ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+ 1 DATE: 2021/02/01 STAR: UCAC4 628-024818 ASTEROID: Hanskya No: 1118 2 OBSERVER: Name: Daniel BLAZEWICZ Address: 32-015 Klaj, POLAND 3 OBSERVING STATION: Klaj Nearest city: Niepolomice (Poland) Longitude: E 20 19 04.2 (WGS84) Latitude: N 49 59 33.0 (WGS84) Altitude: 210 m (MSL) Single station +----------------------------+ 4 TIMING OF EVENTS: | | | EVENT REPORTED: NEGATIVE | | | +----------------------------+ Event code S: observation Start I: Interruption start D: Disappearance J: Interruption end R: Reappearance B: Blink F: Flash E: observation End O: Other (specify) Abbreviations P.E.: Personal Equation = reaction time (for visual obs) Acc.: Accuracy (overall accuracy of the given time) Comments Event Time (UT) P.E. Acc. Code HH:MM:SS.ss S.ss S.ss S - 00:50:50 - - : E - 01:02:00 - - : 5 TELESCOPE: Type: NEWTON Aperture: 350 mm Magnification: prime focus f/4.8 Mount: EQUATORIAL with polar wedge Motor drive: YES 6 TIMING & RECORDING: Time source: NTP Stratum 1, Linux Ubuntu, synchronization every 32 s Sensor: ZWO ASI174MM-C Recording: ZWO ASICAP V2.3 7 OBSERVING CONDITIONS: Atmospheric transparency: poor-fair Wind: no Temperature: -12 deg C Star image stability: good Minor planet visible: no 8 ADDITIONAL COMMENTS: At the beginning, due to thin clouds, the star was barely seen. After a minute or so conditions became better but decided to not decrease exposition time. Exposition time: 900 ms Camera temperature: -20 deg C Analyzed using Tangra v3.6.17 S/N of occulted star: 20 (at about 00:56:00) ITALOccult feed (2021/01/30): Event time: 00:56:08 UT Error in time: 6 s Max duration: 9.3 s Star magnitude: 11.5 m Asteroid magnitude: 13.5 m Combined magnitude: 15.4 m Magnitude drop: 1.9-2.2 m Position: In the shadow, 4 km from the central line Probability: 54.4%