...
首页> 外文期刊>The Astrophysical journal >AGILE DETECTION OF A STRONG GAMMA-RAY FLARE FROM THE BLAZAR 3C 454.3
【24h】

AGILE DETECTION OF A STRONG GAMMA-RAY FLARE FROM THE BLAZAR 3C 454.3

机译:从BLAZAR 3C 454.3的强伽玛射线耀斑的敏捷检测

获取原文
获取原文并翻译 | 示例

摘要

We report the first blazar detection by AGILE. AGILE detected 3C 454.3 during a period of strongly enhanced optical emission in 2007 July. AGILE observed the source with a dedicated repointing during the period 2007 July 24-30 with its two co-aligned imagers, the Gamma-Ray Imaging Detector and the hard X-ray imager Super-AGILE sensitive in the 30 MeV to 50 GeV and 18-60 keV ranges, respectively. Over the entire period, AGILE detected γ-ray emission from 3C 454.3 at a significance level of 13.8 σ with an average flux (E > 100 MeV) of (280 ± 40) × 10~(-8) photons cm~(-2) s~(-1). The γ-ray flux appears to be variable toward the end of the observation. No emission was detected by Super-AGILE in the energy range 20-60 keV, with a 3 σ upper limit of 2.3 × 10~(-3) photons cm~(-2) s~(-1). The γ-ray flux level of 3C 454.3 detected by AGILE is the highest ever detected for this quasar and among the most intense γ-ray fluxes ever detected from flat-spectrum radio quasars.
机译:我们报告了AGILE首次进行的Blazar检测。在2007年7月,AGILE在强烈增强的光发射期间检测到3C 454.3。在2007年7月24日至30日期间,AGILE对其源进行了专门的重新观测,使用了两个对准的成像仪,即在30 MeV至50 GeV和18 MeV敏感的伽玛射线成像探测器和硬X射线成像仪Super-AGILE。分别为-60 keV范围。在整个期间,AGILE探测到3C 454.3以13.8σ的显着性水平发射的γ射线,平均通量(E> 100 MeV)为(280±40)×10〜(-8)光子cm〜(-2 )s〜(-1)。 γ射线通量在观察结束时似乎是可变的。 Super-AGILE在20-60 keV的能量范围内未检测到发射,其3σ上限为2.3×10〜(-3)光子cm〜(-2)s〜(-1)。由AGILE检测到的3C 454.3的γ射线通量水平是该类星体中检测到的最高水平,并且是从平谱无线电类星体中检测到的最强的γ射线通量之一。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号