment intervals: {+/- 0.0187} seconds D: 0.9500 containment intervals: {+/- 0.0536} seconds D: 0.9973 containment intervals: {+/- 0.1692} seconds R time: [22:10:09.2480] R: 0.6800 containment intervals: {+/- 0.0187} seconds R: 0.9500 containment intervals: {+/- 0.0536} seconds R: 0.9973 containment intervals: {+/- 0.1692} seconds Duration (R - D): 0.4500 seconds Duration: 0.6800 containment intervals: {+/- 0.0298} seconds Duration: 0.9500 containment intervals: {+/- 0.0829} seconds Duration: 0.9973 containment intervals: {+/- 0.2035} 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: Sat May 18 20:23:19 2024 ####################