Results 11 to 20 of about 1,428 (186)
The Swift Gamma-Ray Explorer is designed to make prompt multiwavelength observations of Gamma-Ray Bursts (GRBs) and GRB afterglows. The X-ray Telescope (XRT) enables Swift to determine GRB positions with a few arcseconds accuracy within 100 seconds of the burst onset.
Burrows, D. N. +23 more
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VTXO: the virtual telescope for x-ray observations [PDF]
5 pages, 4 figures, submitted to the Proceedings of the 34th Annual Small Satellite Conference (SmallSat 2020)
Krizmanic, John +14 more
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The X-Ray Telescope onboard Suzaku [PDF]
Abstract We present the design parameters, production process, and in-flight performance of the X-ray telescope (XRT) onboard Suzaku. The imaging capability is significantly improved over the ASCA XRT, which had half-power diameters of ${3\rlap {.}{}^{\mathrm {\prime }}6}$, to ${1\rlap {.}{}^{\mathrm {\prime }}8}$–${2\rlap {.}{}^{\mathrm
Serlemitsos, P. +33 more
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The X-Ray Telescope of the CAST Experiment [PDF]
5 pages, 9 ...
Kotthaus, R. +7 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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19 pages, 25 figures and images, replaced by the revised version accepted for publication in New Journal of ...
Kuster, M. +25 more
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Diffractive X-Ray Telescopes [PDF]
Diffractive X-ray telescopes using zone plates, phase Fresnel lenses, or related optical elements have the potential to provide astronomers with true imaging capability with resolution several orders of magnitude better than available in any other waveband.
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A Focusing X-Ray Telescope Monochromator [PDF]
In order to resolve clusters of X-ray lines emitted by flares (Fritz et al, 1967; Neupert and Swartz, 1970) and to determine line shapes, a considerable resolving power is needed. The angular size of flares, typically about 2’ will not allow the necessary resolution to be obtained without a very fine slit system combined with the flat crystal X-ray ...
Aaron S. Filler, Benjamin S. Fraenkel
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Virtual Telescope for X-Ray Observations
Selected by NASA for an Astrophysics Science SmallSat study, The Virtual Telescope for X-Ray Observations (VTXO) is a small satellite mission being developed by NASAs Goddard Space Flight Center (GSFC) and New Mexico State University (NMSU). VTXO will perform X-ray observations with an angular resolution around 50 milliarcseconds, an order of magnitude
Rankin, Kyle +4 more
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The Spectrometer/Telescope for Imaging X-rays (STIX) [PDF]
Aims. The Spectrometer Telescope for Imaging X-rays (STIX) on Solar Orbiter is a hard X-ray imaging spectrometer, which covers the energy range from 4 to 150 keV. STIX observes hard X-ray bremsstrahlung emissions from solar flares and therefore provides diagnostics of the hottest (⪆10 MK) flare plasma while ...
Krucker, Säm +88 more
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