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The Astro-H Soft X-Ray MirrorThe Astro-H is led by the Japanese Space Agency (JAXA) in collaboration with many other institutions including the NASA Goddard Space Flight Center. Goddard's contributions include two soft X-ray telescopes (SXTs). The telescopes have an effective area of 562 square cm at 1 keV and 425 square cm at 6 keV with an image quality requirement of 1.7 arc-minutes half power diameter (HPD). The engineering model has demonstrated 1.1 arc-minutes HPD error. The design of the SXT is based on the successful Suzaku mission mirrors with some enhancements to improve the image quality. Two major enhancements are bonding the X-ray mirror foils to alignment bars instead of allowing the mirrors to float, and fabricating alignment bars with grooves within 5 microns of accuracy. An engineering model SXT was recently built and subjected to several tests including vibration, thermal, and X-ray performance in a beamline. Several lessons were learned during this testing that will be incorporated in the flight design. Test results and optical performance are discussed, along with a description of the design of the SXT.
Document ID
20120009486
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Robinson, David
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Okajima, Takashi
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Serlemitsos, Peter
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Soong, Yang
(Universities Space Research Association Greenbelt, MD, United States)
Date Acquired
August 25, 2013
Publication Date
January 1, 2012
Subject Category
Optics
Report/Patent Number
IEEAC Paper 1565
GSFC.JA.6061.2012
Report Number: IEEAC Paper 1565
Report Number: GSFC.JA.6061.2012
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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