ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 19 March 2022 STAR: HIP 27793 (8.6 mag) ASTEROID: Jimsimons No: 6618 2 OBSERVER: Name: Marek Zawilski Abbr: E-mail: marek.zawilski@p.lodz.pl Address: ul.Julianowska 5/7 m.322, 91-473 Lodz, Poland Assitance: Mieczyslaw Borkowski 3 OBSERVING STATION: Nearest cities: Lodz Station: Bedkow-Kolonia Latitude: 51d 36' 03.9" N Longitude: 19d 44' 49.2" E Altitude: 182 m 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 - 01:17:30 - N/A 1.0 D - 01:18:13.52 0.02 AOTA analysis R - 01:18:13.72 0.03 AOTA analysis E - 01:19:01 - N/A 1.0 Duration : 0.20 sec Mid-event : 01:18:13.62 Predicted mid-event : 19 Mar;01:18:14 UT +/- 1 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: Laptop time controlled by the GPS Shelyak TimeBox device (systematic time delay +0.807 s with 8 satellites, considered in final results). Sensor: ZWO ASI 120MM, shutter set for 50 ms, video time resolution 50 ms, image resolution 640x480 px, gain 50, brightness +12. Recording: SHARPCAP v.4.0.8667.0 software. 7 OBSERVING CONDITIONS: Atmospheric transparency: good Wind: none Temperature: -5 deg C Star image stability: moderate Minor planet visible: yes 8 ADDITIONAL COMMENTS: The light curve analyze using Tangra software and a careful inspection of the screen replay showed a clearly remarkable drop of the star brightness caused by the asteroid. The star image was stable both for the occulted and a guiding star. The D and R times according to the AOTA analysis. The star rapidly disappeared and was invisible on 4 sequential frames. Predicted max.0.5 sec. duration with 8.5 mag. drop. Event probability at site : 51% Distance from center line : 0.3 km, inside the predicted path. Local * conditions (Alt,Az): 12°, @320° in Auriga. Moon (Alt, Az): 34°, @212°, did not disturb the observation.