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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)  | 
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| [ 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 |