Tipo de publicación: Con árbitro

  • Publicación
    First results from the POMME survey of M31
    The POMME survey (Pixel Observations of M31 with MEgacam) monitored two fields in the disc of M31 using MegaCam at CFHT over a timespan of 2.5 months in three...
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    First results from the Very Small Array - I. Observational methods
    The Very Small Array (VSA) is a synthesis telescope designed to image faint structures in the cosmic microwave background on degree and sub-degree angular...
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    First results from the Very Small Array - II. Observations of the cosmic microwave background
    We have observed the cosmic microwave background (CMB) temperature fluctuations in eight fields covering three separated areas of sky with the Very Small Array...
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    First results from the Very Small Array - III. The cosmic microwave background power spectrum
    We present the power spectrum of the fluctuations in the cosmic microwave background detected by the Very Small Array (VSA) in its first season of observations...
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    First results from the Very Small Array - IV. Cosmological parameter estimation
    We investigate the constraints on basic cosmological parameters set by the first compact-configuration observations of the Very Small Array (VSA), and other...
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    First Results from VIRGO, the Experiment for Helioseismology and Solar Irradiance Monitoring on SOHO
    Not Available
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    First results of an Hα based search of classical Be stars in the Perseus Arm and beyond
    We investigate a region of the Galactic plane, between 120° ≤ ℓ ≤ 140° and -1° ≤ b ≤ +4°, and uncover a population of moderately reddened (E(B - V) ˜ 1)...
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    First Results on it P Modes from GOLF Experiment
    The GOLF experiment on the SOHO mission aims to study the internal structure of the Sun by measuring the spectrum of global oscillations in the frequency range...
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    First simultaneous UBVRI photopolarimetric observations of a sample of normal quasars
    We present what we believe to be the first truly simultaneous UBVRI photopolarimetric results for a sample of eight 'normal' quasars. In five of these quasars...