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..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • VPHGs for WEAVE: design, manufacturing and characterization
    WEAVE is the next-generation optical spectroscopy facility for the William Herschel Telescope (WHT). It shows two channels (blue and red) and two working modes, a low-resolution (R=3,000-7,500) and a high-resolution (R=13,000- 25,000). The dispersing elements of the spectrograph are Volume Phase Holographic Gratings (VPHGs), two for the lower
    Bianco, Andrea et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    3
  • Using clustering for disperse objects fields segmentation in MIRADAS instrument
    Mid-resolution InfRAreD Astronomical Spectrograph (MIRADAS), a near-infrared multi-object spectrograph for Gran Telescopio Canarias (GTC), has 12 deployable optomechanical Integral Field Units (IFU). Based on a robotic probe arm with a pick-off mirror, each of these units can observe a different user-defined sky object. MIRADAS can work with target
    Sabater, Josep et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    0
  • Uplink correction demonstrator: test bench and experimental results
    The Uplink Wavefront Corrector System (UWCS) has been conceived by following the premises from simulation outcomes as a pathfinder instrument to demonstrate Adaptive Optics uplink correction in both applications: Free-Space Optical Communications and self-propagating path of Laser Guide Stars. Preliminary design and expected performance have been
    Martínez, Noelia et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    0
  • Unidentified quasars among stationary objects from Gaia DR2
    Here we apply a technique selecting quasar candidates purely as sources with zero proper motions in the Gaia data release 2 (DR2). We demonstrate that this approach is highly efficient toward high Galactic latitudes with ≲25% contamination from stellar sources. Such a selection technique offers very pure sample completeness, since all cosmological
    Heintz, K. E. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    22
  • Towards an improvement in the spectral description of central stars of planetary nebulae
    Context. There are more than 3000 known Galactic planetary nebulae, but only 492 central stars of Galactic planetary nebulae (CSPN) have known spectral types. It is vital to increase this number in order to have reliable statistics, which will lead to an increase of our understanding of these amazing objects. Aims: We aim to contribute to the
    Weidmann, W. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    11
  • Toward the uplink correction: application of adaptive optics techniques on free-space optical communications through the atmosphere
    The optical ground station (OGS), installed in the Teide Observatory since 1995, was built as part of ESA efforts in the research field of satellite optical communications to test laser telecommunication terminals on board of satellites in Low Earth Orbit and Geostationary Orbit. As far as one side of the link is settled on the Earth, the laser
    Martínez, N. et al.

    Fecha de publicación:

    7
    2018
    Número de citas
    9