Energy calibration of superconducting transition edge sensors for x-ray detection using pulse analysis

2006 ◽  
Vol 77 (5) ◽  
pp. 053105 ◽  
Author(s):  
C. Hollerith ◽  
B. Simmnacher ◽  
R. Weiland ◽  
F. v. Feilitzsch ◽  
C. Isaila ◽  
...  
2008 ◽  
Vol 24 (1) ◽  
pp. 11-14 ◽  
Author(s):  
Masashi OHNO ◽  
Hiroyuki TAKAHASHI ◽  
R. M. Thushara DAMAYANTHI ◽  
Yasuhiro MINAMIKAWA ◽  
Fumiakira MORI

2015 ◽  
Vol 22 (3) ◽  
pp. 766-775 ◽  
Author(s):  
J. Uhlig ◽  
W. B. Doriese ◽  
J. W. Fowler ◽  
D. S. Swetz ◽  
C. Jaye ◽  
...  

X-ray emission spectroscopy (XES) is a powerful element-selective tool to analyze the oxidation states of atoms in complex compounds, determine their electronic configuration, and identify unknown compounds in challenging environments. Until now the low efficiency of wavelength-dispersive X-ray spectrometer technology has limited the use of XES, especially in combination with weaker laboratory X-ray sources. More efficient energy-dispersive detectors have either insufficient energy resolution because of the statistical limits described by Fano or too low counting rates to be of practical use. This paper updates an approach to high-resolution X-ray emission spectroscopy that uses a microcalorimeter detector array of superconducting transition-edge sensors (TESs). TES arrays are discussed and compared with conventional methods, and shown under which circumstances they are superior. It is also shown that a TES array can be integrated into a table-top time-resolved X-ray source and a soft X-ray synchrotron beamline to perform emission spectroscopy with good chemical sensitivity over a very wide range of energies.


2021 ◽  
Vol 11 (9) ◽  
pp. 3793
Author(s):  
Luciano Gottardi ◽  
Kenichiro Nagayashi

The state-of-the-art technology of X-ray microcalorimeters based on superconducting transition-edge sensors (TESs), for applications in astrophysics and particle physics, is reviewed. We will show the advance in understanding the detector physics and describe the recent breakthroughs in the TES design that are opening the way towards the fabrication and the read-out of very large arrays of pixels with unprecedented energy resolution. The most challenging low temperature instruments for space- and ground-base experiments will be described.


Materials ◽  
2021 ◽  
Vol 14 (23) ◽  
pp. 7169
Author(s):  
Jian Chen ◽  
Jinjin Li ◽  
Xiaolong Xu ◽  
Zhenyu Wang ◽  
Siming Guo ◽  
...  

An absorber with a high absorbing efficiency is crucial for X-ray transition edge sensors (TESs) to realize high quantum efficiency and the best energy resolution. Semimetal Bismuth (Bi) has shown greater superiority than gold (Au) as the absorber due to the low specific heat capacity, which is two orders of magnitude smaller. The electroplating process of Bi films is investigated. The Bi grains show a polycrystalline rhombohedral structure, and the X-ray diffraction (XRD) patterns show a typical crystal orientation of (012). The average grain size becomes larger as the electroplating current density and the thickness increase, and the orientation of Bi grains changes as the temperature increases. The residual resistance ratio (RRR) (R300 K/R4.2 K) is 1.37 for the Bi film (862 nm) deposited with 9 mA/cm2 at 40 °C for 2 min. The absorptivity of the 5 μm thick Bi films is 40.3% and 30.7% for 10 keV and 15.6 keV X-ray radiation respectively, which shows that Bi films are a good candidate as the absorber of X-ray TESs.


2000 ◽  
Author(s):  
Marcel L. van den Berg ◽  
Daniel T. Chow ◽  
Alex Loshak ◽  
Mark F. Cunningham ◽  
Troy W. Barbee, Jr. ◽  
...  

Author(s):  
Stephen J. Smith ◽  
Joseph S. Adams ◽  
Simon R. Bandler ◽  
James A. Chervenak ◽  
Aaron M. Datesman ◽  
...  

2015 ◽  
Vol 184 (1-2) ◽  
pp. 389-395 ◽  
Author(s):  
W. B. Doriese ◽  
K. M. Morgan ◽  
D. A. Bennett ◽  
E. V. Denison ◽  
C. P. Fitzgerald ◽  
...  

2010 ◽  
Vol 104 (4) ◽  
Author(s):  
John E. Sadleir ◽  
Stephen J. Smith ◽  
Simon R. Bandler ◽  
James A. Chervenak ◽  
John R. Clem

2018 ◽  
Vol 124 (14) ◽  
pp. 144501 ◽  
Author(s):  
E. A. Williams ◽  
S. Withington ◽  
C. N. Thomas ◽  
D. J. Goldie ◽  
D. Osman

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