Pulse energy baseline correction ($U=\int (P-P_{\mathrm{bg}})dt$)

Pulse energy baseline correction subtracts the estimated non-pulse contribution before integrating a measurement trace. For a trace calibrated in power units over a gate $[t_0,t_1]$,The estimate $\hat{b}$ must have the same units as the integrated trace. Optical background and a detector-electronics offset enter at different stages of a physical measurement; a voltage offset cannot be subtracted directly from optical power without a response calibration.

An original drift example takes a $10\mu \mathrm{s}$ gate. Suppose pulse-free observations establish a baseline increasing linearly from $20$ to $40\mathrm{mW}$ across that gate. Its integrated contribution isIf the measured trace integrates to $1.50\mu \mathrm{J}$, the corrected estimate is $1.20\mu \mathrm{J}$. Subtracting only the initial $20\mathrm{mW}$ would yield $1.30\mu \mathrm{J}$, with a positive $0.10\mu \mathrm{J}$ error. This is a baseline-drift bias in pulse-energy integration in a stipulated linear model.

Historical NIST measurements took baselines before and after each run and averaged them to correct background and thermal drift. The leakage-background configuration was specified separately from a pulse injection.^[ref] Bracketing observations must genuinely represent the non-pulse signal; they cannot include an unrecognized pulse tail. Subtraction also cannot recover energy excluded by a detection time gate or repair a nonlinear detector. The Gaussian pulse time-gate energy fraction quantifies one profile-specific truncation effect.