A Fourier transform (PT) spectrometer measures the autocorrelation (in
terferogram) of radiation emitted from a source and estimates the opti
cal power spectral density through application of the discrete Fourier
transform (DFT) to the recorded interferogram. Although a widely used
method, FT spectrometry suffers because its frequency resolution is l
imited to the sampling rate divided by the number of time-series data
points. A large number of points are therefore required to resolve an
optical spectrum properly. In this paper, it is shown that a noise-res
istant technique known as fast orthogonal search (FOS) can be used to
achieve accurate optical spectrum estimation. Further, it is shown tha
t frequency accuracy comparable to the DFT applied to the full interfe
rogram can be obtained with FOS even if the original interferogram is
contaminated with noise and then reduced by a factor of up to 10 by ir
regularly spaced sampling. The FOS application presented here is for t
he estimation of Raman spectra from interferograms acquired with an FT
Raman spectrometer.