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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  • Sin árbitro
    ELAIS deep X-ray survey. I. (Manners+, 2003)
    The ELAIS Deep X-ray Survey (EDXS) is being conducted in the northern ELAIS regions N1 and N2. The Chandra data consist of approximately 75 ks exposures in each field. Region N1 was observed on 2000 August 3-4 (OBSID 888) and N2 on 2000 August 2-3 (OBSID 887). The nominal aimpoints were: N1, 16:10:20.11 +54:33:22.3; and N2, 16:36:46.99 +41:01:33.7
    Manners, J. C. et al.

    Fecha de publicación:

    1
    2004
    Bibcode
    2004yCat..73430293M
    Número de citas
    0
  • Con árbitro
    Determination of near-surface attenuation, with @k parameter, to obtain the seismic moment, stress drop, source dimension and seismic energy for microearthquakes in the Granada Basin (Southern Spain)
    Not Available
    Garcia Garcia, J. M. et al.

    Fecha de publicación:

    1
    2004
    Bibcode
    2004PEPI..141....9G
    Número de citas
    22
  • Sin árbitro
    Coupled Fast and Alfvén MHD Waves in Sheared Coronal Arcades
    The magnetohydrodynamic (MHD) normal modes of oscillation of sheared coronal arcades including longitudinal wave propagation are studied. Solutions have been computed in order to ascertain the effects of the longitudinal magnetic field component, By, and of the longitudinal propagation, ky in these structures. Our results show that whenever By = 0
    Arregui, I. et al.

    Fecha de publicación:

    1
    2004
    Bibcode
    2004ESASP.547..447A
    Número de citas
    0
  • Sin árbitro
    Comet C/2003 WT_42 (LINEAR)
    IAUC 8270 available at Central Bureau for Astronomical Telegrams.
    Binzel, R. P. et al.

    Fecha de publicación:

    1
    2004
    Bibcode
    2004IAUC.8270....1B
    Número de citas
    1
  • Sin árbitro
    Colour-correlated noise: can it improve the S/N of the Eddington data?
    In this paper we use the SoHO/VIRGO three colour time series data to investigate how colour correlated stellar signal and noise may be used to improve the S/N of the Eddington time series. We conclude that one may implement a two-colour system on Eddington in order to reduce the amount of noise at low frequencies. We propose a blue and a red broad
    Kjeldsen, H. et al.

    Fecha de publicación:

    1
    2004
    Bibcode
    2004ESASP.538..335K
    Número de citas
    0