scholarly journals Significance of medium-energy gamma-ray astronomy in the study of cosmic rays

1976 ◽  
Vol 208 ◽  
pp. 211 ◽  
Author(s):  
C. E. Fichtel ◽  
D. A. Kniffen ◽  
D. J. Thompson ◽  
G. F. Bignami ◽  
C. Y. Cheung
2003 ◽  
Vol 214 ◽  
pp. 382-386
Author(s):  
Masato Takita

Sub-TeV and TeV energy gamma-ray astronomy reveals non-thermal gamma-ray pictures of our universe and serve as a probe to understand the origin, acceleration and propagation of cosmic rays. Recent status of ground-based high-energy gamma-ray astronomy is reviewed.


2012 ◽  
Author(s):  
Stanley D. Hunter ◽  
Peter F. Bloser ◽  
Michael P. Dion ◽  
Georgia A. DeNolfo ◽  
Jason Legere ◽  
...  

2019 ◽  
Author(s):  
Elena Orlando ◽  
"Isabelle Grenier" ◽  
"Vincent Tatischeff" ◽  
"Andrey Bykov" ◽  
"Andrew Strong" ◽  
...  

2006 ◽  
Vol 6 (S1) ◽  
pp. 388-392 ◽  
Author(s):  
P. F Bloser ◽  
J. M Ryan ◽  
M. L McConnell ◽  
J. R Macri ◽  
U Bravar ◽  
...  

2003 ◽  
Author(s):  
Gottfried Kanbach ◽  
Robert Andritschke ◽  
Peter F. Bloser ◽  
Florian Schopper ◽  
Volker Schoenfelder ◽  
...  

2018 ◽  
Vol 191 ◽  
pp. 01007 ◽  
Author(s):  
N. Budnev ◽  
I. Astapov ◽  
P. Bezyazeekov ◽  
V. Boreyko ◽  
A. Borodin ◽  
...  

The physics motivations and advantages of the new TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) detector are presented. TAIGA aims at gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV. For the energy range 30 – 200 TeV the sensitivity of 10 km2 area TAIGA array for the detection of local sources is expected to be 5 × 10-14 erg cm-2 sec-1 for 300 h of observations. Reconstruction of the given EAS energy, incoming direction and its core position, based on the timing TAIGA-HiSCORE data, allows one to increase a distance between the IACTs up to 600-1000 m. The low investments together with the high sensitivity for energies ≥ 30-50 TeV make this pioneering technique very attractive for exploring the galactic PeVatrons and cosmic rays. At present the TAIGA first stage has been constructed in Tunka valley, 50 km West from the Lake Baikal. The first experimental results of the TAIGA first stage are presented.


2010 ◽  
Author(s):  
Peter F. Bloser ◽  
James M. Ryan ◽  
Jason S. Legere ◽  
Manuel Julien ◽  
Christopher M. Bancroft ◽  
...  

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