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THE LARGE AREA TELESCOPE ON THEFERMI GAMMA-RAY SPACE TELESCOPEMISSION [PDF]

open access: bronzeThe Astrophysical Journal, 2009
The Large Area Telescope (Fermi/LAT, hereafter LAT), the primary instrument on the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view (FoV), high-energy γ-ray telescope, covering the energy range from below 20 MeV to more ...
W. B. Atwood   +99 more
semanticscholar   +15 more sources

Pulsar timing for theFermigamma-ray space telescope [PDF]

open access: bronzeAstronomy & Astrophysics, 2008
We describe a comprehensive pulsar monitoring campaign for the Large Area Telescope (LAT) on the {\em Fermi Gamma-ray Space Telescope} (formerly GLAST). The detection and study of pulsars in gamma rays give insights into the populations of neutron stars ...
D. A. Smith   +27 more
semanticscholar   +7 more sources

The Fermi Gamma-Ray Space Telescope Discovers the Pulsar in the Young Galactic Supernova Remnant CTA 1 [PDF]

open access: greenScience, 2008
Energetic young pulsars and expanding blast waves [supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma-Ray Space Telescope has unveiled a radio quiet pulsar
A. A. Abdo   +99 more
semanticscholar   +12 more sources

Poisson denoising on the sphere: application to theFermigamma ray space telescope [PDF]

open access: bronzeAstronomy and Astrophysics, 2010
The Large Area Telescope (LAT), the main instrument of the Fermi gamma-ray Space telescope, detects high energy gamma rays with energies from 20 MeV to more than 300 GeV.
Jérémy Schmitt   +4 more
semanticscholar   +9 more sources

Fermi Gamma-ray Space Telescope: high-energy results from the first year [PDF]

open access: greenReports on Progress in Physics, 2010
The Fermi Gamma-ray Space Telescope (Fermi) was launched on 11 June 2008 and began its first year sky survey on 11 August 2008. The Large Area Telescope (LAT), a wide field-of-view pair-conversion telescope covering the energy range from 20 MeV to more ...
P. F. Michelson, W. B. Atwood, S. Ritz
semanticscholar   +6 more sources

Gamma rays, electrons and positrons up to 3 TeV with the Fermi Gamma-ray Space Telescope [PDF]

open access: goldJournal of Physics: Conference Series, 2012
The Fermi Gamma-ray Space Telescope (formerly known as Gamma-ray Large Area Space Telescope, GLAST) was successfully launched on June 11 2008. Its main instrument is the Large Area Telescope (LAT), which detects gamma rays from 20 MeV to more than 300 ...
P. Bruel
semanticscholar   +8 more sources

FERMI GAMMA-RAY SPACE TELESCOPEOBSERVATIONS OF GAMMA-RAY OUTBURSTS FROM 3C 454.3 IN 2009 DECEMBER AND 2010 APRIL [PDF]

open access: bronzeThe Astrophysical Journal, 2010
The flat spectrum radio quasar 3C 454.3 underwent an extraordinary outburst in 2009 December when it became the brightest γ-ray source in the sky for over 1 week.
M. Ackermann   +99 more
semanticscholar   +12 more sources

Jet Physics of Accreting Super-Massive Black Holes in the Era of the Fermi Gamma-ray Space Telescope [PDF]

open access: yesFrontiers in Astronomy and Space Sciences, 2017
The Fermi Gamma-ray Space Telescope with its main instrument on-board, the Large Area Telescope (LAT), opened a new era in the study of high-energy emission from Active Galactic Nuclei (AGN).
Filippo D'Ammando, Filippo D'Ammando
doaj   +8 more sources

Interpretation and implications of the non-detection of GeV spectrum excess by theFermi Gamma-ray Space Telescopein most gamma-ray bursts [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2009
Since the launch of the Fermi Gamma-ray Space Telescope on 2008 June 11, significant detections of high-energy emission have been reported only in six gamma-ray bursts (GRBs) until now.
Yi-Zhong Fan
semanticscholar   +8 more sources

DISCOVERY OF PULSATIONS FROM THE PULSAR J0205+6449 IN SNR 3C 58 WITH THE FERMI GAMMA-RAY SPACE TELESCOPE [PDF]

open access: bronzeAstrophysical Journal, 2009
We report the discovery of γ-ray pulsations (≥ 0.1 GeV) from the young radio and X-ray pulsar PSR J0205+6449 located in the Galactic supernova remnant 3C 58.
A. A. Abdo   +99 more
semanticscholar   +4 more sources

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