A high energy resolution experiment in the hard X-ray rangeThe Low Energy Gamma-Ray Spectrometer (LEGS), a joint project among NASA/GSFC, CEN-SACLAY, and Rice University, is designed to perform fine energy resolution measurements of astrophysical sources. In its low energy configuration (20-800 keV energy range) the instrument uses three planar detectors (effective area of 53 sq cm) surrounded by a combination of passive Fe and active NaI for shielding and collimation (FOW of about 5 x 10 deg FWHM). In a typical one-day balloon flight, LEGS sensitivity limit (3 sigma) for narrow line features is not greater than about 0.0003 ph/sq cm s (at 100 kev).
Document ID
19850040855
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Paciesas, W. (NASA Goddard Space Flight Center Greenbelt; Maryland, University, College Park, MD; Alabama, University, Huntsville, AL, United States)
Baker, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Cline, T. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Ehrmann, C. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Gehrels, N. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Teegarden, B. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Boclet, D. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Durouchoux, PH. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Hameury, J. M. (Commissariat a l'Energie Atomique, Service d'Astrophysique, Gif-sur-Yvette Essonne, France)
Haymes, R. (Rice University Houston, TX, United States)