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<title>Imaging performance of the XMM-Newton x-ray telescopes</title> [PDF]
The in-orbit imaging performance of the three X-ray telescopes on board of the X-ray astronomy observatory XMM-Newton is presented and compared with the performance measured on ground at the MPE PANTER test facility. The comparison shows an excellent agreement between the on ground and in-orbit performance.
B. Aschenbach+7 more
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Improving the Resolution of X-Ray Telescopes with Occulting Satellites [PDF]
One of the challenges of X-ray astronomy is how to both collect large numbers of photons yet attain high angular resolution. Because X-ray telescopes utilize grazing optics, to collect more photons requires a larger acceptance angle which in turn compromises the angular resolution. All X-ray telescopes thus have angular resolution far poorer than their
Craig J. Copi, Glenn D. Starkman
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The challenge to large optical telescopes from x-ray astronomy [PDF]
In the ROSAT era of the mid-1990's, the problems facing deep X-ray surveys could be largely solved with 10 m class telescopes. In the first decade of this new millennium, with X-ray telescopes such as the Chandra X-ray Observatory and XMM-Newton in operation, deep X-ray surveys are challenging 10 m telescopes.
A. E. Hornschemeier
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The X-Ray Telescope of the CAST Experiment [PDF]
5 pages, 9 ...
R. Kotthaus+7 more
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The swift x-ray telescope: status and performance [PDF]
9 pages, 14 ...
D. N. Burrows+25 more
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The eROSITA X-ray telescope on SRG [PDF]
eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the primary instrument on the Spectrum-Roentgen-Gamma (SRG) mission, which was successfully launched on July 13, 2019, from the Baikonour cosmodrome. After the commissioning of the instrument and a subsequent calibration and performance verification phase, eROSITA started a survey of
Predehl P.+94 more
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Characterization of a lobster-eye type X-ray telescope [PDF]
Lobster-eye type X-ray telescopes use reflecting plano mirrors under grazing incidence and can observe a large field of view. As part of a Bavarian-Czech cooperation, two telescopes were build, equipped with mirrors coated with gold and iridium.
Döhring Thorsten+5 more
doaj +1 more source
Simulation of a Simple Wolter Telescope of Type I by Geant4 for Some Widely Used Materials [PDF]
At the present work, the reflection of X-rays from surfaces composed of silicon, gold, iridium, and nickel is simulated in the range of E ≤ 5 keV energy for the two cases, which includes raw mirror surfaces and a typical Wolter-I optics-based X-ray ...
Mehdi Abbasian Motlagh+1 more
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Small Spacecraft Payload Study for X-ray Astrophysics including GRB Science
This paper presents microsatellite spacecraft payload study for prompt observation of transient astrophysical objects in X-ray energy range. By combining telescope concepts and miniaturized detectors, the small spacecraft will be able to probe the X-ray ...
Vladimír Dániel+5 more
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Timing Calibration of the NuSTAR X-Ray Telescope [PDF]
Abstract The Nuclear Spectroscopic Telescope Array (NuSTAR) mission is the first focusing X-ray telescope in the hard X-ray (3–79 keV) band. Among the phenomena that can be studied in this energy band, some require high time resolution and stability: rotation-powered and accreting millisecond pulsars, fast variability from black holes ...
Matteo Bachetti+15 more
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