I've recently been fortunate enough to have access to a couple of different sensors and had a go at trying to benchmark them, in the interests of science
The target was the keyhole/wedge area of Eta Carinae nebula, as it has both subtle and higher contrast features. Each image represents the same exposure time.
They are a fraction of the original images but to retain colour information I chose 24-bit PNGs and then had to squeeze them in to 200KB.
Post some calibrated FITS files and I'll run a few numbers for you, Dunk. It's difficult to judge processed data. I've made a few silk purses out of sow's ears
#2 has the smallest pixels I assume, followed by #1 and then #3 getting larger.
#2 is the best resolved although I cannot figure out anything more than that
Thanks all...it's so hard to look at them side by side on a computer screen and tell one from another
Note that these are all unprocessed - just stacked and with PI's STF applied (for its sins).
They were registered onto the mono image (the smallest) so that I'd be looking at the same field...does this introduce any gremlins of its own? As the camera rotation was not the same in each case, there would have been pixel rotation involved in registering.
But indeed, #2 is from the camera with the smallest pixels...5.2 microns...my modded Canon 1100D. The pixels in images 1 and 3 are about the same size at 6.5 microns, 1 being colour, 3 being mono. I was hoping to see some differentiation between the colour and mono at the same pixel size...the Loch Ness monster of increased resolution, or just variance in seeing perhaps?
I should add that these are what you experts call "under sampled", given my scope focal length is 550mm, but when the images were captured I suspect the seeing would have been better than my resolving capabilities.
@RickS - I did the same calibration on all of them...nil
The mono CCD was cooled but not set point controlled. All three were taken at more or less the same ambient temperature, possibly a degree or two warmer the night the CCD images were taken.
Looking at them on my laptop instead of my iPhone (didn't even notice that two of them were colour!). #3 looks sharper (tighter) than #1 but #1 also looks like it has some elongation.
With #3 being mono it also has a greater dynamic range than #1 but that is mostly likely to be simply the difference between mono (filter) and any OSC.
To my eye, #2 is certainly the noisiest of the three, but also it has the tightest stars. Perhaps it would also be interesting, in the interests of science, to also compare a less bright region in all three?
Here are the stats I derived from single subs and the 30 minute stacks. Note that the single subs are 180s for the OSC cameras and 300s for the mono CCD, so I have estimated the SNR for a 2x180s stack for the OSC camera to give a number that is reasonably comparable.
Here are the stats I derived from single subs and the 30 minute stacks. Note that the single subs are 180s for the OSC cameras and 300s for the mono CCD, so I have estimated the SNR for a 2x180s stack for the OSC camera to give a number that is reasonably comparable.
That's awesome Rick thanks so much for taking the time out to analyse the data.
The old CCD, hereon known as "ol' faithful" really does walk away from the DSLRs. Cooling the DSLRs would make for some more interesting data points.
Quote:
Originally Posted by RickS
And here are comparison images of the three single subs with colour converted to luminance and image scale equalised.
Wow, yeah not only is there a clear difference between the DSLRs, but the CCD still shows its mettle
First of all I'm only into observing so most of the details discussed in this thread are well out of my depth.
But base purely on looking at both sets of 3 pics, I like #2 best for stars and #1 from each set for the gas. The 1s seem to have the sharpest edges between the gas and background sky.