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Low-dose, high-resolution CT of infant-sized lungs via propagation-based phase contrast. [PDF]
Sci RepPollock JA +9 more
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High energy neutrino astronomy
Nature, 1978The possibility of doing point source neutrino astronomy is discussed. Probable sources include galactic nuclei, Seyferts, quasars, radio galaxies, pulsars and supernovae.
David N. Schramm, David Eichler
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The high energy astronomy observatories
13th Annual Meeting and Technical Display Incorporating the Forum on the Future of Air Transportation, 1977The forthcoming NASA project of orbiting High Energy Astronomy Observatories (HEAO's) designed to probe the universe by tracing celestial radiations and particles is outlined. Solutions to engineering problems concerning HEAO's which are integrated, yet built to function independently are discussed, including the onboard digital processor, mirror ...
R. F. Doolittle +2 more
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Very high energy gamma ray astronomy [PDF]
AIP Conference Proceedings, 1988 Abstract Current interest in gamma-astronomy at energies above 100 GeV comes from the identification of Cygnus X-3 and other X-ray binaries as sources. In addition there are reports of emission from radio pulsars and a variety of other objects. The statistical significance of many of the observations is not high and many reported effects await ...
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Gamma-ray astronomy at high energies
Reviews of Modern Physics, 1999Progress in high-energy gamma-ray astronomy has depended upon the development of sophisticated detectors and analysis techniques. Observations in this decade using space-based and ground-based detectors have observed gamma-ray emission from a variety of sources. For the first time a consistent picture of the {gamma}-ray sky has emerged.
Hoffman, C-M. +3 more
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High energy neutrino astronomy
Nuclear Physics B - Proceedings Supplements, 2000Abstract The sky survey with high energy neutrinos is complementary to the survey with photons. The method of the detection of ν μ is described and the expected sensitivity to high energy neutrino sources with a kilometer-scale detector is estimated. The status of the current under-water(ice) detector projects is reported.
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High-energy Gamma-ray Astronomy
Nature, 1970Gamma-ray astronomy above 10 MeV is difficult from the experimental point of view, but promising data are beginning to appear, as this survey progress report shows.
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1989
Techniques of Ultra High Energy astronomy are reviewed in this lecture. Sensitivity of experiments currently underway or planned for the near future is discussed. Recent results from the CYGNUS experiment with regard to steady emission from sources such as Cygnus X-3 and Herculus X-l are compared with those from other experiments.
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Techniques of Ultra High Energy astronomy are reviewed in this lecture. Sensitivity of experiments currently underway or planned for the near future is discussed. Recent results from the CYGNUS experiment with regard to steady emission from sources such as Cygnus X-3 and Herculus X-l are compared with those from other experiments.
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High Energy Astronomy Observatory Program
IFAC Proceedings Volumes, 1978Abstract This paper describes the series of three orbiting high energy astronomy observatories that comprise the High Energy Astronomy Observatory (HEAO) program of the National Aeronautics and Space Administration (NASA). The basis and enthusiasm of the scientific community for this program is presented.
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