Publicaciones

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  • High-resolution IBIS Observations and Comparison with 3D Simulations
    We present first comparisons between high resolution observations of the quiet photosphere, obtained with the Interferometric BIdimensional Spectrometer (IBIS) in the non-magnetic Fe I 7090.4 Å spectral line, and the synthetic spectrum calculated for a 3D snapshot of a radiation-hydrodynamical simulation of the solar atmosphere. Together with
    Cauzzi, G. et al.

    Fecha de publicación:

    12
    2006
    Número de citas
    2
  • High-resolution Observations of Siphon Flows in a Solar Magnetic Pore
    We investigate signatures of siphon flows in a region around a solar magnetic pore, observed in the photosphere at μ = 0.6, during its decay phase. We analyze high-resolution Stokes spectra acquired by Hinode/Solar Optical Telescope along the Fe I pair at 630.2 nm. We determine the vector magnetic field and the line-of-sight velocity by an
    Guglielmino, S. L. et al.

    Fecha de publicación:

    12
    2011
    Número de citas
    5
  • High-resolution solar polarimetry with Sunrise
    Sunrise is a solar telescope with an aperture of 1 m, and is dedicated for spectropolarimetric measurements in the visible and the near UV. The total wavelength range is 200 to 1000 nm for narrowband imaging and diagnostic spectroscopy. Sunrise is planned as a stratospheric long-duration balloon mission with a first flight in 2006
    Schmidt, W. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    4
  • High-resolution spectroscopy of the Seyfert galaxy MRK 595 in the direction of the Cohen HI high-velocity stream
    We have obtained a spectrum of the Na D lines of the Seyfert galaxy Mrk 595 with a signal-to-noise ratio (S/N) of about 30. The importance of this sightline is that this galaxy lies in a direction close to the highest column densities of the Cohen high-velocity (HV) stream, and hence represents the best opportunity of detecting this stream in
    Kemp, S. N. et al.

    Fecha de publicación:

    12
    1998
    Número de citas
    1
  • High-Resolution Spectroscopy of the Transiting Planet Host Star TrES-1
    We report on a spectroscopic determination of the stellar parameters and chemical abundances for the parent star of the transiting planet TrES-1. Based on a detailed analysis of iron lines in our Keck and Hobby-Eberly Telescope spectra, we derive Teff=5250+/-75 K, logg=4.6+/-0.2, and [Fe/H]=0.00+/-0.09. By measuring the Ca II activity indicator and
    Sozzetti, Alessandro et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    61
  • High-Speed Ultraviolet Monitoring in NGC 4151
    The rapidly variable Seyfert 1 galaxy NGC 4151 will be the subject of an intensive monitoring campaign with IUE, Rosat, GRO, ASCA and ground-based telescopes in December 1993. We will report preliminary results of 9.3 days of continuous monitoring with IUE, at a sampling rate of once every ~ 80 min, an order of magnitude faster than that achieved
    Edelson, R. et al.

    Fecha de publicación:

    12
    1993
    Número de citas
    0