Ultra-high-energy gamma rays: Current status

1993 ◽  
Author(s):  
Gaurang B. Yodh
1998 ◽  
Vol 188 ◽  
pp. 125-128
Author(s):  
T. Kifune

The current status of very high energy gamma ray astronomy (in ~ 1 TeV region) is described by using as example results of CANGAROO (Collaboration of Australia and Nippon for a GAmma Ray Observatory in the Outback). Gamma rays at TeV energies, emitted through inverse Compton effect of electrons or π0 decay from proton interaction, provide direct evidence on “hot” non-thermal processes of the Universe, as well as environmental features, such as the strength of magnetic field in the emission region, for the non-thermal processes.


1996 ◽  
Vol 48 (1-3) ◽  
pp. 483-484
Author(s):  
A. Borione ◽  
C.E. Covault ◽  
J.W. Cronin ◽  
B.E. Fick ◽  
L.F. Fortson ◽  
...  

1996 ◽  
Vol 472 (2) ◽  
pp. 800-805 ◽  
Author(s):  
H. Yoshii ◽  
T. Baba ◽  
T. Kaneko ◽  
K. Suga ◽  
F. Kakimoto ◽  
...  

1988 ◽  
Vol 326 ◽  
pp. L9 ◽  
Author(s):  
D. Ciampa ◽  
D. J. Bird ◽  
R. W. Clay ◽  
P. G. Edwards ◽  
R. J. Protheroe

1987 ◽  
Vol 7 (1) ◽  
pp. 73-74 ◽  
Author(s):  
D. J. Bird ◽  
T. E. G. Bruce ◽  
D. Ciampa ◽  
R. W. Clay ◽  
C. L. Corani ◽  
...  

AbstractA search has been made using the Buckland Park air shower array for evidence of any excess of events from the direction of the recent supernova in the Large Magellanic Cloud. Upper limits resulting from this search and their significance are discussed in this paper.


2021 ◽  
Vol 911 (2) ◽  
pp. L27
Author(s):  
A. Albert ◽  
R. Alfaro ◽  
C. Alvarez ◽  
J. D. Álvarez ◽  
J. R. Angeles Camacho ◽  
...  

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