Results 181 to 190 of about 2,168,923 (219)
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Evaluation of In-Orbit Thermal Performance of X-Ray Astronomy Satellite "Hitomi"

, 2017
This study presents the evaluation results of the thermal performance for Japan Aerospace Exploration Agency’s X-ray astronomy satellite (Hitomi) ASTRO-H mission.
N. Iwata   +9 more
semanticscholar   +1 more source

Lightweight and high-resolution single crystal silicon optics for x-ray astronomy

Astronomical Telescopes + Instrumentation, 2016
We describe an approach to building mirror assemblies for next generation X-ray telescopes. It incorporates knowledge and lessons learned from building existing telescopes, including Chandra, XMM-Newton, Suzaku, and NuSTAR, as well as from our direct ...
Will Zhang   +7 more
semanticscholar   +1 more source

Advancements in hard x-ray multilayers for x-ray astronomy

SPIE Optical Engineering + Applications, 2015
This paper is focused on recent progress in the development of broad-band multilayer coatings designed for hard X-ray energies, for use in future astronomical telescopes.
D. Windt
semanticscholar   +1 more source

Chi-squared and C statistic minimization for low count per bin data. [Sampling in X ray astronomy]

, 1989
Results are presented from a computer simulation comparing two statistical fitting techniques on data samples with large and small counts per bin; the results are then related specifically to X-ray astronomy.
J. Nousek, David Shue
semanticscholar   +1 more source

Uniformity of Kilo-Pixel Arrays of Transition-Edge Sensors for X-ray Astronomy

IEEE transactions on applied superconductivity, 2015
We are developing kilo-pixel arrays of transition-edge sensor (TES) microcalorimeters for use in future laboratory and space based X-ray astrophysics experiments. These arrays are required to achieve an energy resolution of ΔEFWHM
S. Smith   +12 more
semanticscholar   +1 more source

Design Parameters of Paraboloid-Hyperboloid Telescopes for X-ray Astronomy.

Applied Optics, 1972
We have evaluated the principal optical characteristics of paraboloid-hyperboloid x-ray telescopes by a ray-tracing procedure; we find that our results for resolution, focal plane curvature, and finite source distance effects may be approximated in terms
L. Vanspeybroeck, R. Chase
semanticscholar   +1 more source

X-ray characterization of curved crystals for hard x-ray astronomy

Europe Optics + Optoelectronics, 2015
Among the methods to focus photons the diffraction in crystals results as one of the most effective for high energy photons. An assembling of properly oriented crystals can form a lens able to focus x-rays at high energy via Laue diffraction in ...
E. Buffagni   +4 more
semanticscholar   +1 more source

X-ray astronomy comes of age

Nature, 2022
B. Wilkes   +3 more
semanticscholar   +1 more source

Instrumental Technique in X-Ray Astronomy

, 1975
This review is confined to nonfocusing, high-sensitivity counter techniques used in the detection of cosmic photons in the 0.20 to 300 keV range. The status of x-ray astronomy, photon interactions, detector principles and applications, sensitivity ...
L. Peterson
semanticscholar   +1 more source

Optics for the x-ray imaging concentrators aboard the x-ray astronomy satellite SAX.

Applied Optics, 1988
The scientific instrumentation onboard the Italian satellite for x-ray astronomy (SAX) foresees x-ray imaging concentrators operating in the 0.1-10-keV energy range with a spatial resolution of 1 min of arc.
O. Citterio   +8 more
semanticscholar   +1 more source

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