Paper
18 October 1996 Imager onboard INTEGRAL
Pietro Ubertini, Guido Di Cocco, Francois Lebrun, L. Bassani, Angela Bazzano, Antony J. Bird, Kjell Broenstad, Ezio Caroli, M. Denis, Andrea Goldwurm, Claudio Labanti, Phillipe Laurent, Giuseppe Malaguti, I. F. Mirabel, Lorenzo Natalucci, M. E. Quadrini, Brian D. Ramsey, Victor Reglero, L. Sabau, Bruno Sacco, Ruediger Staubert, Laurent G. Vigroux, Martin C. Weisskopf, A. Zdziarski, Alex Zehnder
Author Affiliations +
Abstract
To follow up on the remarkable discoveries of the Compton Gamma Ray Observatory and GRANAT, the International Gamma Ray Astrophysics Laboratory (INTEGRAL) mission was selected by ESA as part of the agency's 'HORIZON 2000' strategic plan. It is scheduled to begin detailed gamma ray spectral and imaging studies, of unprecedented resolution, in the year 2001. One of the two main INTEGRAL instruments is a high performance imager. It features a coded aperture mask and a novel large area multilayer detector which utilizes both cadmium telluride and cesium iodide elements to deliver the fine angular-resolution approximately 12 arcmin, wide spectral response (15 keV to 10 MeV) and high resolution spectroscopy (6% at 100 keV) required to satisfy the mission's imaging objectives.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Pietro Ubertini, Guido Di Cocco, Francois Lebrun, L. Bassani, Angela Bazzano, Antony J. Bird, Kjell Broenstad, Ezio Caroli, M. Denis, Andrea Goldwurm, Claudio Labanti, Phillipe Laurent, Giuseppe Malaguti, I. F. Mirabel, Lorenzo Natalucci, M. E. Quadrini, Brian D. Ramsey, Victor Reglero, L. Sabau, Bruno Sacco, Ruediger Staubert, Laurent G. Vigroux, Martin C. Weisskopf, A. Zdziarski, and Alex Zehnder "Imager onboard INTEGRAL", Proc. SPIE 2806, Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions, (18 October 1996); https://doi.org/10.1117/12.253984
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Cited by 15 scholarly publications.
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KEYWORDS
Imaging systems

Sensors

X-rays

Spatial resolution

Calibration

Image resolution

Stars

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