The CIPHER telescope for hard X and soft g-ray polarimetry
E. Caroli, J.B. Stephen, W. Dusi
G. Bertuccio, M. Sampietro
A. J. Bird, A. J. Dean
W. Yu, C. Zhang
R. M. Curado da Silva, P. Siffert
CIPHER (Coded Imager and Polarimeter for High Energy Radiation) is a hard X and soft g-ray
spectroscopic and polarimetric coded mask telescope based on an array of Cadmium Telluride microspectrometers. The position sensitive detector (PSD) will be arranged in 4 modules of 32×32 crystals, each of 2×2 mm2 cross section and 10 mm thickness giving a total active area of about 160 cm2. The PSD is actively shielded by CsI crystals on the bottom and sides in order to reduce background and can operate over a wide energy range ( ~ 10 keV to 1 MeV).
The mask, based on a modified uniformly redundant array (MURA) pattern, is about 4 times the area of the PSD
and, being situated at about 100 cm from the CdTe array top surface, provides a wide field of view.
The CIPHER instrument is proposed for a balloon experiment, both in order to assess the
performance of such an instrumental concept for a small/medium size satellite survey mission and
to perform an innovative measurement of the Crab polarisation level. The CIPHER's wide field of
view allows the instrument to keep a single source within the field of view for a long observation
period without requiring a precise pointing system.
Herein we describe the instrument design, together with results obtained in our development
studies on CdTe detectors. Furthermore we present the expected operational performance in terms
of image and spectral quality (angular and energy resolution) and polarimetric capabilities for
an observation of the Crab pulsar from balloon altitudes.
File translated from TEX by TTH, version 2.32.
On 16 Jul 1999, 09:19.