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The Nikon D200 Digital Camera Review:
Sensor Noise, Dynamic Range, and Full Well Analysis

by Roger N. Clark

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They may not be used except by written permission from Roger N. Clark.
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This page shows an analysis of noise, dynamic range, and full well capacity of a Nikon D200 camera. Raw data were kindly supplied by Eric Livo who gave permission to use the data for this analysis and its publication.

Procedures for performing this analysis are described in: Procedures for Evaluating Digital Camera Noise, Dynamic Range, and Full Well Capacities; Canon 1D Mark II Analysis

The lowest possible noise from a system detecting light is the noise due to Poisson statistics from the random rate of arrival of photons. This is called photon statistics, or photon noise. Noise from the electronics will add to the photon noise. We will see that the noise in Nikon D200 images is limited by photon statistics at high signal levels and by electronic noise from reading the sensor (called readout noise) at very low signal levels. In the case of high signal levels, a system that is photon statistics limited enables us to directly measure how many photons the sensor captures, and by increasing the exposure, we can determine how many photons are required to saturate the sensor. That is called the full well capacity. With data on the lowest noise to the highest signal, we can then determine the dynamic range of the sensor.


Results for determining read noise, gain, dynamic range and maximum signal-to-noise ratio are shown in Table 1. Column B is the gain derived from high signal data. Gains at ISOs higher than 100 are scaled relative to that at ISO 100. Read noise, Column C was determined from exposures with zero light on the sensor. Maximum signal, column D, is 32,680 electrons at ISO 100 for the Nikon D200. That maximum occurs at a signal level just below maximum A-to-D converter output 3980/4096 in 12-bit data numbers (DN). Dynamic range, Column E = maximum signal / read noise, and column F shows that range in photographic stops. Higher ISO reduces the maximum electrons (photons) that are recorded relative to ISO 100 (e.g. ISO 400 sees half the electrons of ISO 200). The maximum signal-to-noise ratio, Column G, is the square root of the number of maximum photons recorded (e.g. square root 16,770 at ISO 200 = 129) (read noise is negligible for the high signal case).

Table 1: Nikon D200: Derived Sensor Performance

 A        B            C          D         E        F         G
        Camera     Apparent
ISO      Gain     Read Noise   Maximum   Dynamic  Dynamic    Maximum
     (electrons/  (electrons)  Signal     Range    Range  Signal-to-Noise
      12-bit DN)             (electrons) (linear) (stops)     Ratio

 100     7.98        10.0      32,680    3,268     11.7       181
 200     4.0          8.1      16,770    2,070     11.0       129
 400     2.0          7.7       8,380    1,088     10.1        92
 800     1.0          7.4       4,190      566      9.1        65
1600     0.5          7.4       2,100      284      8.1        46 

An important factor in high ISO performance is collecting enough photons. Small pixels have difficulty doing just that. The Nikon D200 has pixels spaced every 6.1 microns (this is called the pixel pitch). The direct effect of the number of photons collected is the gain needed to convert the signal from a pixel to a digital number. The gain of the camera is given in column B in Table 1. Once gain drops below 1 electron/DN, there is little point in increasing ISO further. On the Nikon D200, unity gain occurs at about ISO 800. The effect of higher ISO above unity gain only decreases dynamic range without helping to detect lower signals. For comparison, unity gain of some large pixel DSLR cameras (e.g. the Canon 1D Mark IIi with an 8.2 micron pixel pitch) occurs around ISO 1300, and small pixel cameras (e.g. the Canon S70 with 2.3 micron pixel pitch) have unity gain near ISO 100. The unity gain ISO is an indication of the effective sensitivity of the camera. The Nikon D200 unity gain level is similar to other DSLRs with approximately 6-micron pixel spacing.

The system linearity of the Nikon D200 is shown in Figure 1, and is very good. System linearity includes the detector linearity, shutter reproducibility, f/stop reproducibility, and light source stability. At the very highest signals at ISO 100, the Nikon D200 departs from linearity above about 60,000 in a 16-bit tif file (within about 10% of saturation).

The signal-to-noise ratio as a function of intensity is shown in Figure 2. If the sensor is photon noise limited, the trend in this ratio is a square root dependence. If the system is photon noise limited, the signal-to-noise ratio squared directly equals the number of photons collected without needing gain conversions, or computing the slope of a line. The fact that the model matches the data very well indicates there are no other sources of noise contributing to the data at any significant level. Thus, for high signal levels, the Nikon D200 is photon noise limited. This means further improvements in electronics will not improve the signal-to-noise ratio for high signal levels. If the quantum efficiency were improved with a different sensor, that would certainly improve the signal-to-noise ratio.

Figure 1. The Nikon D200 shows a very linear trend with signal. Variations in signal level include repeatability of the shutter and aperture, as well as the light source. The model is the average high signal DN scaled according to exposure time and subtract read noise. The Nikon D200 shows some departure from linearity with signals within about 10% of sensor saturation at ISO 100.

Figure 2. Signal-to-noise ratio observed and predicted. The prediction model uses photon statistics and read noise. Model is average DN scaled to electrons plus read noise. For this case, ISO 100, the gain in the model is 7.98 electrons/camera DN (4096 levels), and the read noise is 10.0 electrons.

Figure 3. The electrons converted by the Nikon D200 sensor are shown relative to an arbitrary exposure level. The sensor saturates at about 32,680 electrons.

Dark Current and Related Noise

Another noise component is due to dark current, which will increase with exposure time. Dark current and its noise is also a function of the temperature of the sensor and associated electronics.

Data to be added.

The noise model is:

N = (P + r2 + t2)1/2, (eqn 1)

Where N = total noise in electrons, P = number of photons, r = read noise in electrons, and t = thermal noise in electrons. Noise from a stream of photons, the light we all see and image with our cameras, is the square root of the number of photons, so that is why the P in equation 1 is not squared (sqrt(P)2 = P).


The data shown here for the Nikon D200 shows that the camera is operating and near perfect levels for the sensor. This means that for high signals, noise is dominated by photon statistics. Noise at low signal levels is good but it would be nice to see a lower read noise, something more like 4 electrons. To achieve higher signal-to-noise ratio images, a higher quantum efficiency sensor with a larger full well would be needed. Without increasing the full well capacity, the maximum signal-to-noise ratio would not improve. Improvements in quantum efficiency of about 3 are possible (Reference 2), but currently that would require much more expensive detectors, such as back-side illuminated CCDs. Note some DSLRs have maximum full well capacities on the order of 50,000 electrons (e.g. Canon 20D) to 80,000 electrons (e.g. Canon 1D Mark II), so the Nikon D200 is on the low end of full well capacity. For comparison with a larger pixel DSLR, compare Table 1 and the figures with that for the Canon 1D Mark II Analysis. Compare the Nikon D200 with the Nikon D50 Analysis, which has a full well of 30,490 electrons at ISO 200, almost double the D200.


1) CCD Gain.

2) Charge coupled CMOS and hybrid detector arrays

3) Canon EOS 20D vs Canon EOS 10D and Canon 10D / Canon 20D / Nikon D70 / Audine comparison


5) Astrophotography Signal-to-Noise with a Canon 10D Camera


DN is "Data Number." That is the number in the file for each pixel. I'm quoting the luminance level (although red, green and blue are almost the same in the cases I cited).

16-bit signed integer: -32768 to +32767

16-bit unsigned integer: 0 to 65535

Photoshop uses signed integers, but the 16-bit tiff is unsigned integer (correctly read by ImagesPlus).

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First published September 16, 2006.
Last updated September 16, 2006