Author/Authors :
Takahashi، نويسنده , , Tadayuki and Nakazawa، نويسنده , , Kazuhiro and Watanabe، نويسنده , , Shin-ichiro Sato، نويسنده , , Goro and Mitani، نويسنده , , Takefumi and Tanaka، نويسنده , , Takaaki and Oonuki، نويسنده , , Kousuke and Tamura، نويسنده , , Ken’ichi and Tajima، نويسنده , , Hiroyasu and Kamae، نويسنده , , Tuneyoshi and Madejski، نويسنده , , Greg and Nomachi، نويسنده , , Masaharu and Fukazawa، نويسنده ,
Abstract :
Cadmium telluride (CdTe) and cadmium zinc telluride (CdZnTe) have been regarded as promising semiconductor materials for hard X-ray and γ -ray detection. The high-atomic number of the materials ( Z Cd = 48 , Z Te = 52 ) gives a high quantum efficiency in comparison with Si. The large band-gap energy ( E g = 1.5 eV ) allows to operate the detector at room temperature. Based on recent achievements in high-resolution CdTe detectors, in the technology of ASICs and in bump-bonding, we have proposed the novel hard X-ray and γ -ray detectors for the NeXT mission in Japan. The high-energy response of the super mirror onboard NeXT will enable us to perform the first sensitive imaging observations up to 80 keV. The focal plane detector, which combines a fully depleted X-ray CCD and a pixellated CdTe detector, will provide spectra and images in the wide energy range from 0.5 to 80 keV. In the soft γ -ray band up to ∼ 1 MeV , a narrow field-of-view Compton γ -ray telescope utilizing several tens of layers of thin Si or CdTe detector will provide precise spectra with much higher sensitivity than present instruments. The continuum sensitivity will reach several × 10 - 8 photons - 1 keV - 1 cm - 2 in the hard X-ray region and a few × 10 - 7 photons - 1 keV - 1 cm - 2 in the soft γ -ray region.
Keywords :
? -ray astronomy , Compton telescope , CZT , CdTe