ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 02 March 2021 STAR: TYC 1224-00140-1 (11.4 mag) ASTEROID: Venusia No: 499 2 OBSERVER: Name: Marek Zawilski Abbr: Address: 91-473 Lodz, Poland 3 OBSERVING STATION: Nearest cities: Lodz and Poddebice Station: Tobolice Latitude: 51d 54' 46.4" N Longitude: 19d 03' 21.9" E Altitude: 140m MSL Datum (WGS84 preferred): WGS84 Single, OR Double or Multiple station (Specify observer's name): SINGLE +----------------------------------+ 4 TIMING OF EVENTS: | | | OCCULTATION RECORDED: POSITIVE | | | +----------------------------------+ Type of event Start observation Interrupt-start Disappearance Blink Flash End observation Jnterrupt-end Reappearance Other (specify) Comments Event Time (UT) P.E. Acc. Code HH:MM:SS.ss S.ss S.ss S - 20:22:58 - N/A - 1 D - 20:23:40.75 0.16 AOTA analysis R - 20:23:44.29 0.11 AOTA analysis E - 20:24:25 - N/A - 1 Duration : 3.54 sec Mid-event : 20:23:42.5 Predicted mid-event : 02 Mar; 20:23:44 UT +/- 2 sec Was your reaction time applied to the above timings? N/A 5 TELESCOPE: Type: Cassegrain Aperture: 203mm Magnification: --- Mount: Equatorial Motor drive: YES Foc.length: 2032mm reduced to 1016mm 6 TIMING & RECORDING: Time source: GPS Shelyak TimeBox for adjusting the Lenovo laptop clock; A time correction established in relation do the 1pps TimeBox diode pulses: minus 0.05s (-50 ms). Sensor: ZWO ASI 120MM, shutter set for 221ms, image resolution 640x480 px, gain 50. Recording: SHARPCAP v.3.2.6480.0 software. 7 OBSERVING CONDITIONS: Atmospheric transparency: good Wind: none Temperature: +5 deg C Star image stability: good Minor planet visible: yes (after the occultation of the target star) 8 ADDITIONAL COMMENTS: The light curve analyze using Tangra software and a careful inspection of the screen replay showed a remarkable drop of the star brightness caused by the asteroid. The star image was stable enough both for the occulted and a guiding star. The D and R times according to the AOTA analysis. The recorded duration longer than epredicted. Magnitude drop smaller than predicted by the last update from Feb.28 (limit magnitude capability - about 13.5 mag.). Assymetric lightcurve (rapid D, gradual R), mean S/N 8.3. Predicted max. 2.7 sec. duration with 4.2 mag. drop (according to the last update from Feb.28). Event probability at site : 61.7% Distance from center line : 8 km in 271° direction, inside the predicted path. Local * conditions (Alt,Az): 20°, @275° Moon (Alt, Az): below the horizon