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An electroformed mirror array for high energy X-ray astronomyA design for a mirror array telescope for high energies with almost 1000 sq cm effective area at 7 keV is described. Briefly, it consists of 36 modules. Each module contains Wolter I mirrors nested 6 deep. The system is small enough to be flown on an Aries rocket. With the current mirrors, the angular resolution at high contrast is 20 arcsec and the half power diameter for images is 1.5 arcmin at 1.5 keV and 3.5 arcmin - 4 arcmin at 7 keV. Plans to improve upon this performance are discussed.
Document ID
19880062607
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ulmer, Melville P.
(Northwestern University Evanston, IL, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1988
Subject Category
Astronomy
Meeting Information
Meeting: Grazing incidence optics for astronomical and laboratory applications
Location: San Diego, CA
Country: United States
Start Date: August 17, 1987
End Date: August 19, 1987
Sponsors: SPIE
Accession Number
88A49834
Funding Number(s)
CONTRACT_GRANT: NAG5-181
Distribution Limits
Public
Copyright
Other

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