Tipo de publicación: Sin árbitro

  • Publicación
    FRIDA: the software architecture to execute and coordinate observing sequences
    The instrument FRIDA (inFRared Imager and Dissector for Adaptive optics) is an integral field spectrograph (near infrared) with imaging capability for being...
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    FRIDÁs mechanisms control system structure and tests
    FRIDA will be a near infrared imager and integral field spectrograph covering the wavelength range from 0.9 to 2.5 microns. FRIDA will work in two observing...
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    Fried's parameter derived from observations of granulation outside the disk centre
    A new method has recently been developed to obtain the Fried's parameter from observations of granulation outside the disk center, based on the different...
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    From atmospheres to exospheres in exoplanets
    Interaction phenomena between atmospheric layers in planetary atmospheres give rise to highly complex exchanges influencing thermal structure, composition and...
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    From Brightness and Colour to Size and Temperature (CD-ROM Directory: contribs/lambert2)
    Not Available
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    From CM Draconis to the Crowded Field BW3: Aspects of the Search
    Having completed a 1000 hour search for terrestrial planets (down to 2.5-Earth-Radii, i.e., planets 1% the size of Jupiter) in the circumstellar habitable zone...
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    From Cores to Stars, Brown Dwarfs and Planets
    Not Available
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    From cosmic spyglass to precision measuring engine: the early decades of the telescope
    Not Available
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    From Deterministic to Probabilistic Population Synthesis (Why Synthesis Models are not what we thought they were, and how they can be much more than that)
    For a number of reasons, the properties of integrated stellar populations are distributed. Traditional synthesis models usually return the mean value of such...