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The success of the SWIFT/BAT and INTEGRAL missions has definitely opened anew window for follow-up and deep study of the transient gamma-ray sky. Thisnow appears as the access key to important progresses in the area ofcosmological research and deep understanding of the physics of compact objects.To detect in near real-time explosive events like Gamma-Ray bursts,thermonuclear flashes from Neutron Stars and other types of X-ray outbursts wehave developed a concept for a wide-field gamma-ray coded mask instrumentworking in the range 8-200 keV, having a sensitivity of 0.4 ph cm-2 s-1 in 1s(15-150 keV) and arcmin location accuracy over a sky region as wide as 3sr.This scientific requirement can be achieved by means of two large area, highspatial resolution CZT detection planes made of arrays of relatively large(~1cm2) crystals, which are in turn read out as matrices of smaller pixels. Toachieve such a wide Field-Of-View the two units can be placed at the sides of aS/C platform serving a payload with a complex of powerful X-ray instruments, asdesigned for the EDGE mission. The two units will be equipped with powerfulsignal read out system and data handling electronics, providing accurateon-board reconstruction of the source positions for fast, autonomous targetacquisition by the X-ray telescopes.

Design of a CZT Gamma-Camera for GRB and Fast Transient Follow-up: a Wide-Field-Monitor for the EDGE Mission