Bibcode
                                    
                            Manchado, A.; Barreto, Mary; Acosta-Pulido, Jose; Prada, Francisco; Dominguez-Tagle, Carlos; Correa, Santiago; Fragoso-Lopez, Ana B.; Fuentes, F. Javier; Iserte, Jose L.; Joven-Alvarez, Enrique; Lopez, Roberto; Manescau, Antonio; Moreno-Arce, Heidy; Padron, Victor; Rasilla, Jose Luis; Redondo, Pablo; Sanchez, Vicente; Sosa, Nicolas A.; Atad-Ettedgui, Eli; Hastings, Peter R.
    Bibliographical reference
                                    Proc. SPIE Vol. 4008, p. 1162-1171, Optical and IR Telescope Instrumentation and Detectors, Masanori Iye; Alan F. Moorwood; Eds.
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                        8
            
                        2000
            
  Citations
                                    6
                            Refereed citations
                                    2
                            Description
                                    LIRIS is a near-IR intermediate resolution spectrograph with added
capabilities for multi-object, imaging, coronography, and polarimetry.
This instrument is now being constructed at the IAC, and upon complexion
will be installed on the 4.2m William Herschel Telescope at the
Observatorio del Roque de Los Muchachos. The optical system uses lenses
and is based on a classical collimator/camera design. Grisms are used as
the dispersion elements. The plate scale matches the median seeing at
the ORM. The detector is a Hawaii 1024 X 1024 HgCdTe array operating at
60K.