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

  • A tale of two GRB-SNe at a common redshift of z=0.54
    We present ground-based and Hubble Space Telescope optical observations of the optical transients (OTs) of long-duration Gamma Ray Bursts (GRBs) 060729 and 090618, both at a redshift of z= 0.54. For GRB 060729, bumps are seen in the optical light curves (LCs), and the late-time broad-band spectral energy distributions (SEDs) of the OT resemble
    Cano, Z. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    89
  • A search for radio counterparts to Chandra ULX candidates
    We present a systematic search for radio counterparts to Ultraluminous X-ray (ULX) source candidates based on a cross-correlation of the Swartz et al. (2004) ULX catalogue based on Chandra data and the FIRST radio survey. We find seven cases of conspicuous peaks of radio emission that could be associated to ULX sources. Among these seven ULX radio
    Pérez-Ramírez, D. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    4
  • A Peculiar Young Eruptive Star in the Dark Cloud Lynds 1340
    We conducted a long-term optical photometric and spectroscopic monitoring of the strongly variable, accreting young sun-like star [KOS94] HA11, associated with the dark cloud Lynds 1340 that exhibited large amplitude (5-6 mag in the I C band) brightness variations on 2-3 years timescales, flat spectral energy distribution (SED), and extremely
    Kun, M. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    21
  • A high-resolution three-dimensional model of the solar photosphere derived from Hinode observations
    A new three-dimensional model of the solar photosphere is presented in this paper and made publicly available to the community. This model has the peculiarity of having been obtained by inverting spectro-polarimetric observations, rather than by using numerical radiation hydrodynamical simulations. The data used here are from the spectro
    Socas-Navarro, H.

    Fecha de publicación:

    5
    2011
    Número de citas
    42
  • Which haloes host Herschel-ATLAS galaxies in the local Universe?
    We measure the projected cross-correlation between low-redshift (z 0.5) far-infrared selected galaxies in the science demonstration phase (SDP) field of the Herschel-ATLAS (H-ATLAS) survey and optically selected galaxies from the Galaxy and Mass Assembly (GAMA) redshift survey. In order to obtain robust correlation functions, we restrict the
    Guo, Qi et al.

    Fecha de publicación:

    4
    2011
    Número de citas
    18
  • Unnoticed Magnetic Field Oscillations in the Very Quiet Sun Revealed by SUNRISE/IMaX
    We present observational evidence for oscillations of magnetic flux density in the quiet areas of the Sun. The majority of magnetic fields on the solar surface have strengths of the order of or lower than the equipartition field (300-500 G). This results in a myriad of magnetic fields whose evolution is largely determined by the turbulent plasma
    Martínez-González, M. J. et al.

    Fecha de publicación:

    4
    2011
    Número de citas
    43