Tipo de publicación: Sin árbitro

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    A novel background reduction strategy for high level triggers and processing in gamma-ray Cherenkov detectors
    Gamma ray astronomy is now at the leading edge for studies related both to fundamental physics and astrophysics. The sensitivity of gamma detectors is limited...
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    A novel biosensor for mercuric ions based on motor proteins
    We explored the potential for use of the contractile proteins, actin and myosin, as biosensors of solutions containing mercury ions. We demonstrate that the...
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    A Novel Precise Method for Correcting the Temperature in Stellar Atmosphere Models
    A mayor problem that arises in the computation of stellar atmosphere models is the self consistent determination of the temperature distribution via the...
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    A novel technique to characterize the merging channel of the galaxies
    Most massive galaxies have grown their sizes during cosmic time. Several mechanisms have been proposed to explain this growth, being minor mergers the most...
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    A numerical laboratory for the diagnostics of stellar properties
    In a recent paper (Crivellari et al., 2003) we summarized the principles of the algorithmic representation of the structure of a stellar atmosphere. We...
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    A Numerical Study - of the Asymptotic Solutions to the Family C of the Periodic Orbits in the Restricted Problem of Three Bodies
    Not Available
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    A One Gyr Old Stellar Burst in NGC 6822?
    Not Available
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    A OSIRIS/GTC emission-line survey of the rich cluster Cl0024+2654 at z = 0.4
    In the framework of the GLACE project, we present the preliminary results of a mapping of emission lines (Hα+[NII], Hβ and [OIII]) in the rich cluster Cl0024...
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    A Parametric Model of the Solar Full-Disk Seismological Signal
    Solar eigenmodes frequencies are most often determined using some kind of modelisation of the Fourier spectrum of the data in one or two dimensions. Many...