LIRIS - Long-slit Intermediate Resolution Infrared Spectrograph

End year
2004
Organizational Unit
    Description

    LIRIS is an intermediate resolution spectrograph for the William Herschel 4.2 m telescope at the Observatorio del Roque de Los Muchachos. Thanks to an agreement with the Isaac Newton Group, it has been designed as a common-user instrument. Its observing modes are direct image and longslit and multi-slit spectroscopy. It is also capable of polarimetry and coronography. It was installed at the WHT in March 2004 for a period of three years. The LIRIS project is being led by the IAC with the participation of the Isaac Newton Group. During 2005 there was little activity whilst new devices like grisms and masks were incorporated, the latest software updates were applied and the documentation was completed.

    Principal investigator
    Project manager
    Project staff
    JESUS JIMENEZ FUENSALIDA
    VICENTE SANCHEZ DE LA ROSA
    F. Prada - Observatorio de Calar Alto
    M. Charcos-Llorens
    M.J. Vidal
    C. Eiroa - Universidad Autónoma de Madrid
    P. Garcia Lario - VILSPA
    R. Rutten - Isaac Newton Group of Telescopes- La Palma
    Jose Vilchez - Instituto de Astrofísica de Andalucía
    Collaborators
    Juan Maria Carranza
    Lluis Cavaller - GRANTECAN S.A.
    Isabel Escudero
    Javier Fuentes
    Marti Pi - GRANTECAN S.A.
    Jose Alberto Ballester
    Jorge Sos
    Jose Luis Iserte Vilar
    Nicolas Sosa
    Victor Padrón

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    Related installation
    LIRIS
    LIRIS
    Long-slit Intermediate Resolution Infrared Spectrograph
    Instrument
    Imaging
    Spectrograph