کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
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1833194 | 1027536 | 2006 | 4 صفحه PDF | دانلود رایگان |
The Japan/US Suzaku (formerly Astro-E2) astrophysics mission has been successfully launched. Suzaku is a powerful new orbiting observatory for studying extremely energetic processes in the universe. Sensitive X-ray spectrometers have been designed to enable precise measurements of high-energy processes in stars, supernova remnants, galaxies, clusters of galaxies, and the environments around neutron stars and black holes. One of the instruments is the high resolution X-ray spectrometer (XRS) that features a 32-pixel array of microcalorimeters with 6 eV (FWHM) spectral resolution, the first such device to be placed into orbit. We will describe the capabilities of the XRS instrument and present some of the very early in-flight results, which clearly show that this new technology can work extremely well in space.
Journal: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment - Volume 559, Issue 2, 15 April 2006, Pages 341–344