SEARCH FOR GAMMA RAYS ABOVE 100 TeV FROM THE CRAB NEBULA WITH THE TIBET AIR SHOWER ARRAY AND THE 100 m2MUON DETECTOR

2015 ◽  
Vol 813 (2) ◽  
pp. 98 ◽  
Author(s):  
M. Amenomori ◽  
X. J. Bi ◽  
D. Chen ◽  
T. L. Chen ◽  
W. Y. Chen ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Crab Nebula ◽  
Air Shower ◽  
The Crab Nebula ◽  
Shower Array ◽  
Air Shower Array

Search for steady emission of 10-TeV gamma rays from the Crab Nebula, Cygnus X-3, and Hercules X-1 using the Tibet air shower array

1992 ◽  
Vol 69 (17) ◽  
pp. 2468-2471 ◽  
Author(s):  
M. Amenomori ◽  
Z. Cao ◽  
L. K. Ding ◽  
Z. Y. Feng ◽  
K. Hibino ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Crab Nebula ◽  
Air Shower ◽  
Tev Gamma Rays ◽  
The Crab Nebula ◽  
Shower Array ◽  
Air Shower Array

Observation of Multi-T[CLC]e[/CLC]V Gamma Rays from the Crab Nebula using the Tibet Air Shower Array

1999 ◽  
Vol 525 (2) ◽  
pp. L93-L96 ◽  
Author(s):  
M. Amenomori ◽  
S. Ayabe ◽  
P. Y. Cao ◽  
Danzengluobu ◽  
L. K. Ding ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Crab Nebula ◽  
Air Shower ◽  
The Crab Nebula ◽  
Shower Array ◽  
Air Shower Array

scholarly journals MULTI-TeV GAMMA-RAY OBSERVATION FROM THE CRAB NEBULA USING THE TIBET-III AIR SHOWER ARRAY FINELY TUNED BY THE COSMIC RAY MOON'S SHADOW

2009 ◽  
Vol 692 (1) ◽  
pp. 61-72 ◽  
Author(s):  
M. Amenomori ◽  
X. J. Bi ◽  
D. Chen ◽  
S. W. Cui ◽  
Danzengluobu ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Crab Nebula ◽  
Cosmic Ray ◽  
Air Shower ◽  
The Crab Nebula ◽  
Shower Array ◽  
Air Shower Array

Predominantly electromagnetic air showers of energy 1014 eV to 1016 eV

1968 ◽  
Vol 46 (10) ◽  
pp. S72-S74 ◽  
Author(s):  
K. Kamata ◽  
S. Shibata ◽  
O. Saavedra ◽  
V. Domingo ◽  
K. Suga ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Cosmic Radiation ◽  
Progress Report ◽  
Point Sources ◽  
Air Showers ◽  
Air Shower ◽  
Upper Limits ◽  
Primary Cosmic Radiation ◽  
Shower Array ◽  
Air Shower Array

The Chacaltaya air shower array has continued to be used for the accumulation of muon-poor air showers in an attempt to find evidence of gamma rays in the primary cosmic radiation. A progress report is given here, and some upper limits to the intensities are presented for possible point sources and for galactic and isotropic backgrounds.

scholarly journals Search for diffuse cosmic gamma rays of energy Eγ> 100 TeV with the Carpet-3 air shower array

2017 ◽  
Vol 798 ◽  
pp. 012028 ◽  
Author(s):  
D D Dzhappuev ◽  
V B Petkov ◽  
A S Lidvansky ◽  
V I Volchenko ◽  
G V Volchenko ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Air Shower ◽  
Shower Array ◽  
Air Shower Array

scholarly journals Limits on the TeV flux of diffuse gamma rays as measured with the HEGRA air shower array

2002 ◽  
Vol 17 (4) ◽  
pp. 459-475 ◽  
Author(s):  
F.A. Aharonian ◽  
A.G. Akhperjanian ◽  
J.A. Barrio ◽  
K. Bernlöhr ◽  
H. Bojahr ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Air Shower ◽  
Shower Array ◽  
Air Shower Array

scholarly journals Observation of Multi‐TeV Diffuse Gamma Rays from the Galactic Plane with the Tibet Air Shower Array

2002 ◽  
Vol 580 (2) ◽  
pp. 887-895 ◽  
Author(s):  
M. Amenomori ◽  
S. Ayabe ◽  
S. H. Cui ◽  
L. K. Ding ◽  
X. H. Ding ◽  
...  
Keyword(s):  
Gamma Rays ◽  
Galactic Plane ◽  
Air Shower ◽  
Shower Array ◽  
Air Shower Array

scholarly journals Search for astrophysical PeV gamma rays from point sources with Carpet-2

2019 ◽  
Vol 207 ◽  
pp. 03004 ◽  
Author(s):  
D. D. Dzhappuev ◽  
I. M. Dzaparova ◽  
E. A. Gorbacheva ◽  
I. S. Karpikov ◽  
M. M. Khadzhiev ◽  
...  
Keyword(s):  
Gamma Rays ◽  
High Energy ◽  
Point Sources ◽  
Muon Detector ◽  
Air Shower ◽  
Early Results ◽  
Upper Limits ◽  
Shower Array ◽  
Air Shower Array

Early results of the search for Eγ > 1 PeV cosmic photons from point sources with the data of Carpet–2, an air-shower array equipped with a 175 m2 muon detector, are presented. They include 95% CL upper limits on PeV photon fluxes from stacked directions of high-energy IceCube neutrino events and from four predefined sources, Crab, Cyg X-3, Mrk 421 and Mrk 501. An insignificant excess of events from Mrk 421 will be further monitored. Prospects of the use of the upgraded installation, Carpet–3 (410 m2 muon detector), scheduled to start data taking in 2019, for searches of Eγ > 100 TeV photons, are briefly discussed.

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