Search for pulsed TeV gamma-ray emission from young pulsars with HESS

被引：0
|
作者：
Schmidt, F [1 ]
Breitling, F [1 ]
Gillessen, S [1 ]
Konopelko, A [1 ]
Lohse, T [1 ]
Schlenker, S [1 ]
Schwanke, U [1 ]
Stegmann, C [1 ]
机构：
[1] Humboldt Univ, Inst Phys, D-12489 Berlin, Germany
来源：
High Energy Gamma-Ray Astronomy | 2005年 / 745卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The H.E.S.S. experiment is a next-generation imaging atmospheric Cherenkov detector with approximate to 1% Crab flux sensitivity for gamma-rays above 100 GeV. The full 4-telescope array has been operational since December 2003. The three young pulsars. Crab, Vela, and PSR B1706-44, are among the six pulsars whose pulsed emission has been detected LIP to energies of several GeV by EGRET. These pulsars have been selected for H.E.S.S. observations on grounds of their high rank in apparent spin-down luminosity E-sd/d2 and observability for the H.E.S.S. array. No Pulsed emission was found and flux upper limits are given.
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页码：377 / 381
页数：5
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