Extended Line Spread Function of TES Microcalorimeters With Au/Bi Absorbers
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Date
2019-03-06
Type of Work
Department
Program
Citation of Original Publication
M. E. Eckart et al., "Extended Line Spread Function of TES Microcalorimeters With Au/Bi Absorbers," in IEEE Transactions on Applied Superconductivity, vol. 29, no. 5, pp. 1-5, Aug. 2019, Art no. 2101205, doi: 10.1109/TASC.2019.2903420.
Rights
This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
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Public Domain Mark 1.0
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Abstract
Microcalorimeters have the potential to provide line
shapes well described by a single Gaussian broadening term of
few-eV width. This attribute makes the detectors especially well
suited for x-ray astrophysics observations; however, low-level non-Gaussian broadening terms are expected and must be characterized. These terms depend on the composition of the x-ray absorber,
the detailed x-ray absorption physics, the device thermalization
processes, and the incident x-ray energy. Here we present the first
measurements targeted at understanding the extended line-spread
function (LSF) of x-ray microcalorimeter pixels under development for the X-ray Integral Field Unit on the Athena X-ray Observatory. These pixels are composed of Mo/Au transition-edge
sensors with overhanging electroplated Au/Bi absorbers. We have
measured the line shapes using monochromatic x-ray sources with
<1-eV width at several x-ray energies (0.85, 0.93, 1.25, 1.5, 5.4,
and 8.0 keV) across the instrument bandpass (0.3–12 keV) and
have modeled the line profiles. These results are compared to the
extended LSF of the Hitomi microcalorimeter pixels that used HgTe
absorbers.