4.7 Article

The first γ-ray detection of the narrow-line Seyfert 1 FBQS J1644+2619

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv1278

关键词

galaxies: active; galaxies: individual: FBQS J1644+2619; galaxies: nuclei; galaxies: Seyfert; gamma-rays: general

资金

  1. National Aeronautics and Space Administration
  2. Department of Energy in the United States
  3. Commissariat a l'Energie Atomique
  4. Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France
  5. Agenzia Spaziale Italiana
  6. Istituto Nazionale di Fisica Nucleare in Italy
  7. Ministry of Education, Culture, Sports, Science and Technology (MEXT)
  8. High Energy Accelerator Research Organization (KEK)
  9. Japan Aerospace Exploration Agency (JAXA) in Japan
  10. K. A. Wallenberg Foundation
  11. Swedish Research Council
  12. Swedish National Space Board in Sweden

向作者/读者索取更多资源

We report the discovery of gamma-ray emission from the narrow-line Seyfert 1 (NLSy1) galaxy FBQS J1644+2619 by the Large Area Telescope on board the Fermi satellite. The Third Fermi LAT Source catalogue reports an unidentified gamma-ray source, detected over the first four years of Fermi operation, 0 degrees.23 from the radio position of the NLSy1. Analysing 76 months of gamma-ray data (2008 August 4-2014 December 31) we are able to better constrain the localization of the gamma-ray source. The new position of the gamma-ray source is 0 degrees.05 from FBQS J1644+2619, suggesting a spatial association with the NLSy1. This is the sixth NLSy1 detected at high significance by Fermi-LAT so far. Notably, a significant increase of activity was observed in gamma-rays from FBQS J1644+2619 during 2012 July-October, and an increase of activity in the V band was detected by the Catalina Real-Time Sky Survey in the same period.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据