Tipo de publicación: Sin árbitro

  • Publicación
    Potential of Photometric Searches for Transiting Planets
    Many ground-based photometric surveys are now under way, and five of them have been successful at detecting transiting exoplanets. Nevertheless, detecting...
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    Power spectra comparison between GOLF and MDI velocity observations
    We present a comparison of the velocity power spectra between the GOLF and MDI instruments. In addition, this poster outlines work towards creating a GOLF...
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    Power spectra comparison between GOLF and MDI velocity observations.
    Not Available
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    pPNe: Lobe-Shaping Models & HST Images
    HST images of some 50 pre planetary nebulae ("pPNe") are now available. A confrontation of images with theoretical shaping models is timely in order to...
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    Precipitable water vapour at the Roque de los Muchachos Observatory from GPS measurements
    Not Available
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    Precipitable water vapour content above the Roque de los Muchachos Observatory from GPS estimations
    The requirements for current large and future extremely large telescopes as well as the quick development of IR instrumentation demand a proper characterization...
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    Precise abundances of Mg and neutron-capture elements in the Milky Way: chemodynamical relations using Gaia data and chemical evolution models
    The abundance of alpha and neutron-capture elements provide an important fossil signature in Galactic archaeology for tracing the chemical evolution of the...
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    Precise seismology with TESS CVZ data
    The release of TESS light-curves gives us the opportunity to perform all-sky seismology for a lot of stars. Among them, the higher quality data that was...
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    Precise surface gravitites of A-type stars from Asteroseismology
    δ Sct are one of the most abundant pulsating stars in our Galaxy. In addition, they have moderate to fast rotations and periods of several hours. That makes...