LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph): Assembly Integration and verification

Bibcode
2003SPIE.4841..160M
DOI
10.1117/12.458920
Manchado, A.; Barreto, Mary; Acosta-Pulido, Jose; Ballesteros Ramirez, Ezequiel; Correa, Santiago; Delgado, Jose M.; Dominguez-Tagle, Carlos; Hernández, Elvio; Lopez, Roberto L.; Manescau, Antonio; Moreno, Heidi; Prada, Francisco; Redondo, Pablo; Sanchez de la Rosa, Vicente; Sosa, Nicolas A.; Tenegi, Fabio
Bibliographical reference

Instrument Design and Performance for Optical/Infrared Ground-based Telescopes. Edited by Iye, Masanori; Moorwood, Alan F. M. Proceedings of the SPIE, Volume 4841, pp. 160-168 (2003).

Advertised on:
3
2003
Number of authors
16
IAC number of authors
16
Citations
2
Refereed citations
1
Description
LIRIS is a near-infrared (0.9 - 2.4 microns) intermediate resolution spectrograph (R = 1000-3000) conceived as a common user instrument for the (WHT) at the Observatorio del Roque de los Muchachos (ORM) La Palma. LIRIS is now being assembled, integrated and virified at the Instituto Astrofisico de Canarias (IAC). LIRIS will have imaging, long-slit and multi-object spectroscopy working modes. Coronography and polarimetry capabilities will eventually be added. Image capability will allow easy target acquisition.
Type
Non-refereed

It may interest you

  • Non-refereed
    EST preliminary design, status and future steps
    The European Solar Telescope (EST) aims to significantly improve our capabilities to observe the solar chromosphere and understanding the solar chromosphere represents one of the most challenging tasks in solar physics. EST incorporates the most innovative technology, with a simple and efficient design, and the most advanced instrumentation to
    Barreto, Mary et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..695B
    Citations
    0
  • Non-refereed
    The Galactic underdogs: characterizing a population of metal-poor stars with disc kinematics in the Milky Way
    To deepen our knowledge of the early history of the Milky Way, it is of particular interest to investigate the orbital and chemical properties of the most metal-poor stars, which are commonly associated with the oldest stars in our Universe. With the advent of astrometric (Gaia), spectroscopic (APOGEE, GALAH, LAMOST, Gaia-RVS), and photometric
    Gonzalez Rivera, Isaure et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..624G
    Citations
    0
  • Non-refereed
    Inferring stellar population properties from HST+JWST photometry using Normalizing Flows
    Spectral energy distributions (SEDs) encode information about the stellar populations within galaxies. By investigating the properties of these stars, such as their ages, masses, and metallicities, we can gain insights into the underlying physical processes that drive the growth and transformation of galaxies over cosmic time. For this purpose, we
    Iglesias Navarro, Patricia et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..225I
    Citations
    0