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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  • Asteroseismology from multi-month Kepler photometry: the evolved Sun-like stars KIC 10273246 and KIC 10920273
    Context. The evolved main-sequence Sun-like stars KIC 10273246 (F-type) and KIC 10920273 (G-type) were observed with the NASA Kepler satellite for approximately ten months with a duty cycle in excess of 90%. Such continuous and long observations are unprecedented for solar-type stars other than the Sun. Aims: We aimed mainly at extracting estimates
    Campante, T. L. et al.

    Fecha de publicación:

    10
    2011
    Número de citas
    77
  • Asteroseismology of the Delta Scuti star V650 Tauri
    The preliminary results of a multisite photometric campaign on the Pleiades Delta Scuti variable V650 Tauri are reported. The star was observed photometrically for 14 days during 2008 November from three observatories distributed in Longitude around the Earth. As a result of the preliminary analysis we have detected in V650 Tauri at least nine
    Fox Machado, L. et al.

    Fecha de publicación:

    10
    2011
    Número de citas
    4
  • Atmospheric turbulence profiling at the Teide Observatory: comparison and calibration of SODAR and SCIDAR measurements
    In order to characterized the vertical atmospheric structure at the Teide Observatory (Tenerife, Spain), we are using two different remote sensing technics: SODAR (SOund Detection And Ranging) and SCIDAR (SCIncitillation Detection And Ranging) at this astronomical site. We present in this work the preliminar results on the comparison of the
    de la Nuez Cruz, A. et al.

    Fecha de publicación:

    10
    2007
    Número de citas
    0
  • Atomic Scattering Polarization. Observations, Modeling, Predictions
    This paper highlights very recent advances concerning the identification of new mechanisms that introduce polarization in spectral lines, which turn out to be key for understanding some of the most enigmatic scattering polarization signals of the solar visible spectrum. We also show a radiative transfer prediction on the scattering polarization
    Trujillo Bueno, J. et al.

    Fecha de publicación:

    10
    2015
    Número de citas
    0
  • Automated analysis of stellar spectra
    Classical model-atmosphere analyses of stellar spectra usually begin by measuring equivalent widths, and then proceed into a loop in which 1) model spectra are calculated for a set of abundances and atmospheric parameters, and 2) observed and computed spectra are compared and corrections to the abundances and parameters are inferred. Automated
    Allende Prieto, C.

    Fecha de publicación:

    10
    2004
    Número de citas
    35
  • Automated analysis of stellar spectra: application to the GAUDI
    In this paper we describe a methodology to be used for the automated analysis of the spectroscopic contents of the GAUDI archive. We perform chi-square minimisation in the 5000-5200 Å spectral window to infer the atmospheric parameters and their random internal uncertainties. Effective temperatures are anchored using a zero-point correction into
    Solano, E. et al.

    Fecha de publicación:

    10
    2008
    Número de citas
    0