Hugh
Active member
Hi all,
I've not been around on here since a thread I posted last december, and, to be honest, I'm now back with the same question, although this time for the new build.....
We're just about to start working on a film that is currently being shot on a RED camera, and we want to make sure that we've got our heads around the colour-space side of it.
We are a VFX company that works almost exclusively on features. We've worked with standard film scans, SI2K and Viper footage, so we're not scared of new colour spaces - we just want to make sure that we have a scientifically accurate conversion from the files to a format where the pixel values are linearly representative of the number of photons hitting the sensor.
I've not had a chance to put a camera through its paces, which would involve doing tests at different exposures/lighting conditions to test the response of the different export formats, otherwise I'd be somewhat happier to figure this out on my own.
One of the test shots that we have been sent included a section where they stopped the camera down by 1, 2, 3 and 4 stops. Using this, I was able to at least get a rough approximation of the black point (quite lifted - about 0.132, or the equivalent of 135 cineon points)
Leaving the dGamma at 1 (or 1.7 in Shake, as it does an internal division by 1.7), as that's what | want my result to be, I found the best nGamma to be in the region of 1.36 (a far cry from the default Cineon nGamma of 0.6).
The white point made absolutely no difference to my test - as it's just adjusting the brightness of the Linear result (we're more than used to dealing with >1.0 values in comps). Seeing as my test was just based on changing the brightness to adjust the exposure in Linear, followed by a Lin->RedLog at the end, they all concatenated and I saw no change in the result. (Setting the white point to 135.001 was interesting... I ended up with float values in the 6-figures... possibly closer to the actual number of photons! Not practical, but fun to see)
However (after all of that), I'm still not convinced by the result. Whether this is down to the fact that what I thought was a stop, 2 stops etc down in camera was actually not, which gave me a bad base to work from, or something else, I don't know. Or maybe I'm just not trusting the numbers enough. I'd expect, though, when I've got a linear image, to be able to convert it to stardard cineon log and put it through a film lookup cube and have it look good, which I can't do with this at the moment.
So, does anyone have any thoughts? Has anyone done more investigation into the conversion and can let me know some details?
Thanks, all help very gratefully received!
I've not been around on here since a thread I posted last december, and, to be honest, I'm now back with the same question, although this time for the new build.....
We're just about to start working on a film that is currently being shot on a RED camera, and we want to make sure that we've got our heads around the colour-space side of it.
We are a VFX company that works almost exclusively on features. We've worked with standard film scans, SI2K and Viper footage, so we're not scared of new colour spaces - we just want to make sure that we have a scientifically accurate conversion from the files to a format where the pixel values are linearly representative of the number of photons hitting the sensor.
I've not had a chance to put a camera through its paces, which would involve doing tests at different exposures/lighting conditions to test the response of the different export formats, otherwise I'd be somewhat happier to figure this out on my own.
One of the test shots that we have been sent included a section where they stopped the camera down by 1, 2, 3 and 4 stops. Using this, I was able to at least get a rough approximation of the black point (quite lifted - about 0.132, or the equivalent of 135 cineon points)
Leaving the dGamma at 1 (or 1.7 in Shake, as it does an internal division by 1.7), as that's what | want my result to be, I found the best nGamma to be in the region of 1.36 (a far cry from the default Cineon nGamma of 0.6).
The white point made absolutely no difference to my test - as it's just adjusting the brightness of the Linear result (we're more than used to dealing with >1.0 values in comps). Seeing as my test was just based on changing the brightness to adjust the exposure in Linear, followed by a Lin->RedLog at the end, they all concatenated and I saw no change in the result. (Setting the white point to 135.001 was interesting... I ended up with float values in the 6-figures... possibly closer to the actual number of photons! Not practical, but fun to see)
However (after all of that), I'm still not convinced by the result. Whether this is down to the fact that what I thought was a stop, 2 stops etc down in camera was actually not, which gave me a bad base to work from, or something else, I don't know. Or maybe I'm just not trusting the numbers enough. I'd expect, though, when I've got a linear image, to be able to convert it to stardard cineon log and put it through a film lookup cube and have it look good, which I can't do with this at the moment.
So, does anyone have any thoughts? Has anyone done more investigation into the conversion and can let me know some details?
Thanks, all help very gratefully received!