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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  • COSMOSOMAS observations of the cosmic microwave background and Galactic foregrounds at 11 GHz: evidence for anomalous microwave emission at high Galactic latitude
    We present observations with the new 11-GHz radiometer of the COSMOSOMAS experiment at the Teide Observatory (Tenerife). The sky region between 0°
    Hildebrandt, S. R. et al.

    Fecha de publicación:

    12
    2007
    Número de citas
    30
  • Cross-correlation of SDSS DR7 Quasars and DR10 BOSS Galaxies: The Weak Luminosity Dependence of Quasar Clustering at z ~ 0.5
    We present the measurement of the two-point cross-correlation function (CCF) of 8198 Sloan Digital Sky Survey Data Release 7 quasars and 349,608 Data Release 10 CMASS galaxies from the Baryonic Oscillation Spectroscopic Survey at 0.3 < z < 0.9. The CCF can be reasonably well fit by a power-law model ξQG(r) = (r/r 0)–γ on projected scales of rp = 2
    Shen, Y. et al.

    Fecha de publicación:

    12
    2013
    Número de citas
    103
  • Cross-Correlation of Tenerife Data with Galactic Templates-Evidence for Spinning Dust?
    The recent discovery of dust-correlated diffuse microwave emission has prompted two rival explanations: free-free emission and spinning dust grains. We present new detections of this component at 10 and 15 GHz by the switched-beam Tenerife experiment. The data show a turnover in the spectrum and thereby support the spinning dust hypothesis. We also
    de Oliveira-Costa, Angélica et al.

    Fecha de publicación:

    12
    1999
    Número de citas
    101
  • Damping of Fast Magnetohydrodynamic Oscillations in Quiescent Filament Threads
    High-resolution observations provide evidence of the existence of small-amplitude transverse oscillations in solar filament fine structures. These oscillations are believed to represent fast magnetohydrodynamic (MHD) waves and the disturbances are seen to be damped in short timescales of the order of 1 to 4 periods. We propose that, due to the
    Arregui, I. et al.

    Fecha de publicación:

    12
    2009
    Número de citas
    0
  • Dark matter searches with Cherenkov telescopes: nearby dwarf galaxies or local galaxy clusters?
    In this paper, we compare dwarf galaxies and galaxy clusters in order to elucidate which object class is the best target for gamma-ray DM searches with imaging atmospheric Cherenkov telescopes (IACTs). We have built a mixed dwarfs+clusters sample containing some of the most promising nearby dwarf galaxies (Draco, Ursa Minor, Wilman 1 and Segue 1)
    Sánchez-Conde, M. A. et al.

    Fecha de publicación:

    12
    2011
    Número de citas
    89