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 cm2 for 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.
AIP Conference Proceedings
Digital Object Identifier (DOI)
Estimation of GRB detection by FiberGLAST Phengchamnan, S. and Aisaka, K. and Atac, M. and Binns, W. R. and Buckley, J. H. and Cherry, M. L. and Cline, D. and Dowkontt, P. and Epstein, J. W. and Finger, M. H. and Fishman, G. J. and Guzik, T. G. and Hink, P. L. and Israel, M. H. and Kappadath, S. C. and Karr, G. R. and Kippen, R. M. and Macri, J. and Mallozzi, R. S. and McConnell, M. L. and Pischalnikov, Y. and Paciesas, W. S. and Parnell, T. A. and Pendleton, G. N. and Preece, R. D. and Richardson, G. A. and Rielage, K. and Ryan, J. M. and Stacy, J. G. and Tümer, T. O. and Wallace, D. B. and Wilson, R. B., AIP Conference Proceedings, 526, 706-710 (2000), DOI:http://dx.doi.org/10.1063/1.1361626
© 2000 American Institute of Physics