Detector baseline subtraction estimates the non-signal level of a photodetector readout and subtracts it before interpreting the desired signal. The baseline can include electronic offset, dark current and background light. Subtracting its estimated mean removes a bias contribution; it does not remove the random fluctuations that occurred in the measurement.
For a current readout over a detection time gate, a constant baseline estimate gives
If the true constant baseline is , its contribution to the charge error is . An original example has and a baseline overestimate of1nanoampere. The corrected charge is then10femtocoulombs too low. A longer gate amplifies this fixed baseline-estimation error linearly.
A finite baseline record also adds uncertainty. Suppose equally spaced signal-window samples and separate baseline samples each have independent zero-mean noise of variance , and the baseline estimate is their arithmetic mean. With spacing ,
The same estimated baseline is subtracted from every signal sample, so its error is shared rather than independently redrawn times. For , and , the standard uncertainty is about14.1femtocoulombs. Treating the baseline as known would give only10femtocoulombs. These are stipulated independent-noise values, not a detector specification.
Baseline drift motivates measuring the baseline near the signal in time. The SR250's active subtraction mode alternates signal-present and signal-absent triggers, reversing the baseline sample's sign before averaging.[ref] Cancellation depends on how well those samples represent the baseline during the signal; a source-correlated artifact need not cancel.
In pulse energy measurement with a photodiode, charge-to-energy conversion propagates this baseline error through , where is spectral responsivity. Baseline characterization is therefore part of the energy measurement, not merely a cosmetic shift of a plotted trace.
The temporal energy centroid of an optical pulse is its energy-weighted mean time. For nonnegative radiant power with finite positive energy and finite absolute first moment,
The normalization uses radiant energy as integrated radiant flux.[ref] The centroid is a moment of the energy-normalized pulse profile; it need not coincide with the largest power value, a threshold crossing or the middle of the FWHM interval.
For an original two-component example, let ninety percent of the energy belong to a symmetric narrow component centred at zero and ten percent to a symmetric component centred at . Linearity of the integral gives . Weak delayed energy can move the centroid even when the dominant peak remains near zero. Multiplying the whole power trace by a positive constant leaves unchanged; translating it by shifts its centroid by .
A detector response can shift the measured centroid too. Suppose a normalized impulse response and normalized optical profile have finite absolute first moments. For their convolution , direct integration with gives
Thus a causal exponential detector response of time constant shifts the recorded centroid by in this model. NIST's pulsed-radiometer characterization explicitly measures detector impulse responses and uses convolution to assess reproduced waveforms.[ref] The centroid identity is the independent moment calculation above.
Baseline drift can cause a separate shift. Suppose a true pulse has and , but a positive residual baseline of remains across the analysis window from to . Its added energy is , centred at . The resulting centroid is
A waveform measurement should therefore record the time window, baseline estimate and detector timing response with its reported centroid. A negative background-subtracted trace also needs care: it is not automatically a nonnegative energy distribution.