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By Baltard,.Louis-Pierre

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I completed these modifications in the summer of 1995. 2 The Art and Science of CCD Astronomy There are several camera operating modes that make the camera easy to use. 8 mm and 378 x 242 pixel mode (2 adjacent pixels binned together) or 252 x 242 pixel mode (three adjacent pixels binned together). In this way, camera sensitivity is improved at the cost of some resolution. This brings up the important subject of matching the telescope focal ratio to the mode in use to maximise the resolving power of the telescope - CCD camera combination.

Physically, the largest CCD that I currently have is the SBIG ST6. I use that and a CFW8 (colour filter wheel) for tri-colour and monochrome deep-sky work. Although this camera is beginning to show its age, it is still very efficient and does a good job on galaxies and nebulae. Finally, I employ a SBIG ST4 for guiding the larger telescopes on comets and deep-sky objects. 4 m) heated room where images are acquired and saved on a 486-40 IBM clone. This PC is networked with a computer in the house, a 486-133 IBM clone.

The 245PLUS software allows you to take multiple exposures automatically. This is very convenient for taking a number of short-exposure images, dark frames and flat fields. In this way, you can catch the moments of excellent seeing and select the best images for further processing and discard the bad ones. I take a number of dark frames throughout an observing session, because the camera is sensitive to temperature changes resulting in bias drift during the night. The latest versions of CB245 now include darkframe matching.

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