File:CCD Flat Field.jpg
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| Description | Flat field image. Subtraction of the dark frame and flat field correction applied to the original, raw CCD image results in the final, calibrated image. The flat field image is recorded by pointing the instrument towards a unifromly illuminated surface. It records differences in the sensitivity of pixels, and vignetting in the optical path. The dark "doughnuts" are caused by dust specks on the CCD window. |
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| Source | Own work |
| Author | H. Raab (User:Vesta), Johannes-Kepler-Observatory, Linz, Austria (http://www.sternwarte.at) |
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All images of the series showing the calibration of a CCD image:
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I, the copyright holder of this work, hereby publish it under the following licenses:
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License. |
  
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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license. | |
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| This licensing tag was added to this file as part of the GFDL licensing update. |
This file is licensed under the Creative Commons Attribution-Share Alike 2.0 Austria license.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 01:26, 18 February 2006 | | 508 × 489 (79 KB) | Vesta~commonswiki (talk | contribs) | * '''Description:''' CCD flat field image (light frame). *'''Source:''' self-made by H. Raab (User:Vesta) {{GFDL}} {{cc-by-sa-2.0-at}} Category:CCD |
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