High resolution 3D fluorescence tomography using ballistic photons

2015 ◽  
Author(s):  
Jie Zheng ◽  
Farouk Nouizi ◽  
Jaedu Cho ◽  
Jessica Kwong ◽  
Gultekin Gulsen
2014 ◽  
Vol 39 (9) ◽  
pp. 2790 ◽  
Author(s):  
Hans M. Hertz ◽  
Jakob C. Larsson ◽  
Ulf Lundström ◽  
Daniel H. Larsson ◽  
Carmen Vogt

2018 ◽  
Vol 24 (S2) ◽  
pp. 84-85
Author(s):  
Jakob C. Larsson ◽  
Carmen Vogt ◽  
William Vagberg ◽  
Muhammet S. Toprak ◽  
Johanna Dzieran ◽  
...  

SPIE Newsroom ◽  
2012 ◽  
Author(s):  
Gultekin Gulsen ◽  
Yuting Lin ◽  
Tiffany C. Kwong ◽  
Uma Sampathkumaran ◽  
Shaaz Ahmed

2015 ◽  
Vol 40 (21) ◽  
pp. 4991 ◽  
Author(s):  
Farouk Nouizi ◽  
Tiffany C. Kwong ◽  
Jaedu Cho ◽  
Yuting Lin ◽  
Uma Sampathkumaran ◽  
...  

2014 ◽  
Vol 21 (5) ◽  
pp. 1031-1047 ◽  
Author(s):  
Martin D. de Jonge ◽  
Christopher G. Ryan ◽  
Chris J. Jacobsen

X-ray nanoprobes require coherent illumination to achieve optic-limited resolution, and so will benefit directly from diffraction-limited storage rings. Here, the example of high-resolution X-ray fluorescence tomography is focused on as one of the most voracious demanders of coherent photons, since the detected signal is only a small fraction of the incident flux. Alternative schemes are considered for beam delivery, sample scanning and detectors. One must consider as well the steps before and after the X-ray experiment: sample preparation and examination conditions, and analysis complexity due to minimum dose requirements and self-absorption. By understanding the requirements and opportunities for nanoscale fluorescence tomography, one gains insight into the R&D challenges in optics and instrumentation needed to fully exploit the source advances that diffraction-limited storage rings offer.


1967 ◽  
Vol 31 ◽  
pp. 45-46
Author(s):  
Carl Heiles

High-resolution 21-cm line observations in a region aroundlII= 120°,b11= +15°, have revealed four types of structure in the interstellar hydrogen: a smooth background, large sheets of density 2 atoms cm-3, clouds occurring mostly in groups, and ‘Cloudlets’ of a few solar masses and a few parsecs in size; the velocity dispersion in the Cloudlets is only 1 km/sec. Strong temperature variations in the gas are in evidence.


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