ASTEROIDAL OCCULTATION - REPORT FORM +----------------------------------------+ +----------------------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +----------------------------------------+ +----------------------------------------------+ 1 DATE: 2021 Februry 25 STAR : TYC1800-01942-1 ASTEROID: (32162) 2000MV5 2 OBSERVER: Name: Gérard VAUDESCAL Abbr:VDC E-mail: gg.vaudescal@free.fr Address: 65380 Azereix - France 3 OBSERVING STATION: Nearest city: AZEREIX (65380) Station: Observatoire d'Azereix Latitude: N 43 12 36.0 (WGS84) Longitude: W 00 00 46.5 (WGS84) Altitude: 340 m Single, OR Double or Multiple station (Specify observer's name): Single +---------------------------------------------------+ 4 TIMING OF EVENTS: | | | OCCULTATION RECORDED: NEGATIVE | | | +---------------------------------------------------+ Type of event Start observation Interrupt-start Disappearance Blink Flash End observation Jnterrupt-end Reappearance Other (specify) Event Time (UT) Acc. Comments Code HH MM SS.ss S.ss S - 22:53:30.84 on frame n°7 D - +/- R - +/- E - 22:55:49.37 on frame n°703 Duration : sec xxxx +/- Mid-event: xxxxx (Pédicted 22:54:43 +/- 2,4 sec UT) Was your reaction time applied to the above timings? NO 5 TELESCOPE: Type: Ritchey Chrétien RC10 - Aperture: 254 mm - Magnification: Focus 1340mm - F/D=5.27 Mount: Equatorial - Motor drive: YES 6 TIMING & RECORDING: Time source: GPS 1 PPS-NMEA Sensor: CAMERA ASI178MM - Binning x2 - Exposition :0,199sec/f => 5,03fps Gamma na - Gain 510/510 Recording: Genika 10bits - format SER - Time insertion: Windows time stamping by recording software Genika Event insertion (specify): PC-Windows10 7 OBSERVING CONDITIONS: Hazy Sky Wind: 0 ms Temperature: 8,9 °C Cloud : 90% Star image stability: seeing 1.2 arcsec Minor planet visible: No 8 ADDITIONAL COMMENTS: Reduction under TANGRA 3.7.3 Rev 20200512 Predicted Max Duration: 0,7sec Predicted Magnitude Drop: 8.1 mag No corrections applied / the test results show a variation of +/- 10ms whatever the exposure times between 20 and 700ms