In recent years, astronomical photometry has been revolutionised by space
missions such as MOST, CoRoT and Kepler. However, despite this progress,
high-quality spectroscopy is still required as well. Unfortunately,
high-resolution spectra can only be obtained using ground-based telescopes, and
since many interesting targets are rather faint, the spectra often have a
relatively low S/N. Consequently, we have developed an algorithm based on the
least-squares deconvolution profile, which allows to reconstruct an observed
spectrum, but with a higher S/N. We have successfully tested the method using
both synthetic and observed data, and in combination with several common
spectroscopic applications, such as e.g. the determination of atmospheric
parameter values, and frequency analysis and mode identification of stellar
pulsations.Comment: Proceedingspaper, 8 pages, 4 figures, appears in "Setting a New
Standard in the Analysis of Binary Stars", Eds K. Pavlovski, A. Tkachenko,
and G. Torres, EAS Publications Serie
