ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 15 August 2022 STAR: TYC 2395-00468-1 (8.8 mag) ASTEROID: Catriona No: 1116 (14.8 mag.) 2 OBSERVER: Name: Marek Zawilski Abbr: E-mail: marek.zawilski@p.lodz.pl Address: ul.Julianowska 5/7 m.322, 91-473 Lodz, Poland Assistance: Klemens Liban 3 OBSERVING STATION: Nearest cities: Sulejow, Piotrkow Tryb. Station: Barkowice Mokre Latitude: 51d 23' 50.0" N Longitude: 19d 51' 07.0" E Altitude: 172 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 - 23:20:00 - N/A 1.0 D - 23:20:47.85 0.03 AOTA analysis R - 23:20:48.88 0.02 AOTA analysis E - 23:21:22 - N/A 1.0 Duration : 1.03 sec Mid-event : 23:20:48.37 Predicted mid-event : 15 Aug;23:20:49 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 (time error 0.000 s with 12 satellites). Sensor: ZWO ASI 120MM, binning 2, shutter set for 50 ms, video time resolution 50 ms, image resolution 640x480 px, gain 76, brightness 9. Recording: SHARPCAP v.4.0.8949.0 software. 7 OBSERVING CONDITIONS: Atmospheric transparency: good Wind: none Temperature: 20 deg C Star image stability: average Minor planet visible: no 8 ADDITIONAL COMMENTS: The light curve analyze using Tangra software and a careful inspection of the screen replay showed a distinct drop of the star brightness caused by the asteroid. The D and R times according to the AOTA analysis. The observation was made inside the predicted path near its center line D and R times very accurate, star scintillation. Predicted max. 1.2 sec. duration with 6.0 mag. drop. Event probability at site : 90.5% Distance from center line :11.8 km in 288° direction, inside the predicted path. Local * conditions (Alt,Az): 21°, @59° in Auriga. Moon (Alt, Az):30°, @128°