Observed by Hideyoshi Karasaki
and Masayuki Ishida
Analized by Kazuhisa Miyashita
Catalogue details
Fig.1 Information of star details by OCCULT Ver.4
Place name Nerima, Tokyo, Japan
Fig.2 Limovie analysis (by Karasaki) The step is visible clearly although measured points are scattered by air scintillation.
Diffraction fitting and photometry
Fig.3A Fitting Karasaki's observation to diffraction simulation. Fig.3B Fitting Ishida's observation to diffraction simulation.
Elements of separation to the radial direction of lunar are 0.100(Karasaki) and 0.095(Ishida) arcsec. These are larger than expected value 0.059(Karasaki) and 0.056(Ishida)
Nerima |
Object | Phenomenon | Time | magnitude | Component B | Appearance | 19h19m10.039s +/- 0.034sec | 7.48 | Component A | Appearance | 19h19m10.481s +/- 0.034sec | 6.90 | Time difference | 0.442 sec |
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Object | Phenomenon | Time | magnitude | Component B | Appearance | 19h15m08.30s +/- 0.034sec | 7.20 | Component A | Appearance | 19h15m08.67s +/- 0.034sec | 7.11 | Time difference | 0.367 sec |
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Calclation of astrometry |
Fig. 4 Position of components. Red cross is the component's position obtained from occultation observations. |