[en] The gamma-ray telescope IBIS, on board the INTEGRAL satellite, features a coded-mask aperture, active and passive shields and two detector arrays. The first one (ISGRI) is an assembly of 16384 CdTe detectors (4x4 mm large, 2 mm thick) operating at room temperature. ISGRI covers the lower part (15 keV-1 MeV) of the IBIS energy range (15 keV-10 MeV). Detectors are arranged on polycells, each including 16 crystals, connected to their front-end electronics (ASICs). Each of the eight independent ISGRI modules are made of 128 polycells. The ASICs contain a low noise charge-sensitive preamplifier and feature pulse rise-time measurement in addition to the standard pulse height measurement. This permits to compute a charge loss correction based on the charge drift time. After application of this correction, a spectral resolution around 7.5% at 122 keV is obtained with the ASICs. Today, 16 polycells have been mounted on the first representative ISGRI module. This module has been interfaced with the entire ISGRI data-processing electronics and forms the engineering model of ISGRI. After a presentation of the scientific context, this paper describes the ISGRI design with particular emphasis on the detectors, the polycells performances and the module assembly. gamma-detection

[en] A low-power low-noise multichannel integrated circuit is implemented in 1.2 μm CMOS technology. This circuit is designed for space γ-ray spectrometer using arrays of CdTe radiation detectors in the 20-750 keV range. The space environment needs rad-tolerant specifications for the technology like 20 krad of total integrated dose and consumption limited to 2 mW/channel. Each channel includes a low-noise charge-sensitive preamplifier, fitted band-pass filters, peak amplitude and rise-time measurements; these enable a remote rise-time corrected γ-ray energy spectral analysis. The circuit includes an associated logic block, dedicated to the internal timing, functional organization, external communication and data transfer. (orig.)