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Angular Fluctuations in the CXB: Is Fe 6.4 keV Line Tomography of the Large-Scale Structure Feasible?

Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201219796
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Abstract

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Categories
AstrophysicsAstronomyPlanetary ScienceSpace
Date

October 22, 2012

Authors
G. HütsiM. GilfanovR. Sunyaev
Publisher

EDP Sciences


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