Quote:
Originally Posted by Tandum
I've only just noticed that. Why would you want to sum? Wouldn't that just burn out parts of the image?
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Summing also reduces the noise.
Depends what you are trying to achieve.
If you are imaging a dim galaxy or supernova or star and you can only reasonably use 5 min exposures due to tracking etc then you are limited to the magnitude that your setup can detect in a 5 min exposure. If you double the exposure you will approximately be able to see 1 mag deeper. You need to add the exposures to achieve this not average them.
Added exposures reduce the noise by the square root of the number of exposures. ie 4 exposures added will 1/2 the noise, 9 added will 1/3 the noise etc.
You are correct that you can burn out bright parts of the image but it also allows you to see very dim parts that are only just above the noise.
I use adding when doing photometry to increase the S/N ration of dim stars letting me measure the mag of stars at mag ~16.5 with a reasonable S/N ratio. It doesn't matter that some of the stars will be burnt out.