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Imaging Signal-to-Noise Ratio

Pixel SNR with background, dark charge, read noise and binning; noise budget, and the frames or co-added scans needed for a target SNR.

Model: Textbook approximation

Signal

3500.0 e⁻

Background 350.0 e⁻, dark 0.010 e⁻

Read Noise per Super-Pixel

1.50 e⁻

Charge binning: read once

Total Noise (one frame)

62.07 e⁻

Shot noise of the signal 59.16 e⁻

SNR (one frame)

56.391

SNR (1 frame averaged)

56.391

SNR·√N

Rose Criterion

Detectable

SNR ≥ 5 to see a feature reliably

Frames for SNR 100

4

⌈(SNR_target/SNR₁)²⌉, white noise

Dominant Noise (one frame)

Signal shot noise

90.9 % of the variance

Noise Budget (one frame)

Sourceσ (e⁻ rms)Share of variance
Signal shot noise59.1690.9 %
Background shot noise18.719.1 %
Dark-charge shot noise0.100.0 %
Read noise1.500.1 %

Independent sources add in quadrature, so the largest share of the variance sets the SNR.

Averaging Frames or Co-adding Scans

The same √N law holds for co-added spectra. It assumes noise that is independent from frame to frame; drift, fixed-pattern noise and 1/f noise are correlated and set a floor that averaging can't lower.

S = QE·N_signal·B², S_bg = QE·N_bg·B², D = R_dark·t·B²

SNR = S / √(S + S_bg + D + σ_read,B²); σ_read,B = σ_read (charge) or B·σ_read (digital)

N averaged frames: SNR_N = √N·SNR; frames for a target: N = ⌈(SNR_target/SNR)²⌉; Rose criterion SNR ≥ 5

Model and references

Textbook approximation. A standard approximation from the literature (for example paraxial, plane-wave or Gaussian-beam), valid within the range the page states. About the tiers

CCD equation: Poisson signal, background and dark charge plus Gaussian read noise per binned super-pixel; charge binning reads once, a digital sum b² times. Averaging N frames (or co-adding N spectra) gains √N only for noise that is independent between frames; drift, 1/f and fixed-pattern noise don't average down. EM gain, fixed-pattern noise and error in the subtracted background are left out.

  1. Janesick J. R. (2007). Photon Transfer: DN → λ. SPIE Press, ch. 5. Signal-to-noise ratio with read, dark and shot noise. doi:10.1117/3.725073
  2. Rose A. (1948). The sensitivity performance of the human eye on an absolute scale. J. Opt. Soc. Am. 38, 196. An SNR of about 5 to detect a feature. doi:10.1364/JOSA.38.000196
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