Publicaciones

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  • Sin árbitro
    Comparison of the Calibrated MDI and GOLF Signals. V. The Low Frequency p-Modes
    Low-frequency p-modes have relatively small amplitudes and are set against the background of granulation on the solar surface. In this work, the calibrated signals of both the MDI and GOLF instruments are processed in the following steps: 1) prewhitening 2) signal extraction and demodulation in given frequency bands and 3) separation of noise and
    Varadi, F. et al.

    Fecha de publicación:

    0
    1998
    Bibcode
    1998ESASP.418..359V
    Número de citas
    2
  • Sin árbitro
    Comparison of the Calibrated MDI and GOLF Signals. IV. p-Mode Energy Budget
    The energy calculation of the p-modes requires accurate estimates of both amplitudes and linewidths. These parameters can be derived from a suitable model used to fit the spectral distribution of the mode. In this poster we describe the technique used to achieve this goal. The model chosen to represent the power spectrum of a solar oscillation is a
    Bertello, L. et al.

    Fecha de publicación:

    0
    1998
    Bibcode
    1998ESASP.418..121B
    Número de citas
    16
  • Sin árbitro
    Compact Galaxies at Z = 0. 2 - 1. 3: Implications for Galaxy Evolution and the Star Formation History of the Universe
    The authors have studied the global properties of 51 compact field galaxies with redshifts z ≡ 0.2 - 1.3 and apparent magnitudes I814 23.74 in the flanking fields of the Hubble Deep Field. Keck spectra covering ≡4000 - 8000 Å, combined with HST I814 images and Keck V band images were used to derive redshifts, V606 - I814 colors, absolute blue
    Guzmán, R. et al.

    Fecha de publicación:

    0
    1998
    Bibcode
    1998HiA....11..147G
    Número de citas
    0