Author Topic: Batch calibration basics  (Read 3342 times)

Offline astrodoc71

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Batch calibration basics
« on: 2012 August 22 04:51:14 »
I have a set of subs taken over many nights at different temps, with appropriately matched darks. Does the script match the dark and light temps if they appear in fits header? If I use 'optimize darks' will it still look for temperature matched files first?
Thanks

Offline astrodoc71

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Re: Batch calibration basics
« Reply #1 on: 2012 August 24 03:01:51 »
Well it does look like it worked totally fine, but I'm wondering now why there was scaling mentioned in the process console during the calibration. I think the factors were around .9 or so. Maybe this is expected for properly matched darks? Just curious

Offline pfile

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Re: Batch calibration basics
« Reply #2 on: 2012 August 24 15:14:08 »
im not sure about how the script matches darks, but scaling factors of 0.9 for matched darks seems about right to me. remember pixinsight is attempting to minimize noise in the calibrated image, numerically. because of this it does not actually care what the duration of the dark is relative to the light.

Offline Juan Conejero

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Re: Batch calibration basics
« Reply #3 on: 2012 August 24 15:54:01 »
Congratulations! If you are getting dark scaling factors around 0.9, that means that you are using very well matched darks.

As Rob has said, our dark frame optimization routine finds the scaling factors that minimize noise in the calibrated frames. It is a purely numerical solution that ignores exposure times, temperatures, etc, because it does not need them: it works exclusively with the pixel data.
Juan Conejero
PixInsight Development Team
http://pixinsight.com/

Offline astrodoc71

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Re: Batch calibration basics
« Reply #4 on: 2012 August 25 03:31:56 »
Hmmm. '....does not need them' That's very cool! Thanks guys.