Minute-of-Arc Resolution Gamma Ray Imaging Experiment - MARGIE
S.C.Kappadath, P.P.Altice, M.L.Cherry, T.G.Guzik
J.G.Stacy
J.Macri, M.L.McConnell, J.M.Ryan
D.L.Band, J.L.Matteson
T.J. O'Neill, A.D.Zych
J.Buckley, P.L.Hink
Abstract
MARGIE (Minute-of-Arc Resolution Gamma-ray Imaging Experiment) is a
large area ( ~ 104 cm2), wide field-of-view ( ~ 1 sr),
hard X-ray/gamma-ray ( ~ 20-600 keV) coded-mask imaging telescope
capable of performing a sensitive survey of both steady and transient
cosmic sources. MARGIE has been selected for a NASA mission-concept
study for an Ultra Long Duration (100 day) Balloon flight. We describe
our program to develop the instrument based on new detector technology
of either cadmium-zinc-telluride (CZT) semiconductors or pixellated
cesium iodide (CsI) scintillators viewed by fast-timing bi-directional
charge-coupled devices (CCDs). The primary scientific objective is to
image faint Gamma-Ray Bursts (GRBs) in near-real-time at the low
intensity end (high-redshift) of the logN-logS distribution, thereby
extending the sensitivity of present observations. Other high-priority
scientific goals include a wide field survey of the Galactic center,
mapping the distribution of the Galactic 511 keV emission and
performing high-resolution spectral and temporal studies of active
galaxies.
File translated from TEX by TTH, version 2.32.
On 16 Jul 1999, 09:19.