首页   按字顺浏览 期刊浏览 卷期浏览 Estimation of GRB detection by FiberGLAST
Estimation of GRB detection by FiberGLAST

 

作者: S. Phengchamnan,   K. Aisaka,   M. Atac,   W. R. Binns,   J. H. Buckley,   M. L. Cherry,   D. Cline,   P. Dowkontt,   J. W. Epstein,   M. H. Finger,   G. J. Fishman,   T. G. Guzik,   P. L. Hink,   M. H. Israel,   S. C. Kappadath,   G. R. Karr,   R. M. Kippen,   J. Macri,   R. S. Mallozzi,   M. L. McConnell,   Y. Pischalnikov,   W. S. Paciesas,   T. A. Parnell,   G. N. Pendleton,   R. D. Preece,   G. A. Richardson,   K. Rielage,   J. M. Ryan,   J. G. Stacy,   T. O. Tu¨mer,   D. B. Wallace,   R. B. Wilson,  

 

期刊: AIP Conference Proceedings  （AIP Available online 1900）
卷期: Volume 526, issue 1  

页码: 706-710

 

ISSN:0094-243X

 

年代: 1900

 

DOI:10.1063/1.1361626

 

出版商: AIP

 

数据来源: AIP

 

摘要:

FiberGLAST is one of several instrument concepts being developed for possible inclusion as the primary Gamma-ray Large Area Space Telescope (GLAST) instrument. The predicted FiberGLAST effective area is more than 12,000 cm2for energies between 30 MeV and 300 GeV, with a field of view that is essentially flat from 0°–80°. The detector will achieve a sensitivity more than 10 times that of EGRET. We present results of simulations that illustrate the sensitivity of FiberGLAST for the detection of gamma-ray bursts. ©2000 American Institute of Physics.

 

点击下载:  PDF (915KB)



返 回