IBIS: The Imager on-board INTEGRAL

• Published in: Astronomy and astrophysics (Berlin) 2003-11, Vol.411 (1), p.L131-L139
• Main Authors: Ubertini, P., Lebrun, F., Di Cocco, G., Bazzano, A., Bird, A. J., Broenstad, K., Goldwurm, A., La Rosa, G., Labanti, C., Laurent, P., Mirabel, I. F., Quadrini, E. M., Ramsey, B., Reglero, V., Sabau, L., Sacco, B., Staubert, R., Vigroux, L., Weisskopf, M. C., Zdziarski, A. A.
• Format: Article
• Language: English
• Subjects: gamma-ray imaging; IBIS; INTEGRAL
• ISSN: 0004-6361; 1432-0746
• DOI: 10.1051/0004-6361:20031224

The IBIS telescope is the high angular resolution gamma-ray imager on-board the INTEGRAL Observatory, successfully launched from Baikonur (Kazakhstan) the 17th of October 2002. This medium size ESA project, planned for a 2 year mission with possible extension to 5, is devoted to the observation of the gamma-ray sky in the energy range from 3 keV to 10 MeV (Winkler [CITE]). The IBIS imaging system is based on two independent solid state detector arrays optimised for low ($15{-}1000$ keV) and high ($0.175{-}10.0$ MeV) energies surrounded by an active VETO System. This high efficiency shield is essential to minimise the background induced by high energy particles in the highly excentric out of van Allen belt orbit. A Tungsten Coded Aperture Mask, 16 mm thick and ~1 squared meter in dimension is the imaging device. The IBIS telescope will serve the scientific community at large providing a unique combination of unprecedented high energy wide field imaging capability coupled with broad band spectroscopy and high resolution timing over the energy range from X to gamma rays. To date the IBIS telescope is working nominally in orbit since more than 9 month.