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26 April 2024 |
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Article overview
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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 | Abstract: | 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. 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 | Services: | Forum | Review | PDF | Favorites |
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