Quote:
Originally Posted by bmitchell82
Well here is a comparison of a 5 second 90 second and a 600 second image taken on the same night same scope same camera. This i hope shows that data doesn't magically appear
I have done a basic curves and levels on these images to bring out a fair bit of the details that are present.
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Hi Brendan,
I'm a newbie as well, so I'm very interested in what you're saying.
I'm curious whether you have come across the "skyfog statistics limited" approach to modelling the SnR (in terms of calculating exposure times)?
http://www.samirkharusi.net/sub-exposures.html
http://www.pbase.com/samirkharusi/image/37608572
http://www.starrywonders.com/snr.html
Basically, it says that the total integration time (i.e. number X duration of subs) correlates with SnR provided some assumptions are met - primarily, that the sky fog histogram peak for each sub is exposed just enough to separate from the left edge (but no more - to maximise dynamic range).
In that case, how would a stack of 120 x 5-second exposures compare to your 1 x 600-second image (equal integration time)?
Furthermore, if you took a 600-second exposure with an f/8 scope, wouldn't that give you a similar histogram to a 150-second exposure with a f/4 scope? Therefore, isn't the ideal/maximum subexposure duration affected more other factors - like sky fog - than just an arbitrary time limit? For example, a 10-minute sub at f/2 lens would probably be overexposed in most locations with even moderate light pollution.
Dave