ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 09 October 2021 STAR: TYC 2344-00070-1 (11.0 mag) ASTEROID: Loreley No: 165 2 OBSERVER: Name: Marek Zawilski Abbr: E-mail: marek.zawilski@p.lodz.pl Address: ul.Julianowska 5/7 m.322, 91-473 Lodz, Poland 3 OBSERVING STATION: Nearest cities: Turek Station: Psary Latitude: 51d 59' 55.4" N Longitude: 18d 38' 25.3" E Altitude: 124m 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 - 18:07:00 - N/A - 1 D - 18:08:04.02 0.06 AOTA analysis R - 18:08:15.75 0.09 AOTA analysis E - 18:09:04 - N/A - 1 Duration : 11.73 sec Mid-event : 18:08:09.89 Predicted mid-event : 08 Oct; 18:08:10 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: Laptop time controlled by the GPS Shelyak TimeBox device (time error 0.000 s). Sensor: ZWO ASI 120MM, shutter set for 100 ms, time resolution 116 ms, image resolution 1024x768 px, gain 82. Recording: SHARPCAP v.3.2.6480.0 software. 7 OBSERVING CONDITIONS: Atmospheric transparency: very good Wind: none Temperature: +5 deg C Star image stability: good Minor planet visible: yes 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. Predicted max. 20.2 sec. duration with 2.2 mag. drop. Event probability at site : 97.4% Distance from center line : 101 km in 133° direction, inside the predicted path. Local * conditions (Alt,Az): 20°, @61° in Perseus. Moon (Alt, Az): below the horizon