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. XXXI. Consistency of the Planck data
    The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the comparison of the 70 GHz (amplifier) and 100 GHz (bolometer) channels. Based on different instrument technologies, with feeds located differently in the focal plane, analysed
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    73
  • Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
    We present new measurements of cosmic infrared background (CIB) anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross-frequency power spectrum is measured from 143 to 3000 GHz, and the auto-bispectrum from 217 to 545 GHz. The total areas used to compute the CIB power spectrum and bispectrum are about 2240 and 4400
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    262
  • Planck 2013 results. XXVIII. The Planck Catalogue of Compact Sources
    The Planck Catalogue of Compact Sources (PCCS) is the catalogue of sources detected in the first 15 months of Planck operations, the “nominal” mission. It consists of nine single-frequency catalogues of compact sources, both Galactic and extragalactic, detected over the entire sky. The PCCS covers the frequency range 30–857 GHz with higher
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    184
  • Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
    Our velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30 years, and has an accepted amplitude of v/c = 1.23 × 10-3, or v = 369. In addition to this signal generated by Doppler boosting of the CMB monopole, our motion also
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    249
  • Planck 2013 results. XXVI. Background geometry and topology of the Universe
    The new cosmic microwave background (CMB) temperature maps from Planck provide the highest-quality full-sky view of the surface of last scattering available to date. This allows us to detect possible departures from the standard model of a globally homogeneous and isotropic cosmology on the largest scales. We search for correlations induced by a
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    146
  • Planck 2013 results. XXV. Searches for cosmic strings and other topological defects
    Planck data have been used to provide stringent new constraints on cosmic strings and other defects. We describe forecasts of the CMB power spectrum induced by cosmic strings, calculating these from network models and simulations using line-of-sight Boltzmann solvers. We have studied Nambu-Goto cosmic strings, as well as field theory strings for
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    355