  Automated method of full spectrum fitting gives reliable estimates of stellar
atmospheric parameters (Teff, logg and [Fe/H]) for late A, F, G and early K
type stars. Recently, the technique was further improved in the cooler regime
and the validity range was extended up to M6 - M7 spectral type( Teff
$\sim\,2900$ K). The present study aims to explore the application of this
method on the low-resolution spectra of Am stars, a class of chemically
peculiar (CP) stars, to examine its robustness for these objects. We use ULySS
with MILES (Medium-resolution INT Library of Empirical Spectra) V2 spectral
interpolator for parameter determination. Determined Teff and logg are found to
be in good agreement with those obtained from high-resolution spectroscopy.
