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Table of Contents
1. Introduction
1.1 Equipment for imaging comets
2. Basics to CCD / CMOS image sensors
2.1 Full-Frame / Interline CCD sensor
2.2 Microlenses
2.3 Number of pixels
2.4 Pixel size
2.5 Surface
2.6 Characteristics of the image sensors
2.7 Cooling
2.8 Electronics
2.9 Field of application
2.10 Resolution
3. Basic concepts + practices
3.1 Light or Light frame
3.2 Dark or Dark frame
3.3 Bias or Bias frame
3.4 Flat or Flat frame
3.5 Creating a Flat frame
3.6 Creating a Dark frame
3.7 Creating a Bias frame
4. Standard image processing and calibration
4.1. Calibration of the data
4.2. Calibration with Astroart, how to do it
4.2.1 Manual calibration
4.2.2 Batch processing with Astroart including stacking the calibrated
images
4.3 Calibration with Fitswork. How to do it.
4.3.1 Creating Master dark-/Master flats
4.3.2 Manual method of calibrating images
4.3.3 Automatic method, stacking of calibrated images
4.4 Processing RAW-Images of DLSR cameras
4.4.1 Developing a RAW Image with Fitswork
4.4.2 Batch mode RAW Images
5. Advanced image processing
5.1 Histogram
5.2 Levels
5.3 Curves
5.4 Digital Development Processing
5.5 Noise reduction + sharpening + save as JPG
6. Special processing of comet images
6.1 Stacking without star trails
6.2 DeepSkyStacker-Method
6.3. Radial Weighted Model + Median Coma Model with Astroart
6.4 Larson-Sekanina filter
7. Measuring the tail and coma with Astrometrica
8. Evaluation, documentation and publication
References:
Glossary:
9. Table of CCD cameras, manufacturers, software