Publication type: Non-refereed

  • Publication
    The JWST Transiting Exoplanet Community Early Release Science Program
    With a 6.5-meter diameter primary mirror in space and a wavelength coverage from the visible to the mid-infrared, the James Webb Space Telescope (JWST) will...
  • Publication
    The K 769.9 NM line profile
    The observation of a solar absorption line by means of resonant scattering over several months in the study of solar oscillations, yields data which may be...
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    The K-correction For LMXBs. Application To X1822-371 and GX339-4
    We present the K-correction for emission lines formed on the irradiated face of the companion stars in X-ray binaries. We compute this K-correction in a general...
  • Publication
    The K-correction for LMXBs: an application to X1822-371 and GX339-4
    We present the K-correction for emission lines formed on the irradiated face of the companion stars in X-ray binaries. We compute this K-correction in a general...
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    The Keck/NIRSPEC Search for Giant Exoplanets around Late M-dwarfs
    We present the rationale, first observations and preliminary results of our radial velocity search for exoplanets around M dwarfs. So far we have obtained 2.5...
  • Publication
    The Kepler space mission sheds a new light on variable A- and F-type stars
    Not Available
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    The Kinematic Signature of the Sagittarius Dwarf Galaxy Tidal Debris from SDSS-DR1
    Recent results from the Sloan Digital Sky Survey (SDSS) and the 2MASS All-Sky Survey have clearly revealed the extent of the spatial distribution of stars...
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    The kinematical behavior of Galactic PNe with [WC] central star
    High resolution spectroscopic data of a large sample of galactic planetary nebulae with [WC] central stars ([WC]PNe) are analyzed to determine their kinematical...
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    The kinematical behavior of ORLs and CELs in PNe with [WC] central star
    In Planetary Nebulae (PNe) and HII regions ionic abundances can be derived by using collisionally excited lines (CELs) or recombination lines (ORLs). Such...