+--------------------------------+ +--------------------------------+ ASTERIODAL OCCULTATION - REPORT FORM +--------------------------------+ +--------------------------------+ EAON & IOTA-ES EUROPEAN ASTEROIDAL OCCULTATION NETWORK INTERNATIONAL OCCULTATION TIMING ASSOCIATION EUROPEAN SECTION +--------------------------------+ +--------------------------------+ 1. DATE: 31 Dec 2016 STAR: 4U 545-29824 ASTEROID: (1076) Viola 2. OBSERVER Name: Stefano SPOSETTI Address: 6525 GNOSCA - Switzerland Email: stefanosposetti@ticino.com 3. OBSERVING STATION Nearest city: CH-6525 Gnosca Longitude: 9d 1m 26.5s (E) Latitude: 46d 13m 53.2s (N) Altitude: 260m (WGS84) 4. TIMING OF EVENTS Occultation recorded: POSITIVE Type of event: "S"tart observation; "I"nterrupt-start; "D"isappearance; "B"link; "F"lash; "E"nd observation; "I"nterrupt-end; "R"eappearance; "O"ther (specify) Personal Equation Substracted: No Event Time (UTC) Accuracy + Comments code: HH:MM:SS.ss S.sss -S : 22:03:57 -D : 22:12:22.35 ± 0.04 s -R : 22:12:23.55 ± 0.04 s -E : 22:17:06 Duration: 1.20 s ± 0.08 s TELESCOPE -Type: Schmidt-Cassegrain, Celestron 11-inch -Aperture: 280 mm -Focal length: 930 mm (with focal reducer) -FOV: about 23x18 arcmin -Mount: Equatorial -Motor drive: Yes 6. TIMING & RECORDING Sensor/Camera: Videocamera WAT-910HX, CCIR, 1/2", ICX429ALL sensor Videocamera settings: Shutter = x4; Gain = 41/41; Gamma = 1.00 Device of recording: Personal computer, Imaging Source DFG/SV1 PCI grabber, composite input, Virtualdub software, saved as uncompressed file on Harddisk Timekeeping: GPS 1PPS (US Global Sat EM-406A) Time insertion device: IOTA-VTI, v.1.1.42 Integration time: 0.080 s 7. OBSERVING CONDITIONS Atmospheric transparency: good Wind: no Star image stability: good Minor Planet Visible: - 8. ADDITIONAL COMMENTS -Target position at: azimut = 147 deg; elevation = 59 deg -Moonlight: none Accordingly to Occultwatcher prediction (IBEROC feed): -Rank: 31 -Probability: 8.7 % -Lightdrop: 1.6 mag -Max duration: 2.7 s -Event time: 22:12:21 UT -Error in time: 6 s -Tangra v. 3.6 was used to generate the lightcurve (aperture photometry, average background). -A correction of - 0.060 s was applied because of the use of an integration camera. -Measured lightdrop: 1.5 mag. -A lightcurve can be seen here: http://sposetti.ch/wp-content/uploads/2014/09/2016DEC31_Viola.png