Tipo de publicación: Sin árbitro

  • Publicación
    Constructing the Largest Galaxy Morphological Catalogue with Supervised Deep Learning ... with No Training Sample!
    Galaxies exhibit a wide variety of morphologies which contain valuable information about their star formation histories. Having large samples of morphologically...
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    Construction progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope
    We present an update on the overall construction progress of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), now that...
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    Contact binary stars as standard candles
    Rucinski (1996) suggested to use contact binary stars as standard candles. We investigated the properties of contact binary stars in order to search for...
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    Continuing X-ray Emission of Nova Vul 2007
    We report a new observation of Nova Vul 2007 (S. Nakano, IAUC 8861) obtained by the Swift X-ray Telescope (XRT) on 2008 June 18. The nova was detected at count...
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    Continuous observation of solar oscillations from two suitably spaced ground stations
    By operating two observing stations, one at Izana on Tenerife and the other at Haleakala on Maui, up to 22 hours of continuous solar surface velocity data per...
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    Continuous Upflow of Material in an Active Region Filament from the Photosphere to the Corona
    Using spectropolarimetric data of an Active Region (AR) filament we have carried out inversions in order to infer vector magnetic fields in the photosphere (Si...
  • Publicación
    Continuous upflow of material in an active region filament from thephotosphere to the corona
    Using spectropolarimetric data of an Active Region (AR) filament we have carried out inversions in order to infer vector magnetic fields in the photosphere (Si...
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    Continuum and emission line variability induced by microlensing
    Not Available
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    Continuum intensity and magnetic flux of solar fluxtubes
    The continuum contrast between flux tubes and their quiet background, and the magnetic flux carried by these magnetic elements, have been determined at...