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26 April 2024
 
  » arxiv » astro-ph/0011062

 Article overview



CORMASS: A Compact and Efficient NIR Spectrograph for Studying Low-Mass Objects
J. C. Wilson ; M. F. Skrutskie ; M. R. Colonno ; A. T. Enos ; J. D. Smith ; C. P. Henderson ; J. E. Gizis ; D. G. Monet ; J. R. Houck ;
Date 2 Nov 2000
Subject astro-ph
Affiliation Cornell University, UMASS, IPAC, USNO Flagstaff Station
AbstractCorMASS (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. Its 2-dimensional spectral format provides simultaneous coverage from lambda ~ 0.75 microns to lambda ~ 2.5 microns (z’JHK bands). A remotely operated cold flip mirror permits its NICMOS3 detector to function as a K_s slit viewer to assist object placement into the 2 arcsec x 15 arcsec slit. CorMASS was primarily designed for the rapid spectral classification of low-mass stellar and sub-stellar objects identified by the Two-Micron All Sky Survey (2MASS). CorMASS’ efficiency and resolution also make it a versatile instrument for the spectral observation and classification of many other types of bright objects (K<14) including quasars, novae, and emission line objects.
Source arXiv, astro-ph/0011062
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