ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 08 December 2020 STAR: 3UC231-011079 ASTEROID: Comet Schwassmann-Wachmann 1 N?: 29P 2 OBSERVER: Name: Richard MILES Abbr: RMI E-mail: rmiles.btee@btinternet.com 3 OBSERVING STATION: Golden Hill Obs. (MPC J77) Nearest city: SHERBORNE Station: Fixed Latitude: N 50 55 51".5 Longitude:W 02 24 19".0 Altitude: 80m Datum (WGS84 preferred): WGS84 Single, OR Double or Multiple station (Specify observer's name): Single +----------------------------------+ 4 TIMING OF EVENTS: | | | OCCULTATION RECORDED: NEGATIVE | | | +----------------------------------+ 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 02 - - : - - - : D - - - : R - - - : - - - : E - 23 27 58 - - : Duration : Mid-event : Was your reaction time applied to the above timings? N/A 5 TELESCOPE: Type: SCHMIDT-CASSEGRAIN Aperture: 355mm Magnification: Prime focus F/8 Mount: Paramount MEII Motor drive: Yes 6 TIMING & RECORDING: Time source: Computer clock synchronised with Dimension 4 Sensor: SXV H694 integrating CCD camera Recording: Computer harddisk (read/write interval = 0.75s) Start time of exposure recorded to nearest 0.1s Time insertion (specify): Event insertion (specify): 7 OBSERVING CONDITIONS: Atmospheric transparency: Good Wind: 5 km/s Temperature: 4C Star image stability: 4/5 Minor planet visible: Yes 8 ADDITIONAL COMMENTS: A CCD frame integration time of 1.5s was used, which equated to the electronic shutter open for 67% of time. The star was of R magnitude 14.7. The pseudonucleus of the comet was R magnitude 16.2. Apparent motion on the sky was 12.2 km/s. The observing location was about 370km south of the nominal JPL ephemeris track but 700km south of a high-precision orbit calculated by Mike Kretlow using Gaia DR2 astrometry of >550 2.0-m images. The size of the comet nucleus from HST and Spitzer data is 59-71km across Photometry used 4 reference stars all within 3.0' of the star. The ensemble magnitude of the comparisons exhibited a standard deviation of 0.05 mag. A total of 213 frames were recorded in which the star brightness remained constant with a standard deviation of 0.06 mag and no fade greater than 0.15 mag was observed during the entire monitoring interval. 2020 December 09 1700UT