The results of a search for cool subdwarfs are presented .
Kinematic ( U , V , and W ) and stellar parameters ( T _ { eff } , log g , [ Fe/H ] , and \xi _ { t } ) are derived for 134 candidate subdwarfs based on high resolution spectra .
The observed stars span 4200K < T _ { eff } < 6400K and -2.70 < [ Fe/H ] < 0.25 including only 8 giants ( log g < 4.0 ) .
Of the sample , 100 stars have MgH bands present in their spectra .
The targets were selected by their large reduced proper-motion , the offset from the solar metallicity main sequence , or culled from the literature .
We confirm the claims made by Ryan ( 41 ) regarding the NLTT catalog being a rich source of subdwarfs and verify the success of the reduced proper-motion constraint in identifying metal-poor stars .