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 objectives are to image faint Gamma-Ray Bursts (GRBs) in near-real-time at the low intensity (high-redshift) end of the logN-logS distribution, thereby extending the sensitivity of present observations, and to perform a wide field survey of the Galactic plane.
Space Science Center, Physics
AIP Conference Proceedings
Digital Object Identifier (DOI)
Minute-of-Arc Resolution Gamma ray Imaging Experiment—MARGIE Kappadath, S. C. and Altice, P. P. and Cherry, M. L. and Guzik, T. G. and Stacy, J. G. and Macri, J. and McConnell, M. L. and Ryan, J. M. and Band, D. L. and Matteson, J. L. and O’Neill, T. J. and Zych, A. D. and Buckley, J. and Hink, P. L., AIP Conference Proceedings, 510, 779-783 (2000), DOI:http://dx.doi.org/10.1063/1.1303304
© 2000 American Institute of Physics