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

  • Very Small Array. Flux density at 33GHz (Cleary+, 2005)
    We describe the source subtraction strategy and observations for the extended Very Small Array (VSA), a cosmic microwave background interferometer operating at 33GHz. A total of 453 sources were monitored at 33GHz using a dedicated source subtraction baseline. 131 sources brighter than 20mJy were directly subtracted from the VSA visibility data
    Cleary, K. A. et al.

    Fecha de publicación:

    11
    2009
    Número de citas
    0
  • Very small grain emission in NGC 7023.
    We observed the reflection nebula NGC 7023 at various positions using wide and narrow band photometry centred on the 7.7 and 11.3μm PAH emission features and wide band photometry at 20 and 25μm. No significant variations have been detected over the nebula in the 7.3 and 20μm continuum relative to the total emission in the 6-15μm range (hereafter
    Laureijs, R. J. et al.

    Fecha de publicación:

    11
    1996
    Número de citas
    13
  • VI and [Fe/H] of Fornax dSph RGB stars (Battaglia+, 2006)
    We present the results of the DART imaging and CaII triplet (CaT) survey of the Fornax dwarf spheroidal galaxy (dSph) at ESO. We collected hundreds of low resolution spectra of Red Giant Branch (RGB) stars in the CaT region, using VLT/FLAMES in Medusa mode, with the GIRAFFE spectrograph (grating LR8, resolving power R~6500). We list the results for
    Battaglia, G. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    0
  • VII Zw403 - a BCD galaxy with an X-ray emission excess.
    VII Zw403 is a nearest BCD galaxy. This izolated system is so close (~4.5 Mp c), that it makes it possible to study it's star forming regions with unprecedently great details. recent X-ray observations (Papaderos et al. 1994) added more interest to the system, as revealed an extended, kpc-scale region of the diffuse X-ray emission. We use our
    Silich, S. et al.

    Fecha de publicación:

    11
    2000
    Número de citas
    0
  • VIRGO: The solar monitor experiment on SOHO
    The Variability of solar IRradiance and Gravity Oscillations (VIRGO) experiment contains two types of active cavity radiometers for monitoring of the solar constant, two three channel sunphotometers for the measurement of spectral irradiance at 335, 500 and 865 nm and a low resolution imager with 12 pixels. The main scientific objective is probing
    Froehlich, C. et al.

    Fecha de publicación:

    11
    1988
    Número de citas
    0
  • Visible and near-infrared spectroscopic survey of Jupiter Trojan asteroids: investigation of dynamical families
    Trojan asteroids located in the Jupiter Lagrangian points L4 and L5 (60 degrees ahead and behind Jupiter) are widely believed to be primordial bodies since their orbits are stable over the age of the Solar System. They seem to have been formed in a region of the solar nebula rich in frozen volatiles and to have never suffered selective induction
    Dotto, E. et al.

    Fecha de publicación:

    11
    2004
    Número de citas
    0