FOREWARD

   In 1995, NASA formed the Gamma-Ray Astronomy Program Working Group (GRAPWG) to formulate recommendations for future directions in NASA's gamma-ray astronomy program. The energy range considered in this study extends from hard x-rays (>~ 15 keV) through TeV gamma rays. The mandate of the working group is to recommend a road map to the future for use as an input to the next NASA strategic plan, currently slated for 1997. The working group, whose membership is given below, has met four times over the past 2 years. It has assessed the state of the field including current missions and approved future missions, the critical scientific problems open today, the promising technologies for the future, the mission priorities for the future, and the needs for data analysis and theory. This report presents a summary of the GRAPWG findings and gives detailed recommendations. The acronyms used in the report are defined in Appendix A. Gamma-Ray Astronomy Program Working Group Members:
Elena Aprile (Columbia)
Alan Bunner (NASA) [Ex-Officio (NASA Headquarters)]
Neil Gehrels (GSFC) [Co-Chair]
Jonathan Grindlay (Harvard)
Gerald Fishman (MSFC)
W. Neil Johnson (NRL)
Kevin Hurley (UCB/SSL)
Steve Kahn (Columbia)
Richard Lingenfelter (UCSD)
Peter Michelson (Stanford)
Thomas Prince (Caltech) [Co-Chair]
Roger Romani (Stanford)
James Ryan (UNH)
Bonnard Teegarden (GSFC)
David Thompson (GSFC)
Trevor Weekes (Harvard/Smithsonian)
Stanford Woosley (UCSC)       

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