Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

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  • High-redshift BL Lac Objects: Spectroscopy of Candidates
    We report on 16 BL Lacertae objects that were proposed to be at z > 1. We present spectroscopic observations secured at the 10.4 m GTC that allowed us to assess the redshift of these sources. In particular, for five objects, we disprove the previous value of the redshift reported in the literature and found that they lie at z 1. Moreover, two of
    Landoni, M. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    23
  • High redshift galaxies in the ALHAMBRA survey. II. Strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 ≤ z≤ 4.5 by PDF analysis
    Context. Knowing the exact shape of the ultraviolet (UV) luminosity function (LF) of high-redshift galaxies is important to understand the star formation history of the early Universe. However, the uncertainties, especially at the faint and bright ends of the LFs, remain significant. Aims: In this paper, we study the UV LF of redshift z = 2.5 - 4.5
    Viironen, K. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    11
  • HARMONI pre-optics design at PDR
    HARMONI is a visible and near-infrared (0.5 to 2.45 μm) integral field spectrograph, providing the E-ELT's core spectroscopic capability, over a range of resolving powers from R (λ/Δλ) 3500 to 18000. The instrument provides simultaneous spectra of ˜32000 spaxels arranged in a sqrt(2):1 aspect ratio contiguous field. The pre-optics take light
    Cagigas, M. A. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    0
  • GTCAO real time AO closed loop software implementation and initial computer performance analysis
    The Gran Telescopio Canarias Adaptive Optics (GTCAO) is a single-conjugated post-focal system with a Shack Hartmann wavefront sensor working at visible wavelength and one Deformable Mirror (DM) conjugated to the pupil. GTCAO does not include a fast tip-tilt mirror in its optical bench so it relies on the telescope secondary mirror (M2) to correct
    Marco de la Rosa, J. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    0
  • GTC adaptive optics first performance tests in laboratory
    The GTC AO system designed and developed during the last years is based on a single deformable mirror with 21 x 21 actuators, conjugated to the telescope pupil, and a Shack-Hartmann wavefront sensor with 20 x 20 subapertures, using an OCAM2 camera. The GTCAO system will provide a corrected beam with a Strehl Ratio (SR) of 0.65 in K-band with bright
    Reyes García-Talavera, M. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    1
  • Gravitational lensing detection of an extremely dense environment around a galaxy cluster
    Galaxy clusters form at the highest-density nodes of the cosmic web1,2. The clustering of dark matter halos hosting these galaxy clusters is enhanced relative to the general mass distribution, with the matter density beyond the virial region being strongly correlated to the halo mass (halo bias)3. Halo properties other than mass can further enhance
    Sereno, M. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    21