ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 2018 May 31 STAR: 4UC 531-050024 ASTEROID: (221)Eos 2 OBSERVER: Name: Gérard VAUDESCAL Abbr:VDC E-mail: gg.vaudescal@free.fr Address: 65380 Azereix - France Name: Abbr: E-mail: Address: 3 OBSERVING STATION: Nearest city: VISKER(65200) Station: Observatoire de Biscarmiau Latitude: N 43 08 40.4 (WGS84) Longitude: E 00 03 31.8 (WGS84) Altitude: 488 m Single, OR Double or Multiple station (Specify observer's name): Single +----------------------------------+ 4 TIMING OF EVENTS: | | | OCCULTATION RECORDED: UNCERTAIN?| | | +----------------------------------+ Type of event Start observation Interrupt-start Disappearance Blink Flash End observation Jnterrupt-end Reappearance Other (specify) Comments Event Time (UT) Acc. Code HH MM SS.ss S.ss S - 22:15:54.57 on frame n°32 (correction Gerhard Dangl) D - 22:16:23.05 +/-0.32 R - 22:16:28.17 +/-0.32 E - 22:17:22.89 on frame n°170 " Duration: 5.12sec(forecasts 4,7s)- Mid-event: 22:16:25.61 (forecasts 22:16:28 UT +/-3.5s) Was your reaction time applied to the above timings? NO 5 TELESCOPE: Type: NEWTON Aperture: 305 mm Magnification: Focus 1188 mm Mount: Equatorial Motor drive: YES 6 TIMING & RECORDING: Time source: GPS 1 PPS Sensor: CAMERA WATEC 910HX/RC CCIR - integrated Shutter Low x32 (0,64sec/f) - Gamma 1 - Gain 32dB Recording: OccuRec V 3.2.0 Beta and Grabber Lindy USB2 - vidéo mode AAV Time insertion (specify):IOTA VTI V3 (CCIR) Event insertion (specify): PC-Windows7 7 OBSERVING CONDITIONS: Cloudy SKY (50%) Wind: 0 ms Temperature: 15 °C Star image stability: good variable transparency Minor planet visible: Yes 8 ADDITIONAL COMMENTS: Reduction under TANGRA 3.6.15 end AOTA v4.5.3.0 Note:No normalization on the flows (Tangra) of the star occulted with the star of comparison. The comparison star is too far from the target. The presumptions of a positive occultation remain however strong.