Navigation
index
next
|
previous
|
AsPyLib 2.0.0 documentation
»
4. Script for accurate photometry
ΒΆ
4.1 Assumptions
Philosophy
Star catalogs and reference stars
Calculating magnitude noises
Last changes (v1.2.0 and later)
4.2 Input parameters
Where to start ?
Names of the input images
Disk sizes for photometry
Generic name for output files
4.3 Running the photometry script
Checking input images
Computing image shifts
Selecting the targets
Checking quality of reference stars
Checking the photometry curves
Final results
Previous topic
3.6 Fitting stars
Next topic
4.1 Assumptions
This Page
Show Source
Quick search
Enter search terms or a module, class or function name.
Navigation
index
next
|
previous
|
AsPyLib 2.0.0 documentation
»