Quote:
Originally Posted by Peter Ward
I don't see the well depth causing a "star bloat" problem.
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How can this not be Peter? The on pixel architecture such as the ABG LOD is identical across the KAF series. The only thing that comes to mind is the combination of well depth and pixel size (in correlation to sampling). I'm not stating that you can't produce great results with this camera, but its a horses for courses matter. You only need to review what Wolfgang Promper is doing with the U8300M to see the chip's potential, however there is no denying that the approach to imaging changes with a low well depth. Speaking with others on this matter at AIC, many take short and long subs to address the issue. There are undoubtedly other methods to address this such as post processing as previously mentioned.