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We report a study of a new X-ray interferometer with a beam splitter for future observation of celestial objects. A
possible configuration of an interferometer is proposed. By using a beam splitter, the length of the interferometer
becomes short and without a formation flight of satellites a reasonable X-ray interferometric observation can be
possible. An observation of early type stars is discussed. A laboratory experiment for performance verification
is also discussed.
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S. Kitamoto, H. Murakami, D. Takei, K. Sakata, Y. Yoshida, "A new x-ray interferometer," Proc. SPIE 8147, Optics for EUV, X-Ray, and Gamma-Ray Astronomy V, 81471P (6 October 2011); https://doi.org/10.1117/12.894244