  We present medium resolution (R = 5000-6000) spectra in the near-infrared
band, 1.4-1.8 microns, for template stars in G, K, and M types observed by the
echelle spectrometer, IRCS, at the SUBARU 8.2 m telescope. The identification
of lines is based on the spectra of Arcturus (K2 III) in the literature. We
measured the equivalent of widths and compared our results to those of Meyer et
al. (1998). We conclude that our spectral resolution (R = 6000) data can
investigate more accurately the properties of lines in stellar spectra. The
library of the template stellar spectra in ASCII format are available for
download on the World Wide Web.
