Publication type: Non-refereed

  • Publication
    Detection of periodic signatures in the solar power spectrum On the track of l=1 gravity modes
    In the present work we show robust indications of the existence of g modes in the Sun using 10 years of GOLF data. The present analysis is based on the...
  • Publication
    Detection of polarization from the E4Π-A4Π system of FeH in sunspot spectra
    We report the first detection of polarization signals induced by the Zeeman Effect in lines of the E4Π-A4Π system of FeH located at 1.6 μm. Motivated by the...
  • Publication
    Detection of pulsations and identification of SAX J1748.9-2021 as the X-ray transient in NGC 6440.
    On the 28th of December, MAXI/GSC detected an X-ray outburst from the globular cluster NGC6440 (Atel #2360), which has continued to the present.
  • Publication
    Detection of second-generation asymptotic giant branch stars in metal-poor globular clusters
    Multiple stellar populations are actually known to be present in Galactic globular clusters (GCs). The first generation (FG) displays a halo-like chemical...
  • Publication
    Detection of Strong 3.4 μm and 2.8 μm Emission Features in Comet p/Brorsen-Metcalf
    Not Available
  • Publication
    Detection of terrestrial planets and moons with the photometric transit method
    An overview is given over the photometric transit method for the detection of extraterrestrial planets. Discussed are: its basic principals, its derivable...
  • Publication
    Detection of the 2175Å extinction feature in a lens galaxy at z = 0.83
    We determine the extinction curve in the zl = 0.83 lens galaxy of the gravitational lens SBS 0909+532 from the wavelength dependence of the flux ratio between...
  • Publication
    Detection of the Effect of Cosmological Large--Scale Structure on the Orientation of Galaxies
    Galaxies are not distributed randomly throughout space but are instead arranged in an intricate "cosmic web" of filaments and walls surrounding bubble-like...
  • Publication
    Detection of the Periodic Signatures of l=1 Solar g Modes with 10 Years of GOLF/SOHO Data
    Not Available