Tipo de publicación: Sin árbitro

  • Publicación
    First results using a new near-infrared 1% narrow-band filter in the GTC 10.4m telescope to detect galaxies at the dawn of the universe
    We present the first results using a new SCHOTT 1% narrow band filter in the near infrared for the CIRCE camera of the 10.4m GTC telescope. The goal of the...
  • Publicación
    First scientific observations with MEGARA at GTC
    On June 25th 2017, the new intermediate-resolution optical IFU and MOS of the 10.4-m GTC had its first light. As part of the tests carried out to verify the...
  • Publicación
    First Scientific Results from HORuS and GTC
    We present the first science results from the High Optical Resolution Spectrograph (HORuS), a cross-dispersed echelle spectrograph now in operation on the 10.4...
  • Publicación
    First Scientific Results of the Near Infrared Spectrograph LIRIS
    LIRIS is a near-infrared (1-2.5 microns) intermediate resolution spectrograph (R=1000-3000) with added capabilities for multi-slit, imaging, coronography, and...
  • Publicación
    First Simultaneous UBVRI Photopolarimetric Observations of a Sample of Normal Quasars
    Not Available
  • Publicación
    First steps of the GTC photometric calibration plan
    Large telescopes require a very precise calibration in order to maximize its scientific output. Current catalogues of standard stars are generally too bright...
  • Publicación
    First Steps toward Seismic Holography of the Tachocline
    The solar dynamo is thought to be generated at the tachocline and the deepest layers of the convection zone. Yet much about these layers or how this mechanism...
  • Publicación
    First Steps Towards the Electronic Inversion of the Radiative Transfer Equation
    The radiative transfer equation (RTE) gives us information about how the light streams through the medium. It must be inverted in order to obtain the properties...
  • Publicación
    First tests on the Integral Field Unit for GRIS at GREGOR
    The observation of the highly dynamic events in the chromosphere with current slit or filter spectropolarimeters is not adequate. With the sake of incresing the...