Lecture - Image Processing

6. Image Calibration (unavailable)


Learning Objectives:

  • Why is image calibration necessary?
  • What are the regions of possible light-matter interactions?
  • What effects influence our primary astronomical signal?
  • How can we handle this influences?
  • How does the callibration change for different wavelength?

!!! Please note !!!
The content of this section is not part of the Demo-Version!