I just bought a Hasselblad X2D and it arrived one week ago. I am now learning about photographic post-processing.
I arrive by way of Astrophysics and PixInsight processing of both: filter wheel multi-color exposure stacks, and CFA image stacks from Bayer matrix sensors.
There is no ISO setting on an Astronomical camera, and I have full control over what linear and nonlinear processing steps I apply to raw images, once corrected for flat field, read noise, and bias, (and possibly deBayered).
So, now in the photon rich environment of photography, there is ISO -- which appears to be simply a way of scaling the significant portion of 16 bit DAC outputs to the upper 8 bits shown on histograms in programs like Phocus, Capture One, and others.
I am confused that there is so little discussion of deBayering of CFA's as an integral part of "color science" in the popular posts. And there appears to be no available information from any of the camera manufacturers about how they deBayer their raw data. Likewise, there are no explicit mentions of the ordering of exposure correction, histogram adjustments, saturation changes, etc.
My impression is that Phocus reads in a Bayer'ed image from the camera and applies lens distortion and vignetting corrections (akin to my flat field corrections), and deBayering, in addition to a possible nonlinear Gamma correction, on the way to the in-memory image shown on screen, and used for export conversion.
However, the .FFF files remain as RGGB Bayer'ed images, and are possibly stored without lens distortion and vignetting corrections. The .FFF files also do not appear to have the Gamma correction folded in.
All these camera corrections appear to be performed by Phocus, and not by the camera body processor. I cannot say what happens to in-camera JPEG images. Certainly much of this happens in camera, but that is of little concern to me. I am mainly interested in RAW processing.
Do any of you veterans out there know any of these details of processing? Thanks in advance!
I arrive by way of Astrophysics and PixInsight processing of both: filter wheel multi-color exposure stacks, and CFA image stacks from Bayer matrix sensors.
There is no ISO setting on an Astronomical camera, and I have full control over what linear and nonlinear processing steps I apply to raw images, once corrected for flat field, read noise, and bias, (and possibly deBayered).
So, now in the photon rich environment of photography, there is ISO -- which appears to be simply a way of scaling the significant portion of 16 bit DAC outputs to the upper 8 bits shown on histograms in programs like Phocus, Capture One, and others.
I am confused that there is so little discussion of deBayering of CFA's as an integral part of "color science" in the popular posts. And there appears to be no available information from any of the camera manufacturers about how they deBayer their raw data. Likewise, there are no explicit mentions of the ordering of exposure correction, histogram adjustments, saturation changes, etc.
My impression is that Phocus reads in a Bayer'ed image from the camera and applies lens distortion and vignetting corrections (akin to my flat field corrections), and deBayering, in addition to a possible nonlinear Gamma correction, on the way to the in-memory image shown on screen, and used for export conversion.
However, the .FFF files remain as RGGB Bayer'ed images, and are possibly stored without lens distortion and vignetting corrections. The .FFF files also do not appear to have the Gamma correction folded in.
All these camera corrections appear to be performed by Phocus, and not by the camera body processor. I cannot say what happens to in-camera JPEG images. Certainly much of this happens in camera, but that is of little concern to me. I am mainly interested in RAW processing.
Do any of you veterans out there know any of these details of processing? Thanks in advance!