Full sensor specification

Including the lensmount mechanical, electrical and data interfaces and tolerances?

Has Olympus made those public yet? As far as I'm concerned, they should be a PDF file on one of their websites.

--
Bob
 
I made a few quick calculations from the data in the DPREVIEW version of the data table.

First, we see the RMS readout noise of 21 electrons rms at maximum readout speed. We also see that the pixel saturates at 40000. Thus, for a maximally exposed pixel, the expected dynamic range based on read-out noise alone is:

20*log(40000/21) = 66 dB, consistent with the entry in the table.

This also equates to 11 bits worth of range. You can get this by dividing the dynamic range in dB by 6 by taking the base-2 log of the dynamic range on a linear scale:

base-2 log of (40000/21) = 10.89

On the dark current front, we see

I'm not sure if these calculations are useful. I did them quickly, so they may have errors. They are certainly without context, since I don't have another table to compare against!
 
On the dark current front, we see
pixel fill-factor listed, but if we assume that the active pixel is
a full 6.8um x 6.8um, this equates to 2.312E-18 A for a pixel. Amps
are Coulombs/sec, with 1.6E-19 Coulombs/electron. Thus, we have a
dark current of 14.5 electrons/sec at 25C. It would seem that it
would take about a 1.5 sec. exposure for the dark current to
introduce pixel noise of the same order as the read-out noise. It
would take about an 11 sec exposure for the noise to limit the
dynamic range to 8 bits and thus for any noise to be visible at all
when viewed in 256-step grayscale - assuming no further noise
reduction algorithm is applied. All of this is at the native ISO
rating of the sensor and ignores any noise introduced later in the
signal stream.
This all relates to the electronic noise of the sensor, BTW, and doesn't address the statistical noise of the photons hitting the sensor, which grows less and less with larger pixel area. Rather, this dark current noise tends to appear as fixed-pattern noise, which is generally subtracted out using a dark frame for large exposures. By the time it's even visible in this sensor, it's already beyond the exposure length for this subtraction to kick in.
 
Including the lensmount mechanical, electrical and data interfaces
and tolerances?
Has Olympus made those public yet? As far as I'm concerned, they
should be a PDF file on one of their websites.
I'm beginning to get a very skewed view of the "four-third consortium". Kodak is outrageously generous with information. You can download spec sheets, applications notes, sample code, file formats, etc. for all their production sensors, and even sensors still in development. Kodak makes it easy to buy evaluation boards and development systems for these sensors. A friend of mine sent them an outline of his Ph.D. thesis, and Kodak sent him a sensor evaluation board for 6 months loan.

Kodak sells sensors in any quantity (including single pieces) to anyone who wants one for any purpose. Weather it's someone like me who would use it to build small quantities of lab equipment, or someone like Oly who wants to build 90,000 cameras.

My best guess is the "open spec" is entirely the work of Olympus, and that even Kodak isn't allowed free access.

--
Ciao!

Joe
 
DRG, you have to take gamma into account. x=y^0.45 where y is the luminance (normally in 12-bit) and x is the 8-bit gamma-corrected value. This also does not take colourspace conversions into account, which normally increase the numerical noise value.

Note: this relationship is not held at the lowest values precisely, but it's good enough.
I made a few quick calculations from the data in the DPREVIEW
version of the data table.

First, we see the RMS readout noise of 21 electrons rms at maximum
readout speed. We also see that the pixel saturates at 40000. Thus,
for a maximally exposed pixel, the expected dynamic range based on
read-out noise alone is:

20*log(40000/21) = 66 dB, consistent with the entry in the table.

This also equates to 11 bits worth of range. You can get this by
dividing the dynamic range in dB by 6 by taking the base-2 log of
the dynamic range on a linear scale:

base-2 log of (40000/21) = 10.89

On the dark current front, we see
pixel fill-factor listed, but if we assume that the active pixel is
a full 6.8um x 6.8um, this equates to 2.312E-18 A for a pixel. Amps
are Coulombs/sec, with 1.6E-19 Coulombs/electron. Thus, we have a
dark current of 14.5 electrons/sec at 25C. It would seem that it
would take about a 1.5 sec. exposure for the dark current to
introduce pixel noise of the same order as the read-out noise. It
would take about an 11 sec exposure for the noise to limit the
dynamic range to 8 bits and thus for any noise to be visible at all
when viewed in 256-step grayscale - assuming no further noise
reduction algorithm is applied. All of this is at the native ISO
rating of the sensor and ignores any noise introduced later in the
signal stream.

I'm not sure if these calculations are useful. I did them quickly,
so they may have errors. They are certainly without context, since
I don't have another table to compare against!
 
DRG, you have to take gamma into account. x=y^0.45 where y is the
luminance (normally in 12-bit) and x is the 8-bit gamma-corrected
value. This also does not take colourspace conversions into
account, which normally increase the numerical noise value.

Note: this relationship is not held at the lowest values precisely,
but it's good enough.
Ah, thanks. I was assuming a linear output.

Even so, at least this sensor seems quiet enough to keep read-out and dark current noise pretty much out of the picture for typical exposures, leaving photon statistics for the given pixel area as the main noise source. Given the large saturation electron count, I'd imagine the sensor could accept longer exposures than the typical interline CCD (low ISO mode) and thus reduce this statistical noise over a similar interline imager.
 

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