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CorMASS (Cornell Massachusetts Slit Spectrograph) is a compact,low-resolution (R=300), double-pass prism cross-dispersed near-infrared (NIR)spectrograph in operation on the Palomar Observatory 60-inch telescope. Its2-dimensional spectral format provides simultaneous coverage from lambda ~ 0.75microns to lambda ~ 2.5 microns (z'JHK bands). A remotely operated cold flipmirror permits its NICMOS3 detector to function as a K_s slit viewer to assistobject placement into the 2 arcsec x 15 arcsec slit. CorMASS was primarilydesigned for the rapid spectral classification of low-mass stellar andsub-stellar objects identified by the Two-Micron All Sky Survey (2MASS).CorMASS' efficiency and resolution also make it a versatile instrument for thespectral observation and classification of many other types of bright objects(K<14) including quasars, novae, and emission line objects.Comment: To be published in Feb 2001 PASP, 19 pages, 12 Figures, High  Resolution file can be retrieved from  ftp://iras2.tn.cornell.edu/pub/wilson/papers/cormass.ps.g

CorMASS: A Compact and Efficient Near‐Infrared Spectrograph for Studying Low‐Mass Objects