 Noise cost of polynomial baseline cancellation

The noise cost of polynomial baseline cancellation is the change in random measurement uncertainty when extra background trends are removed. For a linear pulse estimate $\hat{U}={\mathbf{a}}^T\mathbf{x}$ and reading-error covariance matrix $C$,The moment conditions for baseline-drift cancellation constrain $\mathbf{a}$ to reject specified polynomial backgrounds. They do not make the remaining random error vanish.^[ref]

For an original comparison, assume a pulse occupies only the central sample and the other samples contain background alone. Three samples at $-h,0,h$ with weights $\Delta t(-1/2,1,-1/2)$ cancel constant and linear backgrounds. Five samples at $-2h,-h,0,h,2h$ can instead useThese weights preserve the central signal and have zero moments of orders $0,1,2,3$. For independent reading errors of equal variance ${\sigma }^2$, the three-sample variance is $3\Delta t^2{\sigma }^2/2$, while the five-sample variance isWith $\sigma =1\mathrm{mW}$ and $\Delta t=1\mu \mathrm{s}$, the standard uncertainties are approximately $1.225$ and $1.394\mathrm{nJ}$. The second design removes quadratic and cubic drift as well, but its larger reference weights increase noise. This compares two specified estimators; it is not a claim that collecting more background data must worsen precision.

NIST's pulse-energy apparatus used before/after baseline measurements for background and thermal-drift correction.^[ref] The polynomial comparison above is an original model for choosing such measurements. Choosing minimum-noise weights under baseline moment constraints can exploit additional reference samples and their measured correlations. Pulse leakage into a reference or drift outside the cancelled polynomial family still creates bias.