scholarly journals Full field-of-view, high-resolution, photon-counting detector CT: technical assessment and initial patient experience

Author(s):  
Kishore Rajendran ◽  
Martin Petersilka ◽  
Andre Henning ◽  
Elisabeth Shanblatt ◽  
Jeffrey F Marsh Jr ◽  
...  
2021 ◽  
Vol 28 (6) ◽  
Author(s):  
Silvia Cipiccia ◽  
Francesco Brun ◽  
Vittorio Di Trapani ◽  
Christoph Rau ◽  
Darren J. Batey

X-ray ptychography and X-ray fluorescence are complementary nanoscale imaging techniques, providing structural and elemental information, respectively. Both methods acquire data by scanning a localized beam across the sample. X-ray ptychography processes the transmission signal of a coherent illumination interacting with the sample, to produce images with a resolution finer than the illumination spot and step size. By enlarging both the spot and the step size, the technique can cover extended regions efficiently. X-ray fluorescence records the emitted spectra as the sample is scanned through the localized beam and its spatial resolution is limited by the spot and step size. The requisites for fast ptychography and high-resolution fluorescence appear incompatible. Here, a novel scheme that mitigates the difference in requirements is proposed. The method makes use of two probes of different sizes at the sample, generated by using two different energies for the probes and chromatic focusing optics. The different probe sizes allow to reduce the number of acquisition steps for the joint fluorescence–ptychography scan compared with a standard single beam scan, while imaging the same field of view. The new method is demonstrated experimentally using two undulator harmonics, a Fresnel zone plate and an energy discriminating photon counting detector.


1990 ◽  
Vol 139 ◽  
pp. 449-452 ◽  
Author(s):  
M. Lampton ◽  
S. Bowyer ◽  
J. M. Deharveng

The FAUST telescope is an ultraviolet survey instrument that features a wide 8° field of view, ~1′ angular resolution, and a photon counting detector. Operating in the 1400–1800 Å band, it will be sufficiently sensitive to detect blue mv =17 objects in a single 20 minute night. The instrument is part of the ATLAS-1 shuttle mission, presently scheduled for flight in May 1991. A substantial number of high galactic latitude fields will be investigated, with particular emphasis on studies of the origin of the diffuse far UV background.


2018 ◽  
Vol 13 (12) ◽  
pp. C12006-C12006 ◽  
Author(s):  
D. Vavřík ◽  
D. Kytýř ◽  
S. Mühleder ◽  
M. Vopálenský ◽  
P. Beneš ◽  
...  

2016 ◽  
Vol 11 (02) ◽  
pp. C02003-C02003 ◽  
Author(s):  
I. Kumpová ◽  
D. Vavřík ◽  
T. Fíla ◽  
P. Koudelka ◽  
I. Jandejsek ◽  
...  

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