  We present ROBOSPECT, a new code to automatically measure and deblend line
equivalent widths for both absorption and emission spectra. We test the
accuracy of these measurements against simulated spectra as well as manual
equivalent width measurements of five stellar spectra over a range of
signal-to-noise values and a set of long slit emission spectra. We find that
ROBOSPECT accurately matches both the synthetic and manual measurements, with
scatter consistent with the expectations based on the data quality and the
results of Cayrel (1988).
