Tipo de publicación: Con árbitro

  • Publicación
    Accurate modeling of the forward-scattering Hanle effect in the chromospheric Ca I 4227 Å line
    Context. Measurable linear scattering polarization signals have been predicted and detected at the solar disk center in the cores of chromospheric lines. These...
  • Publicación
    Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265
    Context. The star HD 52265 is a G0V metal-rich exoplanet-host star observed in the seismology field of the CoRoT space telescope from November 2008 to March...
  • Publicación
    Accurate parameters for HD 209458 and its planet from HST spectrophotometry
    We present updated parameters for the star HD 209458 and its transiting giant planet. The stellar angular diameter θ = 0.2254 ± 0.0017 mas is obtained from the...
  • Publicación
    Accurate positions of candidate planetary nebulae in M 33
    We present new determinations of the positions of the planetary nebulae candidates found in Messier 33 by Magrini et al. (2000). The new coordinates have an...
  • Publicación
    Accurate sky signal reconstruction for ground-based spectroscopy with kinetic inductance detectors
    Context. Wide-field spectrometers are needed to deal with current astrophysical challenges that require multiband observations at millimeter wavelengths. An...
  • Publicación
    Accurately constraining velocity information from spectral imaging observations using machine learning techniques
    Determining accurate plasma Doppler (line-of-sight) velocities from spectroscopic measurements is a challenging endeavour, especially when weak chromospheric...
  • Publicación
    Acenes adducts with C70 fullerene: Anthracene, tetracene and pentacene
    Not Available
  • Publicación
    Acoustic oscillations and dynamo action in the G8 sub-giant EK Eridani
    We present further evidence of acoustic oscillations in the slowly rotating overactive G8 sub-giant EK Eri. This star was observed with the 1m Hertzsprung SONG...
  • Publicación
    Acoustic power absorption and enhancement generated by slow and fast MHD waves. Evidence of solar cycle velocity/intensity amplitude changes consistent with the mode conversion theory
    We used long duration, high quality, unresolved (Sun-as-a star) observations collected by the ground based network BiSON and by the instruments GOLF and VIRGO...