
Two part mosaic of the eastern half of the Barnard's loop.
In this page I have collected links to a series of pages or pdf documents where I have outlined some of the techniques used in my processing. The date of the documents reflect the evolution of the processing, and some of the tips I describe I use no more, but might still be useful. Use any of this at your risk and peril!
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Processing a globular cluster (2004)Some tips on preserving colour information while improving the star sharpness. |
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Evaluation of the FD/EOS adaptor (2004) |
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Using a low pass filtered image to enhance subtle nebular features (2005).A complex interplay of bright and dark nebulae with several open clusters. This image has been processed with a procedure I developed to enhance the nebular features in a wide field image. See here for a detailed description. Modified Canon 350D, 30x4' exposures, 135 mm f2.8. The field is about 6° by 4° 18'. See here for an old 40 min exposure on the never forgotten Kodak 2415 (300 mm f4 plus deep red filter). |
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Processing of IC 1848 (2006) |
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a Narrow Band Imaging with a DSRL camera (2007)A long paper published on the January 2008 issue of Coelum. In Italian. |
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Fighting against the periodic error of a Losmandy mount (2008)Looking south-east from our house. D300, 135 mm f 2.0 composition of two frames exposed for the Moon and background. |
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Fighting differential flexures and mirror shift in the ASA (2008) About detecting and fixing the problem. |
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Fixing stars that are way too bright (2009) |
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Power point presentation prepared for the Monte Amiata 2009 star party (in Italian) |
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Correcting gradients in a desperate case: a new technique (2009) |
Copyright © 1997-2009 by Gimmi Ratto. (May 30, 2009)