Tipo de publicación: Sin árbitro

  • Publicación
    LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph): Assembly Integration and verification
    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...
  • Publicación
    LIRIS (long-slit intermediate-resolution infrared spectrograph): project status
    LIRIS is a near-IR intermediate resolution spectrograph with added capabilities for multi-object, imaging, coronography, and polarimetry. This instrument is now...
  • Publicación
    LIRIS Multi-slit Hα Spectroscopy of a z˜1 DEEP2 Sample of Star-forming Galaxies
    We present preliminary results of Hα near-infrared spectroscopy of six galaxies with redshifts z˜1 drawn from the DEEP2 Galaxy Redshift Survey. The spectra have...
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    LIRIS Observations of SN 2004ao
    The knowledge of the properties of supernovae (SNe) at optical wavelengths has experienced enormous progress in the current decade. In contrast, comparatively...
  • Publicación
    LIRIS: A Long-Slit Intermediate Resolution Infrared Sectrograph for the WHT
    LIRIS is an Instituto de Astrofísica de Canarias (IAC) project that consists in a near-infrared (0.9-2.4microns) intermediate resolution spectrograph...
  • Publicación
    LIRIS: a long-slit intermediate-resolution infrared spectrograph for the WHT
    The Instituto de Astrofisica de Canarias (IAC) is undertaking the design and construction of a common-user near IR spectrograph (LIRIS) for the Cassegrain focus...
  • Publicación
    LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization
    LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for...
  • Publicación
    Lithium Abundances Below the Substellar Limit
    Not Available
  • Publicación
    Lithium Abundances in a New Sample of Metal Deficient Dwarfs
    The authors have measured the Li abundance in a sample of 37 field dwarfs of low metallicity. Stars with [Fe/H] -1.4 ("EMD" stars) form a much more homogenous...