+--------------------------------+ +--------------------------------+ ASTERIODAL OCCULTATION - REPORT FORM +--------------------------------+ +--------------------------------+ EAON & IOTA-ES EUROPEAN ASTEROIDAL OCCULTATION NETWORK INTERNATIONAL OCCULTATION TIMING ASSOCIATION EUROPEAN SECTION +--------------------------------+ +--------------------------------+ 1. DATE: 8 Oct 2016 STAR: TYC 5242-00199-1 ASTEROID: (67) Asia 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 : 21:26:28 -D : 21:31:14.02 ± 0.04 s -R : 21:31:21.14 ± 0.04 s -E : 21:36:30 Duration: 7.12 s ± 0.08 s 5. TELESCOPE Type: Newton Aperture: 420 mm Focal length: about 1000 mm (with focal reducer) Magnification: - Mount: Equatorial Motor drive: Yes 6. TIMING & RECORDING Timekeeping: GPS 1PPS (US Global Sat EM-406A) Camera: Videocamera WAT-902H Ultimate, 1/2" sensor, CCIR Camera settings: Gamma = OFF, Gain = LO Device of recording: Personal computer, Hauppauge HVR-1700 (PCIcard), S-video input, Virtualdub software, uncompressed AVI saved on Harddisk Integration time = 0.040 s Time insertion device: IOTA-VTI, v.1.1.42 7. OBSERVING CONDITIONS Atmospheric transparency: fair/bad Wind: no Star image stability: good Minor Planet Visible: yes 8. ADDITIONAL COMMENTS -Target position at azimut: 183 deg (South) and elevation 42 deg -No moonlight -Limiting naked eye luminosity around the target area: 3 mag. Accordingly to Occultwatcher prediction (IOTA feed): -Rank: 100 -Probability: 99.1 % -Lightdrop: 1.0 mag -Max duration: 13.0 s -Tangra v. 3.5 was used to produce the lightcurve. -A Schmidt-Cassegrain 11-inch telescope was placed 2.5 m north and was observing the same event. It was equipped with a Watec 910HX/RC videocam. Shutter = 1/50, Manual Gain = 35/41; Gamma = 1.00. Both instruments show similiar results. -Both lightcurves can be seen here: http://sposetti.ch/wp-content/uploads/2014/09/Asia_C11_N420_lightcurve_11.png