  We give preliminary results from a spectroscopic study of composite spectrum
hot subdwarfs (sd+late-type). We obtained spectra of a sample of hot subdwarfs
selected from the "Catalogue of Spectroscopically Identified Hot Subdwarfs" on
the basis of near-infrared photometry from the Two Micron All Sky Survey
(2MASS). The sample consists of 20 photometric and spectroscopic single and 54
composite hot subdwarfs, 6 resolved (or barely resolved) visual doubles, and 5
objects with emission lines or broad absorption lines with emission cores.
Spectra of 84 "standard" (single late-type) stars with Hipparcos parallaxes
were also obtained for calibration. These observations cover 4600-8900 Ang with
3 Ang resolution. We measured equivalent width-like indices around Mg I b, Na I
D, the Ca II infrared triplet, H-alpha, and H-beta. Using the single late-type
star observations combined with model energy distributions, we explore how the
measured indices of a composite spectrum vary as the temperature and luminosity
of the late-type companion are varied and as the temperature and radius of the
hot subdwarf are varied. We use the measured indices of the composite systems
to estimate the temperature and gravity of the late-type star, taking into
account the dilution of its spectral features by light from the hot subdwarf.
