11,649 research outputs found

    Computer analysis of EEG data for a normative library Final report, Sep. 24, 1963 - Jan. 31, 1966

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    Computer analysis of electroencephalographic data for development of normative criteri

    Comprehensive Spectral Analysis of Human EEG GENERATORS in Posterior Cerebral Regions

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    Human electroencephalogram generator spectral analysis in posterior cerebral region

    Results of electroencephalographic examina- tions under the influence of vibration and centrifuging in the monkey

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    Electroencephalographic examinations of monkeys under influence of vibrations and centrifugin

    Analysis of baseline and Gemini flight GT-7 EEG data with specification of on-line computing requirements

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    Analysis of baseline and Gemini GT-7 ELECTROENCEPHALOGRAM data with specification of on-line computing requirement

    Effect of low-level, low-frequency electric fields on EEG and behavior in Macaca nemestrina

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    Effect of low level, low frequency electric fields on EEG and behavior of Macaca nemestrin

    Electroencephalographic baselines in astronaut candidates estimated by computation and pattern recognition techniques

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    Electroencephalographic baselines in astronaut candidates estimated by computer and pattern recognition technique

    The hard quiescent spectrum of the neutron-star X-ray transient EXO 1745-248 in the globular cluster Terzan 5

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    We present a Chandra observation of the globular cluster Terzan 5 during times when the neutron-star X-ray transient EXO 1745-248 located in this cluster was in its quiescent state. We detected the quiescent system with a (0.5-10 keV) luminosity of ~2 x 10^{33} ergs/s. This is similar to several other neutron-star transients observed in their quiescent states. However, the quiescent X-ray spectrum of EXO 1745--48 was dominated by a hard power-law component instead of the soft component that usually dominates the quiescent emission of other neutron-star X-ray transients. This soft component could not conclusively be detected in EXO 1745-248 and we conclude that it contributed at most 10% of the quiescent flux in the energy range 0.5-10 keV. EXO 1745-248 is only the second neutron-star transient whose quiescent spectrum is dominated by the hard component (SAX J1808.4-3658 is the other one). We discuss possible explanations for this unusual behavior of EXO 1745-248, its relationship to other quiescent neutron-star systems, and the impact of our results on understanding quiescent X-ray binaries. We also discuss the implications of our results on the way the low-luminosity X-ray sources in globular clusters are classified.Comment: Accepted by ApJ Main Journal, September 22, 2004. Figure 2 is a color figur

    Analysis of Brain Wave Records from Gemini Flight GT-7 by Computations to Be Used in a Thirty Day Primate Flight

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    Data analysis and display techniques for biosatellite flight and application of astronaut electroencephalogram analysi
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