Abstract
The hard X-ray detector (HXD-II) is one of the scientific payloads onboard Suzaku, the 5th Japanese cosmic X-ray satellite. After the launch in July 2005, all the HXD-II components, including the sensors and analog/digital electronics, have been working normally. In order to archive the maximum performance of the HXD-II, especially the GSO/BGO well-type phoswich counters, extensive in-orbit qualification and calibration have been carried out utilizing the data acquired in early operations. Major items of these efforts include; to estimate the circuit dead time, calibrate energy scale, optimize the event selection criteria for background reduction, study the background, and examine the detector response. As a result of these in-orbit calibrations, the HXD-II background in the 10 ∼ 600 keV range has been successfully lowered to (0.5 - 5.0) × 10-4 c s-1keV-1cm-2. This is the lowest among the background ever achieved in orbit by cosmic hard X-ray detectors.
Original language | English |
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Title of host publication | Hard X-Ray and Gamma-Ray Detector Physics and Penetrating Radiation Systems VIII |
DOIs | |
Publication status | Published - 2006 |
Externally published | Yes |
Event | Hard X-Ray and Gamma-Ray Detector Physics and Penetrating Radiation Systems VIII - San Diego, CA, United States Duration: 2006 Aug 14 → 2006 Aug 17 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
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Volume | 6319 |
ISSN (Print) | 0277-786X |
Conference
Conference | Hard X-Ray and Gamma-Ray Detector Physics and Penetrating Radiation Systems VIII |
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Country/Territory | United States |
City | San Diego, CA |
Period | 06/8/14 → 06/8/17 |
Keywords
- Astronomy satellite
- Detector
- Hard X-ray
- Spectroscopy
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering