Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray 2022
DOI: 10.1117/12.2629368
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Performance of the SRON Ti/Au transition edge sensor x-ray calorimeters

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Cited by 9 publications
(6 citation statements)
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References 30 publications
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“…These data show that reducing the TES width to 15 μm leads to a further reduction in (dI/dB)/I(0) compared with a width of 30 μm. This is expected; as the effective area of the weak-link is reduced, the current distribution across the TES is altered, and the effect of self-field from the TES current is also reduced 14 , 27 , 36 , 41 , 42 . The reduced sensitivity of the TES current to magnetic field in narrower devices correlates with a reduced gain scale sensitivity of the x-ray pulse height to variations in the magnetic field.…”
Section: Resultsmentioning
confidence: 73%
See 1 more Smart Citation
“…These data show that reducing the TES width to 15 μm leads to a further reduction in (dI/dB)/I(0) compared with a width of 30 μm. This is expected; as the effective area of the weak-link is reduced, the current distribution across the TES is altered, and the effect of self-field from the TES current is also reduced 14 , 27 , 36 , 41 , 42 . The reduced sensitivity of the TES current to magnetic field in narrower devices correlates with a reduced gain scale sensitivity of the x-ray pulse height to variations in the magnetic field.…”
Section: Resultsmentioning
confidence: 73%
“…This is expected; as the effective area of the weak-link is reduced, the current distribution across the TES is altered, and the effect of self-field from the TES current is also reduced. 14,27,36,41,42 The reduced sensitivity of the TES current to magnetic field in narrower devices correlates with a reduced gain scale sensitivity of the x-ray pulse height to variations in the magnetic field. This magnetic field dependence is calculated as the change in the energy gain scale at 1.5 keV δE B , after optimal filtering, divided by the change in magnetic field B.…”
Section: Energy Gain Scale Sensitivitymentioning
confidence: 99%
“…They have also been extensively developed for other applications, such as x-ray and nuclear spectroscopy. To the best of our knowledge, the best demonstrated FWHM energy resolutions are 0.7 eV at 1.5 keV [150] and 1.3-1.6 eV for 5.9 keV x-rays [143,144], 65 eV for 208 keV gamma rays [151] and 1.0-1.1 keV for 5.3 MeV alpha particles [11,152]. These energy resolutions are improved by orders of magnitudes compared to those of comparable commercial semiconductor detectors, such as Si(Li) detectors and high purity Ge detectors for x-rays and gamma rays and passive implanted planar Si detectors for alpha particles.…”
Section: Transition Edge Sensorsmentioning
confidence: 96%
“…In recent years, significant improvements have been achieved in the development of sensor materials and readout technologies, resulting in energy resolutions that are better than those of conventional detectors by orders of magnitude. For example, the highest energy resolutions achieved with superconducting microcalorimeters are a 1.3-1.6 eV FWHM at 6 keV [143][144][145] and a 0.9-1.1 keV FWHM at 5.5 MeV [11,12]. Furthermore, with a carefully chosen absorber and detection scheme, the high resolution phonon measurement technique can be accompanied by measurements in other detection channels, such as ionization and scintillation.…”
Section: Motivationmentioning
confidence: 99%
“…For comparison, Micromegas detectors demonstrated resolving power capabilities ΔE/E of the order of 20% at E = 6 keV, 21 whereas at SRON, we have shown resolving powers for TES micro-calorimeters at a level of 0.03%. 22 A review of the detectors currently considered for IAXO is reported in Ref. 19.…”
Section: Article Scitationorg/journal/rsimentioning
confidence: 99%