IDENTIFICATION OF THE EARLY FERMI/LAT GAMMA-RAY BRIGHT OBJECTS WITH EXTRAGALACTIC VLBI SOURCES

被引:57
作者
Kovalev, Y. Y. [1 ,2 ]
机构
[1] Max Planck Inst Radioastron, D-53121 Bonn, Germany
[2] PN Lebedev Phys Inst, Ctr Astro Space, Moscow 117997, Russia
基金
俄罗斯基础研究基金会; 美国国家航空航天局;
关键词
catalogs; galaxies: active; gamma rays: observations; radio continuum: galaxies; ACTIVE GALACTIC NUCLEI; ALL-SKY SURVEY; CELESTIAL REFERENCE FRAME; LARGE-AREA TELESCOPE; CALIBRATOR SURVEY; 5; GHZ; RADIO-SOURCES; SOURCE LIST; BLAZAR; POLARIMETRY;
D O I
10.1088/0004-637X/707/1/L56
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A list of 205 gamma-ray strong objects was reported recently as a result of a three-month integration with the Large Area Telescope on board the Fermi Gamma-Ray Space Telescope. We attempted identification of these objects, cross-correlating the gamma-ray positions with very long baseline interferometry (VLBI) positions of a large all-sky sample of extragalactic radio sources selected on the basis of their parsec-scale flux density. The original associations reported by the Fermi team are confirmed, and six new identifications are suggested. A Monte Carlo analysis shows that the fraction of chance associations in our analysis is less than 5%, and confirms that the vast majority of gamma-ray bright extragalactic sources are radio-loud blazars with strong parsec-scale jets. A correlation between the parsec-scale radio and gamma-ray flux is supported by our analysis of a complete VLBI flux-density-limited sample of extragalactic jets. The effectiveness of using a VLBI catalog to find associations between gamma-ray detections and compact extragalactic radio sources, especially near the Galactic plane, is demonstrated. It is suggested that VLBI catalogs should be used for future identification of Fermi/LAT objects.
引用
收藏
页码:L56 / L59
页数:4
相关论文
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