The Si/CdTe semiconductor camera of the ASTRO-H Hard X-ray Imager (HXI)
The Hard X-ray Imager (HXI) is one of the instruments onboard the ASTRO-H mission [1–4] to be launched in early 2016. The HXI is the focal plane detector of the hard X-ray reflecting telescope that covers an energy range from 5 to 80keV. It will execute observations of astronomical objects with a se...
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Published in | Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Vol. 831; pp. 235 - 241 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
21.09.2016
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Subjects | |
Online Access | Get full text |
ISSN | 0168-9002 1872-9576 |
DOI | 10.1016/j.nima.2016.03.038 |
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Abstract | The Hard X-ray Imager (HXI) is one of the instruments onboard the ASTRO-H mission [1–4] to be launched in early 2016. The HXI is the focal plane detector of the hard X-ray reflecting telescope that covers an energy range from 5 to 80keV. It will execute observations of astronomical objects with a sensitivity for point sources as faint as 1/100,000 of the Crab nebula at >10keV. The HXI camera – the imaging part of the HXI – is realized by a hybrid semiconductor detector system that consists of silicon (Si) and cadmium telluride (CdTe) semiconductor detectors. Here, we present the final design of the HXI camera and report on the development of the flight model. The camera is composed of four layers of Double-sided Silicon Strip Detectors (DSSDs) and one layer of CdTe Double-sided Strip Detector (CdTe-DSD), each with an imaging area of 32mm×32mm. The strip pitch of the Si and CdTe sensors is 250μm, and the signals from all 1280 strips are processed by 40 Application Specified Integrated Circuits (ASICs) developed for the HXI. The five layers of sensors are vertically stacked with a 4mm spacing to increase the detection efficiency. The thickness of the sensors is 0.5mm for the Si, and 0.75mm for the CdTe. In this configuration, soft X-ray photons will be absorbed in the Si part, while hard X-ray photons will go through the Si part and will be detected in the CdTe part. The design of the sensor trays, peripheral circuits, power connections, and readout schemes are also described. The flight models of the HXI camera have been manufactured, tested and installed in the HXI instrument and then on the satellite. |
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AbstractList | The Hard X-ray Imager (HXI) is one of the instruments onboard the ASTRO-H mission [1–4] to be launched in early 2016. The HXI is the focal plane detector of the hard X-ray reflecting telescope that covers an energy range from 5 to 80keV. It will execute observations of astronomical objects with a sensitivity for point sources as faint as 1/100,000 of the Crab nebula at >10keV. The HXI camera – the imaging part of the HXI – is realized by a hybrid semiconductor detector system that consists of silicon (Si) and cadmium telluride (CdTe) semiconductor detectors. Here, we present the final design of the HXI camera and report on the development of the flight model. The camera is composed of four layers of Double-sided Silicon Strip Detectors (DSSDs) and one layer of CdTe Double-sided Strip Detector (CdTe-DSD), each with an imaging area of 32mm×32mm. The strip pitch of the Si and CdTe sensors is 250μm, and the signals from all 1280 strips are processed by 40 Application Specified Integrated Circuits (ASICs) developed for the HXI. The five layers of sensors are vertically stacked with a 4mm spacing to increase the detection efficiency. The thickness of the sensors is 0.5mm for the Si, and 0.75mm for the CdTe. In this configuration, soft X-ray photons will be absorbed in the Si part, while hard X-ray photons will go through the Si part and will be detected in the CdTe part. The design of the sensor trays, peripheral circuits, power connections, and readout schemes are also described. The flight models of the HXI camera have been manufactured, tested and installed in the HXI instrument and then on the satellite. |
Author | Murakami, Hiroaki Hagino, Kouichi Kobayashi, Shogo Masukawa, Kazunori Takahashi, Hiromitsu Nakano, Toshio Sato, Rie Nakazawa, Kazuhiro Makishima, Kazuo Harayama, Atsushi Kanematsu, Hironori Takeda, Shin׳ichiro Miyake, Katsuma Saito, Shinya Onishi, Mitsunobu Takahashi, Tadayuki Odaka, Hirokazu Kataoka, Jun Watanabe, Shin Kokubun, Motohide Genba, Kei Noda, Hirofumi Sato, Goro Katsuragawa, Miho Mimura, Taketo Yuasa, Takayuki Tajima, Hiroyasu Sato, Tamotsu Kuroda, Yoshikatsu Kawaharada, Madoka |
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Kazuhiro organization: Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan – sequence: 20 givenname: Hirofumi surname: Noda fullname: Noda, Hirofumi organization: Nishina Center for Accelerator-Based Science, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan – sequence: 21 givenname: Hirokazu surname: Odaka fullname: Odaka, Hirokazu organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuou, Sagamihara, Kanagawa 252-5210, Japan – sequence: 22 givenname: Mitsunobu surname: Onishi fullname: Onishi, Mitsunobu organization: Nagoya Guidance and Propulsion Systems Works, Mitsubishi Heavy Industry Ltd., 1200 Higashi Tanaka, Komaki, Aichi 485-8561, Japan – sequence: 23 givenname: Shinya surname: Saito fullname: Saito, Shinya organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuou, Sagamihara, Kanagawa 252-5210, Japan – sequence: 24 givenname: Rie surname: Sato fullname: Sato, Rie organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuou, Sagamihara, Kanagawa 252-5210, Japan – sequence: 25 givenname: Tamotsu surname: Sato fullname: Sato, Tamotsu organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuou, Sagamihara, Kanagawa 252-5210, Japan – sequence: 26 givenname: Hiroyasu surname: Tajima fullname: Tajima, Hiroyasu organization: Solar Terrestrial Environment Laboratory, Nagoya University, Chikusa, Nagoya, Aichi 464-8601, Japan – sequence: 27 givenname: Hiromitsu surname: Takahashi fullname: Takahashi, Hiromitsu organization: Department of Physical Science, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan – sequence: 28 givenname: Tadayuki surname: Takahashi fullname: Takahashi, Tadayuki organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuou, Sagamihara, Kanagawa 252-5210, Japan – sequence: 29 givenname: Shin׳ichiro surname: Takeda fullname: Takeda, Shin׳ichiro organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuou, Sagamihara, Kanagawa 252-5210, Japan – sequence: 30 givenname: Takayuki surname: Yuasa fullname: Yuasa, Takayuki organization: Nishina Center for Accelerator-Based Science, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan |
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Snippet | The Hard X-ray Imager (HXI) is one of the instruments onboard the ASTRO-H mission [1–4] to be launched in early 2016. The HXI is the focal plane detector of... |
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SubjectTerms | ASTRO-H HXI CdTe Hard X-ray detector Semiconductor detector Silicon Strip detector |
Title | The Si/CdTe semiconductor camera of the ASTRO-H Hard X-ray Imager (HXI) |
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