LIRIS (Long-Slit Intermediate Resolution Infrared Spectrograph)

Project status
  • A. Manchado
  • M. Barreto
  • J. Acosta-Pulido
  • F. Prada
  • C. Domínguez-Tagle
  • E. Ballesteros
  • S. Correa
  • J. M. Delgado
  • R. López
  • A. Manescau
  • H. Moreno
  • J. Rasilla
  • P. Redondo
  • V. Sánchez
Conference paper

Abstract

LIRIS is a near-infrared (0.9–2.4 microns) intermediate resolution spectrograph (R = 1000 – 8000) 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 4.2 m William Herschel Telescope (WHT) at the Observatorio del Roque de Los Muchachos (ORM, La Palma).

Keywords

Test Bench Starburst Galaxy Intermediate Resolution Spectroscopic Mode Stellar Kinematic 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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References

  1. Manchado A., Fuentes F.J., Prada F. et al., 1998, SPIE, 3354, 448ADSCrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 2001

Authors and Affiliations

  • A. Manchado
    • 1
  • M. Barreto
    • 1
  • J. Acosta-Pulido
    • 1
  • F. Prada
    • 2
  • C. Domínguez-Tagle
    • 1
  • E. Ballesteros
    • 1
  • S. Correa
    • 1
  • J. M. Delgado
    • 1
  • R. López
    • 1
  • A. Manescau
    • 1
  • H. Moreno
    • 1
  • J. Rasilla
    • 1
  • P. Redondo
    • 1
  • V. Sánchez
    • 1
  1. 1.Instituto de Astrofísica de CanariasLa Laguna, TenerifeSpain
  2. 2.Centro Astronómico Hispano-AlemánAlmeríaSpain

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