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Wlodzimierz Klamra

Researcher at Royal Institute of Technology

Publications -  154
Citations -  6947

Wlodzimierz Klamra is an academic researcher from Royal Institute of Technology. The author has contributed to research in topics: Scintillator & Neutron. The author has an hindex of 31, co-authored 154 publications receiving 6410 citations. Previous affiliations of Wlodzimierz Klamra include Stockholm University & McMaster University.

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The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

W. B. Atwood, +292 more
TL;DR: The Large Area Telescope (Fermi/LAT) as mentioned in this paper is the primary instrument on the Fermi Gamma-ray Space Telescope, which is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from below 20 MeV to more than 300 GeV.
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Properties of the YAG:Ce scintillator

TL;DR: In this paper, the light yield, light pulse shape due to γ-rays and α-particles, energy resolution and time resolution of the new YAG:Ce scintillator were studied using a light readout by means of the XP2020Q photomultiplier and the S3590-03 photodiode.
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The on-orbit calibration of the Fermi Large Area Telescope

A. A. Abdo, +310 more
TL;DR: In this paper, the authors describe on-orbit calibration results obtained using known astrophysical sources, galactic cosmic rays, and charge injection into the front-end electronics of each detector, which have been used to calibrate the LAT datasets to be publicly released in August 2009.
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Fermi large area telescope observations of the vela pulsar

A. A. Abdo, +280 more
TL;DR: In this paper, the Vela pulsar was used to verify Fermi timing and angular resolution, and the high energy behavior of the pulsed emission was examined; initial spectra suggest a phase-averaged power law index of Gamma=1.51{+0.05/-0.04} with an exponential cut-off at E_c=2.1 GeV.
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Properties of the YAP : Ce scintillator

TL;DR: In this article, a 10 × 10 × 5 mm 3 YAB crystal coupled to the XP2020Q photomultiplier was studied, which exhibited an energy resolution of 5.7% for 662 keV γ-rays fron a 137 Cs source.