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

  • Con árbitro
    Gamma-ray Excess from a Stacked Sample of High- and Intermediate-frequency Peaked Blazars Observed with the MAGIC Telescope
    Between 2004 and 2009, a sample of 28 X-ray selected high- and intermediate-frequency peaked blazars with an X-ray flux larger than 2 μJy at 1 keV in the redshift range from 0.018 to 0.361 was observed with the MAGIC telescope at energies above 100 GeV. Seven among them were detected and the results of these observations are discussed elsewhere
    Aleksić, J. et al.

    Fecha de publicación:

    3
    2011
    Bibcode
    2011ApJ...729..115A
    Número de citas
    29
  • Con árbitro
    Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0
    We present the galaxy stellar mass function and its evolution in clusters from z˜ 0.8 to the current epoch, based on the WIde-field Nearby Galaxy-cluster Survey (WINGS) (0.04 ≤z≤ 0.07), and the ESO Distant Cluster Survey (EDisCS) (0.4 ≤z≤ 0.8). We investigate the total mass function and find that it evolves noticeably with redshift. The shape at M*
    Vulcani, Benedetta et al.

    Fecha de publicación:

    3
    2011
    Bibcode
    2011MNRAS.412..246V
    Número de citas
    110
  • Sin árbitro
    Galaxies and quasars in the early Universe: recent results and future prospects from sub-millimeter observations
    Not Available
    Cox, P.

    Fecha de publicación:

    3
    2011
    Bibcode
    2011iac..talk..201C
    Número de citas
    0
  • Con árbitro
    Fossil groups origins. I. RX J105453.3+552102 a very massive and relaxed system at z ~ 0.5
    Context. The most accepted scenario for the origin of fossil groups is that they are galaxy associations in which the merging rate was fast and efficient. These systems have assembled half of their mass at early epoch of the Universe, subsequently growing by minor mergers, and therefore could contain a fossil record of the galaxy structure
    Aguerri, J. A. L. et al.

    Fecha de publicación:

    3
    2011
    Bibcode
    2011A&A...527A.143A
    Número de citas
    43
  • Errata
    Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans (Corrigendum)
    Not Available
    Tafelmeyer, M. et al.

    Fecha de publicación:

    3
    2011
    Bibcode
    2011A&A...527C...1T
    Número de citas
    2
  • Errata
    Erratum: "The Iron Abundance in Galactic Planetary Nebulae" (2009, ApJ, 694, 1335)
    Not Available
    Delgado-Inglada, G. et al.

    Fecha de publicación:

    3
    2011
    Bibcode
    2011ApJ...729...77D
    Número de citas
    0