Before answering let me ask something :Have you ever tried shooting Pluto?
Of course!
I ask that because I always encounter people saying those same things about the Dawes, Raleigh principles, Airy disks, Lagrange that, ..etc and that it is impossible to resolve anything on Pluto.
Lagrange (Lagrangian Points?) - and resolution???
In the end, it boils down to this: first finding Puto in the nightsky (most people cannot find it).If you haven`t, you would be suprised. (I can upload my RAW FITS images of Pluto later if needed)
Finding Pluto - and?
Second:The reading of a CCD camera of objects captured in exposures taken in the HMIR way ( did you watch our demonstration vídeos on SPACENOW?.They are lengthy, about 35 minutes, but they show all) is a totaly new raw material to work with.The LRGB combination of bands gives the astro imager a depth that researchers are not familiar with (why? Because they reject color digital SLRs and color CCD cameras).
Reseachers ARE familiar with any detector and any band (of which LRGB is only a tiny part) and they do NOT reject SLRs and Color CCDs as long as this is appropriate for the job (and it usually is not). Researchers know their detectors and their limits.
What my coleague and I discovered while developing the HMIR processing method is that on single perfect shots, an object`s disk will come across imaculate to the sensors of the CCD câmera( you need to take hundres of shots ,sometimes ,to get what we call THE perfect shot).
Lucky imaging is well established within the scientific community and there is also a huge amount of knowledge about thresholds and limits, about defects and spurious signals. In Lucky imaging there is nos uch thing as THÈ perfect shot as it is all about statistics.
What´s done after is simply processing out what is noise and excess color while FREE TRANSFORMING the processed object in little enlargement installments so that the resolution achieved in the RAW image does not get lost.( this is the answer to your question).FREE TRANSFORMING stops when limit to enlarging it further becomes aparent.
Lots of tiny increments introduce spurious signals and after some iterations the original signal is most likely severely damaged or lost. What is left is spurious detail.
People will say that that can not be done in research because it`s an algorithm and we are creating artifacts that were not there to begin with. This is the theory, but in reality it WORKS.
Algortihms - however good - can not introduce real information that is not in the raw data. And as we know sub arcsecond imaging is difficult and imaging ten fold finer detail with amateur telescopes from the Earths surface sound like a dream - and HMIR imaging seems to be a dream. Wishful thinking and nothing more (even fantasy litterature seems serious compared to the HMIR-claims).
Depending on the quality of the RAW image captured with this method and a CCD of ,say 4,2 million pixels, we can enlarge objects to as much as 800% of their original size with practically no resolution loss.
Enlarging 800 % with practically no resolution loss should leave images with LESS resolution than the original images. Lost information is lost. There is no way to reclaim lost information. did not get this one at all.
The images shown are real (any image is, even paintings and drawings) but the images do not correspond with reality.
'nuff said this time? This is my last post about this thread - enough said about dubious claims without root in reality and images showing only artefacts from excessive post prosessing.