Publication type: Refereed

  • Publication
    A measurement of galaxy halo mass from the surrounding H I Lyα absorption
    We measure the dark matter halo masses of ≈ 2.36 UV colour-selected star-forming galaxies by matching the observed median H I Lyα absorption around them, as...
  • Publication
    A measurement of the background solar velocity spectrum
    Ten years of continuous measurements of the radial velocity of the Sun have been used to estimate the contribution of various solar surface phenomena to the...
  • Publication
    A Measurement of the Galactic Rotation in the 4TH Quadrant
    Using the VLA and the VLBA we have observed water maser emission in the proto-planetary nebula candidate IRAS 19134+2131, in which the water maser spectrum has...
  • Publication
    A measurement of the I = I solar rotational splitting
    A precise measurement of the l = 1 rotational splitting has been derived from the 1991 IRIS data and it leads to a moderate rotation rate in the solar core.
  • Publication
    A meta-analysis of the magnetic line broadening in the solar atmosphere
    A multiline Bayesian analysis of the Zeeman broadening in the solar atmosphere is presented. A hierarchical probabilistic model, based on the simple but...
  • Publication
    A metamaterial with applications in broad band antennas used in radio astronomy and satellite communications
    Electromagnetic metamaterials at microwave frequencies are well established in industry and research. Recent work has shown how a specific kind of metallic...
  • Publication
    A meteorological and photometric study of the Oukaimeden site. Comparison with the Observatorio del Roque de los Muchachos using Carlsberg Automatic Meridian Circle data
    In this paper, we present meteorological and photometric studies of the Oukaimeden astronomical site in Morocco. The meteorological measurements were obtained...
  • Publication
    A Methane, Isolated, Planetary-Mass Object in Orion
    We report on the discovery of a free-floating methane dwarf toward the direction of the young star cluster σ Ori. Based on the object's far-red, optical, and...
  • Publication
    A method to deconvolve stellar profiles. The non-rotating line utilizing Gaussian sum approximation
    Context. Currently, one of the standard procedures used to determine stellar and wind parameters of massive stars involves to comparing the observed spectral...