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Objects Session Notes
W And - mira variable Astrometric & Photometric Monitoring - W And (mira variable)
- Very short evening session (0.4hr), rapidly cut short by cloud and shower of rain. - CCD operation of -25 degC
(at 84% average cooling).- main objective was to acquire images of certain selected stars for ongoing photometric and astrometric analysis, however in the event only images of W And were actually acquired
Light Curve for variable W And
(Andromeda) |
[ Images and more Light Curves for W And ] |
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Images collected for Astrometric Monitoring
of Nearby Stars Project
Images collected for Photometric Monitoring
of Variable Stars
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This Web Page: | CCD Images - Session 280 (2008-04-04) |
Last Updated : | 2015-05-16 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |