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M. L. McConnell, P. F. Bloser, J. R. Macri, J. M. Ryan (UNH), G. L. Case, J. G. Stacy (LSU/SU), M. L. Cherry, T. G. Guzik, B. Schaefer, J. P. Wefel (LSU), J. Cravens (SwRI), K. Hurley (UCB), R. M. Kippen, W. T. Vestrand (LANL), R. S. Miller, W. Paciesas (UAH)
The primary scientific mission of the Black Hole Finder Probe (BHFP), part of the NASA Beyond Einstein program, is to survey the local Universe for black holes over a wide range of mass and accretion rate. One approach to such a survey is a hard X-ray coded-aperture imaging mission operating in the 10--600 keV energy band, a spectral range that is considered to be especially useful in the detection of black hole sources. The development of new inorganic scintillator materials provides improved performance (for example, with regards to energy resolution and timing) that is well suited to the BHFP science requirements. Detection planes formed with these materials coupled with a new generation of readout devices represent a major advancement in the performance capabilities of scintillator-based gamma cameras. Here, we discuss the Coded Aperture Survey Telescope for Energetic Radiation (CASTER), a concept that represents a BHFP based on the use of the latest scintillator technology.
The author(s) of this abstract have provided an email address for comments about the abstract: Mark.McConnell@unh.edu
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Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.