Translator Disclaimer
Paper
20 July 2016 The soft gamma-ray detector (SGD) onboard ASTRO-H
Author Affiliations +
Abstract
The Soft Gamma-ray Detector (SGD) is one of science instruments onboard ASTRO-H (Hitomi) and features a wide energy band of 60{600 keV with low backgrounds. SGD is an instrument with a novel concept of "Narrow field-of-view" Compton camera where Compton kinematics is utilized to reject backgrounds which are inconsistent with the field-of-view defined by the active shield. After several years of developments, the flight hardware was fabricated and subjected to subsystem tests and satellite system tests. After a successful ASTRO-H (Hitomi) launch on February 17, 2016 and a critical phase operation of satellite and SGD in-orbit commissioning, the SGD operation was moved to the nominal observation mode on March 24, 2016. The Compton cameras and BGO-APD shields of SGD worked properly as designed. On March 25, 2016, the Crab nebula observation was performed, and, the observation data was successfully obtained.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
PROCEEDINGS
16 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

Soft gamma-ray detector for the ASTRO-H Mission
Proceedings of SPIE (July 29 2010)
Soft gamma-ray detector for the ASTRO-H Mission
Proceedings of SPIE (September 17 2012)

Back to Top