| Autor: |
Phengchamnan, S., Aisaka, K., Atac, M., Binns, W. R., Buckley, J. H., Cherry, M. L., Cline, D., Dowkontt, P., Epstein, J. W., Finger, M. H., Fishman, G. J., Guzik, T. G., Hink, P. L., Israel, M. H., Kappadath, S. C., Karr, G. R., Kippen, R. M., Macri, J., Mallozzi, R. S., McConnell, M.L. |
| Předmět: |
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| Zdroj: |
AIP Conference Proceedings; 2000, Vol. 526 Issue 1, p706, 5p, 4 Charts |
| Abstrakt: |
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. © 2000 American Institute of Physics. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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