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Gamma-Ray Bursts as seen by the Fermi Gamma-Ray Space Telescope

AIP Conference Proceedings, 2009
The Large Area Telescope (LAT) instrument on the Fermi mission is revealing the rich spectral and temporal gamma‐ray burst phenomena in the >100 MeV band. The synergy with Fermi’s GBM detectors links these observations to those in the well‐explored 10–1000 keV range; the addition of the >100 MeV band observations brings new hint and new information ...
Nicola Omodei   +2 more
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The Fermi Gamma-Ray Space Telescope: Overview and early science results

2009 IEEE Aerospace conference, 2009
The Fermi Gamma-ray Space Telescope (formerly named GLAST) was designed and built by NASA, the United States Department of Energy, and agencies in France, Germany, Italy, Japan and Sweden. It launched in June of 2008 and has been observing the gamma-ray sky for over 6 months.
Jack Leibee   +2 more
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Fermi Gamma-ray Space Telescope: Highlights of the GeV Sky

Nuclear Physics B - Proceedings Supplements, 2011
Because high-energy gamma rays can be produced by processes that also produce neutrinos. the gamma-ray survey of the sky by the Fermi Gamma-ray Space Telescope offers a view of potenl ial targds for neutrino observations. Gamma-ray bursts. active galactic nuclei, and supernova remnants are all sites where hadronic, neutrino-producing interactions are ...
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First light from the Vela pulsar with the Fermi Gamma-ray Space Telescope

AIP Conference Proceedings, 2009
The Fermi Gamma‐ray Space Telescope, launched in June 2008, is an international space mission entirely devoted to the study of the high‐energy gamma rays from the Universe. The main instrument aboard Fermi is the Large Area Telescope (LAT), a pair conversion telescope equipped with the state‐of‐the art in gamma‐ray detectors technology.
M. Razzano   +2 more
openaire   +1 more source

Viewing the High-Energy Universe with the Fermi Gamma-ray Space Telescope

Frontiers in Optics 2010/Laser Science XXVI, 2010
The Fermi Gamma-ray Space Telescope has completed 2 years of observations of the entire sky from 10 keV to more than 300 GeV, providing a new view of the high-energy Universe.
openaire   +1 more source

Status of the technology of the current space missions including the Fermi gamma-ray space telescope

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2010
Abstract We review the status of X-rays and γ -rays space missions operational in 2009. We provide highlights of the current semiconductor technology instrumentation and briefly discuss challenges to be addressed by future missions.
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Some highlights of the first four years of the Fermi Gamma-ray Space Telescope

Frontiers of Physics, 2013
The Fermi Gamma-ray Space Telescope, formerly called GLAST, measures the cosmic gamma-ray flux in the energy range 8 keV to > 300 GeV. In addition to breakthrough capabilities in energy coverage and localization, the very large field of view enables observations of 20% of the sky at any instant, and the entire sky on a timescale of a few hours.
openaire   +1 more source

Responsive materials architected in space and time

Nature Reviews Materials, 2022
Xiaoxing Xia   +2 more
exaly  

The biofilm matrix: multitasking in a shared space

Nature Reviews Microbiology, 2022
Hans-Curt Flemming   +2 more
exaly  

Multifunctional biomolecule nanostructures for cancer therapy

Nature Reviews Materials, 2021
Jing Wang, Yiye Li, Guangjun Nie
exaly  

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