Translator Disclaimer
29 July 2010 The high-resolution x-ray microcalorimeter spectrometer system for the SXS on ASTRO-H
Author Affiliations +
We present the science and an overview of the Soft X-ray Spectrometer onboard the ASTRO-H mission with emphasis on the detector system. The SXS consists of X-ray focusing mirrors and a microcalorimeter array and is developed by international collaboration lead by JAXA and NASA with European participation. The detector is a 6×6 format microcalorimeter array operated at a cryogenic temperature of 50 mK and covers a 3' ×3' field of view of the X-ray telescope of 5.6 m focal length. We expect an energy resolution better than 7 eV (FWHM, requirement) with a goal of 4 eV. The effective area of the instrument will be 225 cm2 at 7 keV; by a factor of about two larger than that of the X-ray microcalorimeter on board Suzaku. One of the main scientific objectives of the SXS is to investigate turbulent and/or macroscopic motions of hot gas in clusters of galaxies.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.


First measurements with DUO/ROSITA pnCCDs
Proceedings of SPIE (August 18 2005)
The Palermo XACT facility a new 35 m long...
Proceedings of SPIE (June 15 2006)
ASTRO-E/XRS calibration program and results
Proceedings of SPIE (October 22 1999)
Calibration of the AXAF observatory: overview
Proceedings of SPIE (July 11 1997)

Back to Top