19 sept 2023

siril dslr processing

 EOS/Ti and dslr-in-general users. Keep it simple.

Forget about in-camera bias and dark frames. They'll introduce further artefacts, noise in particular. Instead, simply subtract the bias value [1] as follows. 

Here I'm using a modern EOS with an offset of 2048. Earlier models [2] used 1024.

1. Calibration of flat frames

Convert all your raw files to fits files using Siril's Conversion tab

Load the flat frame sequence.

Calibrate as follows:

Now stack to get the master flat frame. The default is:  pp_flat_stacked.fits

2. Calibration of light frames 

Load the light frame sequence, then, leaving the bias value intact, include your newly stacked flat frame from (1) above:


Don't forget to check debayer.
Register then stack.

That's it.

[1] How do I find or check the offset?

  • Take a raw frame in total darkness with a shutter of 1/4000s or 1/8000s
  • Convert it to fits using the conversion tab
  • Open in Siril
  • Tools -> Image Analysis -> Statistics (on older versions: right click the image -> Statistics)

The origin of the 2048 should now be self explanatory


[2] 450d and older. There maybe others, but it's easy to check as above anyway.

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