ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 06 August 2020 STAR: UCAC4 405-090153 (11.9 mag) ASTEROID: de Villegas No: 15785 2 OBSERVER: Name: Marek Zawilski Abbr: Address: 91-473 Lodz, Poland 3 OBSERVING STATION: Nearest cities: Lodz and Poddebice Station: Tobolice Latitude: 51d 54' 48.3" N Longitude: 19d 03' 22.4" 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: NEGAITIVE | | | +----------------------------------+ 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 - 22:36:45 - N/A - 1 : D - - : R - - : E - 22:37:30 - N/A - 1 : Duration : no occultation for sure Mid-event : Predicted mid-event : 6 Aug; 22:37:16 UT +/- 6 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: NTP via Dimension4 using the time server "tempus1.gum.gov.pl",Warsaw, laptop-time synchronized better than 0.01s, response of about 10 Polish ntp time servers checked evry one minute with the use of the professional software by T.Kluwak, regarding the time offset and resopose delay (both of very low value and stable - offset < +0.05s, delay <0.04s at 21:42-22:44 UT); Sensor: ZWO ASI 120MM, shutter set for 200 ms, image resolution 640x480 px, gain 70 (star faint). Recording: SHARPCAP v.3.1.5220.0 software 7 OBSERVING CONDITIONS: Atmospheric transparency: good Wind: none Temperature: +18 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 no remarkable drop of the star brightness caused by the asteroid. The star image was stable enough both for the occulted and a guiding star and there was no occultation longer than 0.2s. Predicted max 1.3 sec duration with 6.4 mag drop. Event probability at site : 8.8% Distance from center line : 23.6 km in 236° direction, outside the predicted path, inside the 1-sigma limit Local * conditions (Alt,Az): 24°, @8213° Moon (Alt, Az): 20°, @8134° at a distance of 72°, not disturbing much.