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Spectral common-mode offset rejection is cancellation of an additive frequency-axis shift when the same shift enters two spectral estimates with equal sensitivity and the estimates are subtracted. It improves a frequency difference without establishing accurate absolute frequencies. The relevant measurement model must identify what is shared, and over which observations.

For true frequencies ${\omega }_1,{\omega }_2$, write measured estimates asThe unknown common offset $b$ disappears exactly fromFor independent residual errors of standard uncertainty $s$, the difference still has standard uncertainty $\sqrt{2}s$. Cancellation of $b$ is not cancellation of all measurement noise. With correlated residuals, the covariance term must be retained in uncertainty propagation.^[ref]

An original example uses two spectral positions at $1600$ and $1650{\mathrm{cm}}^{-1}$. An additive shift of $3{\mathrm{cm}}^{-1}$ gives measured positions $1603$ and $1653{\mathrm{cm}}^{-1}$, with the same $50{\mathrm{cm}}^{-1}$ separation. A shared gain error is different: $Y_i=1.01{\omega }_i+3$ gives separation $50.5{\mathrm{cm}}^{-1}$. Subtraction rejects the offset but retains the scale error.

The algebra generalizes to a contrast of several spectral positions. If $Z={\sum }_i{w}_i{Y}_i$ and each $Y_i$ contains the same additive $b$, its contribution is $b{\sum }_i{w}_i$. Thus weights satisfying ${\sum }_i{w}_i=0$ reject that offset. Averaging positions with weights summing to one does not. This is an original linear-model derivation of the rejection condition, not a claim that every spectral estimator has this form.

Two failures of the ideal assumption are especially informative. With unequal spectral offset sensitivity, $Y_i={\omega }_i+a_{i}b+{\eta }_i$, subtraction leaves $(a_2-a_1)b$. If the offset drifts between observations, it instead leaves $b(t_2)-b(t_1)$. For a stationary drift with variance $s_b^2$ and correlation ${\rho }_b(\tau )$ at lag $\tau$, this residual has varianceA common instrument or reference does not alone imply perfect cancellation at different times.

An apparatus-level check measures two stable reference features using the same acquisition and fitting pipeline, then deliberately shifts the assigned axis origin. Their separation should stay fixed under an additive reassignment; a scale change should alter it. Repeated reference observations test temporal drift and residual covariance. In two-dimensional infrared spectroscopy, this test concerns frequency-estimation errors; spectral diffusion also describes physical fluctuations and cannot be identified or removed merely by subtracting an instrumental offset.

Unequal spectral offset sensitivity occurs when a shared instrumental or reference offset influences two spectral estimates by different amounts. It limits spectral common-mode offset rejection: subtraction cancels a common disturbance only to the extent that its two response coefficients match.

For frequencies ${\omega }_1,{\omega }_2$, write an explicit measurement modelwhere $b$ is the shared offset, $a_i$ are dimensionless sensitivities and ${\eta }_i$ are residual errors. ThenThus even perfectly shared $b$ leaves a residual when $a_1\ne a_2$.

An original uncertainty example uses $a_1=0.98$, $a_2=1.02$ and standard uncertainty $u_b=0.50{\mathrm{cm}}^{-1}$. The offset contribution to the difference is $0.04u_b=0.020{\mathrm{cm}}^{-1}$. With independent residual standard uncertainties of $0.010{\mathrm{cm}}^{-1}$ each and no correlation with $b$, the combined uncertainty isA general calculation retains the relevant covariances; the independent-error simplification is an assumption, not a consequence of a shared instrument.^[ref]

Reweighting also changes what is measured. Subtracting $Y_1/a_1$ from $Y_2/a_2$ cancels $b$ when both sensitivities are nonzero, but estimates ${\omega }_2/a_2-{\omega }_1/a_1$, not generally the original frequency difference. Achieving cancellation is insufficient unless the resulting estimator still answers the intended physical question.

A controlled reference perturbation can estimate the slopes $a_1$ and $a_2$ while the true spectral features are held stable. Their difference predicts leakage. Spectral offset identifiability asks whether the available observations can distinguish a real change of frequency separation from this leakage; one observed difference alone cannot determine both an unknown physical change and an unknown offset. Reference features, controlled perturbations or independently established response coefficients supply additional information.