SEARCH FOR VERY HIGH ENERGY GAMMA-RAYS FROMACTIVE GALACTIC NUCLEI
SEARCH FOR VERY HIGH ENERGY GAMMA-RAYS FROMACTIVE GALACTIC NUCLEI
批准号:
12640292
负责人:
NISHIJIMA Kyoshi
金额:
$1.15万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
2000
资助国家:
日本
项目状态:
已结题
起止时间:
2000 至 2001
中文摘要
活动星系核的观测:我用CanGaroo-II 10米望远镜观测到了四个能量范围在几百GeV以上的活动星系核。对于PKS2155-304,源上扫描已观察约36小时,源外扫描约35小时,包括参与多波长运动。我没有看到PKS2155-304持续发射伽马射线的证据。对于400GeV以上,获得的通量上限(2δ)为1.2×10;;-11;cm;-2;秒;-1;-1;对于源扫描,PKS2005-489观察了33小时,离源扫描为31小时。在我2000年的观察期内进行了为期15天的RXTE观察。我没有看到PKS2005-489持续伽马射线发射的证据。在450GeV以上获得的磁通上限(2δ)为6.4×10;-12;cm;-2。在我的观察期间,这两个目标都保持在低水平状态。2001年初,我们利用极大天顶角技术,在其活跃态期间对MRK421进行了10个晚上的观测。结果表明,在10TeV以上的能量范围内,探测到了MRK421的伽马射线。触发模块的开发:为了降低能量阈值,通过蒙特卡罗模拟对触发条件进行了研究,发现聚簇触发是非常有效的。然后利用配套的可编程逻辑器件开发了智能触发模块,实现了集群式触发。
英文摘要
Observation of AGNs : I have observed four AGNs in the energy range above several hundred GeV using CANGAROO-II 10 m telescope. For PKS2155-304, observation has been done for about 36 hours for on-source scan and about 35 hours for off-source scan including participation in the mulriwave length campaign. I have seen no evidence for persistent gamma-ray emission from PKS2155-304. Flux upper limits(2δ)is obtained to be 1.2×10^<-11>cm^<-2> sec^<-1> for above 400GeV.PKS2005-489 was observed for 33 hours for on-source scan and 31 hours for off-source scan. RXTE observation were carried out for 15 days during my observation periods in 2000. I have seen no evidence for persistent gamma-ray emission from PKS2005-489. Flux upper limit(2δ) obtained for above 450 GeV is 6.4×10^<-12> cm^<-2> sec^<-1>. During my observation periods, both targets remained in a low level state. We observed Mrk421 for ten nights during its active state in early 2001 using the very large zenith angle technique. The result shows the detection of gamma-rays from Mrk421 in the energy range above 10 TeV. Considering the absorption by extragalactic infrared photons, this implies that the energy spectrum in a high level state is very hard.Development of trigger module : In order to lower the energy threshold, I studied the trigger condition by the Monte Carlo simulation, and I found clustering trigger is very effective. Then I develop the intelligent trigger module using complimentary programmable logic device to realize the clustering trigger.
期刊论文(3)
专著(0)
科研奖励(0)
会议论文
Kyoshi Nishijima: "Very High Energy Gamma-Ray Observations of AGNs with CANGAROO"Publication of the Astronomical Society of Australia. 19(in press). (2002)
Kyoshi Nishijima:“用 CANGAROO 对活动星系核进行甚高能伽马射线观测”澳大利亚天文学会出版物。
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通讯作者:
Kyoshi Nishijima: "Very High Energy Gamma-Ray Observations of AGNs with CANGAROO"Publication of the Astronomical Society of Australia. 19. 26-28 (2002)
Kyoshi Nishijima:“用 CANGAROO 对活动星系核进行甚高能伽马射线观测”澳大利亚天文学会出版物。
DOI:
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作者:
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通讯作者:
K. Nishijima: "Very High Energy Gamma-Ray Obervation of AGNs with CANGAROO"Publication of the Astronomical Society of Australia. 19. 26-28 (2002)
K. Nishijima:“用 CANGAROO 对 AGN 进行甚高能伽马射线观测”澳大利亚天文学会出版物。
DOI:
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发表时间:
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作者:
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通讯作者:
Development of the next generatiof PPD camera for the ground based gamma-ray telescope
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批准号:22340061
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项目类别:Grant-in-Aid for Scientific Research (B)
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资助金额:$11.4万
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财政年份:2010
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负责人:NISHIJIMA Kyoshi
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依托单位:
Development of all-sky infrared cloud monitor for the ground based gamma-ray observations
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批准号:17540266
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项目类别:Grant-in-Aid for Scientific Research (C)
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资助金额:$2.11万
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财政年份:2005
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负责人:NISHIJIMA Kyoshi
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依托单位:
海外基金