W. W. Zhang,1 M. Atanassova,1 M. Biskach,1,2 P. N. Blake,1 G. Byron,1,2 K. W. Chan,1,3 T. Evans,1,2 C. Fleetwood,1,4 M. Hill,1 M. Hong,1,2 L. Jalota,1,3 L. Kolos,1 J. M. Mazzarella,1,2 R. McClelland,1,2 L. Olsen,1,2 R. Petre,1 D. Robinson,1 T. T. Saha,1 M. Sharpe,1,2 M. V. Gubarev,5 W. D. Jones,5 T. Kester,5 S. L. O'Dellhttps://orcid.org/0000-0002-1868-8056,5 D. Caldwell,6 W. Davis,6 M. Freeman,6 W. Podgorski,6 P. B. Reid,6 S. Romaine6
1NASA Goddard Space Flight Ctr. (United States) 2Stinger Ghaffarian Technologies, Inc. (United States) 3Univ. of Maryland, Baltimore County (United States) 4Ball Aerospace & Technologies Corp. (United States) 5NASA Marshall Space Flight Ctr. (United States) 6Smithsonian Astrophysical Observatory (United States)
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The International X-ray Observatory (IXO) is designed to conduct spectroscopic, imaging, and timing studies
of astrophysical phenomena that take place as near as in the solar system and as far as in the early universe. It
is a collaborative effort of ESA, JAXA, and NASA. It requires a large X-ray mirror assembly with an
unprecedented X-ray collection area and a suite of focal plane detectors that measure every property of each
photon. This paper reports on our effort to develop the necessary technology to enable the construction of the
mirror assembly required by IXO.
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W. W. Zhang, M. Atanassova, M. Biskach, P. N. Blake, G. Byron, K. W. Chan, T. Evans, C. Fleetwood, M. Hill, M. Hong, L. Jalota, L. Kolos, J. M. Mazzarella, R. McClelland, L. Olsen, R. Petre, D. Robinson, T. T. Saha, M. Sharpe, M. V. Gubarev, W. D. Jones, T. Kester, S. L. O'Dell, D. Caldwell, W. Davis, M. Freeman, W. Podgorski, P. B. Reid, S. Romaine, "Mirror technology development for the International X-ray Observatory mission (IXO)," Proc. SPIE 7732, Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, 77321G (29 July 2010); https://doi.org/10.1117/12.857536