Characterization of a VPE gallium arsenide x-gamma-ray detector

1998 ◽  
Author(s):  
Giuseppe Bertuccio ◽  
D. Maiocchi ◽  
C. Rente ◽  
Arno Foerster ◽  
Hans Luth
Keyword(s):  
Gallium Arsenide ◽  
Gamma Ray ◽  
Gamma Ray Detector

Imaging characterization of a new gamma ray detector based on CRY019 scintillation crystal for PET and SPECT applications

2017 ◽  
Vol 12 (02) ◽  
pp. C02034-C02034 ◽  
Author(s):  
C. Polito ◽  
R. Pani ◽  
C. Trigila ◽  
M.N. Cinti ◽  
A. Fabbri ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Scintillation Crystal ◽  
Gamma Ray Detector ◽  
Imaging Characterization

Growth and characterization of SrI2:Eu2+ single crystal for gamma ray detector applications

2018 ◽  
Author(s):  
A. Raja ◽  
D. Joseph Daniel ◽  
P. Ramasamy ◽  
S. G. Singh ◽  
S. Sen ◽  
...  
Keyword(s):  
Single Crystal ◽  
Gamma Ray ◽  
Gamma Ray Detector

scholarly journals Full-volume characterization of an AGATA segmented HPGe gamma-ray detector using a $$^{152}Eu$$ source

2021 ◽  
Vol 57 (7) ◽  
Author(s):  
B. De Canditiis ◽  
G. Duchêne ◽  
M. H. Sigward ◽  
M. Filliger ◽  
F. Didierjean ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Detector ◽  
Full Volume

scholarly journals The STACEE ground-based gamma-ray detector

2005 ◽  
Author(s):  
D.M. Gingrich ◽  
L.M. Boone ◽  
D. Bramel ◽  
J. Carson ◽  
C.E. Covault ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Detector

scholarly journals Introducing the HD+B model for pulsar wind nebulae: a hybrid hydrodynamics/radiative approach

2020 ◽  
Vol 494 (3) ◽  
pp. 4357-4370
Author(s):  
B Olmi ◽  
D F Torres
Keyword(s):  
Gamma Ray ◽  
High Energy ◽  
Theoretical Modelling ◽  
X Rays ◽  
Pulsar Wind Nebulae ◽  
New Approach ◽  
Energy Gamma ◽  
Radiative Model ◽  
Pulsar Wind

ABSTRACT Identification and characterization of a rapidly increasing number of pulsar wind nebulae is, and will continue to be, a challenge of high-energy gamma-ray astrophysics. Given that such systems constitute -by far- the most numerous expected population in the TeV regime, such characterization is important not only to learn about the sources per se from an individual and population perspective, but also to be able to connect them with observations at other frequencies, especially in radio and X-rays. Also, we need to remove the emission from nebulae in highly confused regions of the sky for revealing other underlying emitters. In this paper, we present a new approach for theoretical modelling of pulsar wind nebulae: a hybrid hydrodynamic-radiative model able to reproduce morphological features and spectra of the sources, with relatively limited numerical cost.

Characterization of Uranium Ore Samples by HPGe Gamma-Ray Spectroscopy

2020 ◽  
Vol 67 (4) ◽  
pp. 654-661 ◽  
Author(s):  
Thomas Marchais ◽  
Bertrand Perot ◽  
Cedric Carasco ◽  
Jean-Luc Ma ◽  
Pierre-Guy Allinei ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Uranium Ore ◽  
Gamma Ray Spectroscopy
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