ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 29 October 2019 STAR: TYC 1932-00469-1 (10.1 mag) ASTEROID: Sylvia (+Remus) No: 87 2 OBSERVER: Name: Artur Wrembel, Wojciech Broczkowski Abbr: Address: Zielonczyn at Bydgoszcz, Poland 3 OBSERVING STATION: Nearest cities: Bydgoszcz Station: Tobolice Latitude: 53d 09' 10.4" N Longitude: 17d 48' 03.0" E Altitude: 80m 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 - 23:37:04 - N/A - 1 : D - 23:39:29.20 - - 0.08 : D rapid R - 23:39:48.40 - - 0.08 : a moment of full brightness regaining, R on two frames 48.38 and 38.40, gradual E - 22:44:03 - N/A - 1 : Duration : 19.2 s Mid-event : 22:35:38.8 Predicted mid-event : 29 Oct; 23:39:43 UT +/- 2 sec Was your reaction time applied to the above timings? N/A 5 TELESCOPE: Type: Maxutov-Newton Mn-86 Aperture: 203mm Magnification: --- Mount: Equatorial Motor drive: YES Foc.length: 1200 mm 6 TIMING & RECORDING: Time source: UTC video time inserter DCF-77, version Cuno (around 2005). Sensor: Tayama night vision v.TC-3182, system CCIR, 25 fps. Recording: filmed from screen by Sony-Cybershot camera as a mpg file. 7 OBSERVING CONDITIONS: Atmospheric transparency: very good Wind: none Temperature: -2 deg C Star image stability: good Minor planet visible: no 8 ADDITIONAL COMMENTS: The D and R times were found from a direct screen view of the recording with the time display of 25 fps. The light curve analyze using Tangra software by M.Zawilski after converting the recording file into "avi" format. Unfortunately, only the target star seen in the field of view, therefore lightcurves for D and R have been found separately. S/N was about 2.5-2.7. The D and R times shown in the lightcurve images are not fully compatible with the given above due to undistinct display of some fractions of seconds obtained from the time inserter. So, the accuracy of both times have been decreased (see above). The dis- and reappearance clearly noticed on screen during the observation and the recording analyze. Predicted max 23.0 sec duration with 3.3 mag drop. Event probability at site : 94% Distance from center line : 93 km Local * conditions (Alt,Az): 29°, @84°