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

  • Planck 2013 results. III. LFI systematic uncertainties
    We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. We also present an overall budget of
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    53
  • Planck 2013 results. II. Low Frequency Instrument data processing
    We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5 months of operations at 30, 44, and 70 GHz. In particular, we discuss the various steps involved in reducing the data, from telemetry packets through to the production of
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    79
  • Planck 2013 results. I. Overview of products and scientific results
    The European Space Agency’s Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    1000
  • Physical properties of asteroids derived from a novel approach to modeling of optical lightcurves and WISE thermalinfrared data
    Convex shape models and spin vectors of asteroids are now routinely derived from their disk-integrated lightcurves by the lightcurve inversion method of Kaasalainen et al. (2001, Icarus 153, 37). These shape models can be then used in combination with thermal infrared data and a thermophysical model to derive other physical parameters - size
    Durech, J. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    0
  • On the Reliability of Microvariability Tests in Quasars
    Microvariations probe the physics and internal structure of quasars. Unpredictability and small flux variations make this phenomenon elusive and difficult to detect. Variance-based probes such as the C and F tests, or a combination of both, are popular methods to compare the light curves of the quasar and a comparison star. Recently, detection
    de Diego, J. A.

    Fecha de publicación:

    11
    2014
    Número de citas
    46
  • On the Orientation of Prehistoric Sardinian Monuments: A Comparative Statistical Approach
    On the basis of a recently updated data base of Sardinian Megalithic monuments, we perform two independent statistical analyses on several groups of these structures and confirm the existence of differences between the southern and northern halves of Sardinia, indicating that there seem to be different traditions of orientation in these two parts
    González García, A. C. et al.

    Fecha de publicación:

    11
    2014