Multiabsorber transition-edge sensors for x-ray astronomy

Stephen J. Smith; Joseph S. Adams; Simon R. Bandler; James A. Chervenak; Aaron M. Datesman; Megan E. Eckart; Fred M. Finkbeiner; Ruslan Hummatov; Richard L. Kelley; Caroline A. Kilbourne; Antoine R. Miniussi; Frederick S. Porter; John E. Sadleir; Kazuhiro Sakai; Nicholas A. Wakeham; Edward J. Wassell

doi:10.1117/1.JATIS.5.2.021008

8 April 2019 Multiabsorber transition-edge sensors for x-ray astronomy

Stephen J. Smith, Joseph S. Adams, Simon R. Bandler, James A. Chervenak, Aaron M. Datesman, Megan E. Eckart, Fred M. Finkbeiner, Ruslan Hummatov, Richard L. Kelley, Caroline A. Kilbourne, Antoine R. Miniussi, Frederick S. Porter, John E. Sadleir, Kazuhiro Sakai, Nicholas A. Wakeham, Edward J. Wassell

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Journal of Astronomical Telescopes, Instruments, and Systems, Vol. 5, Issue 2, 021008 (April 2019). https://doi.org/10.1117/1.JATIS.5.2.021008

Abstract

We are developing arrays of position-sensitive microcalorimeters for future x-ray astronomy applications. These position-sensitive devices commonly referred to as hydras consist of multiple x-ray absorbers, each with a different thermal coupling to a single-transition-edge sensor microcalorimeter. Their development is motivated by a desire to achieve very large pixel arrays with some modest compromise in performance. We report on the design, optimization, and first results from devices with small pitch pixels (<75 μm) being developed for a high-angular and energy resolution imaging spectrometer for Lynx. The Lynx x-ray space telescope is a flagship mission concept under study for the National Academy of Science 2020 decadal survey. Broadband full-width-half-maximum (FWHM) resolution measurements on a 9-pixel hydra have demonstrated ΔE_FWHM = 2.23 ± 0.14 eV at Al-K_α, ΔE_FWHM = 2.44 ± 0.29 eV at Mn-K_α, and ΔE_FWHM = 3.39 ± 0.23 eV at Cu-K_α. Position discrimination is demonstrated to energies below <1 keV and the device performance is well-described by a finite-element model. Results from a prototype 20-pixel hydra with absorbers on a 50-μm pitch have shown ΔE_FWHM = 3.38 ± 0.20 eV at Cr-K_α1. We are now optimizing designs specifically for Lynx and extending the number of absorbers up to 25/hydra. Numerical simulation suggests optimized designs could achieve ∼3 eV while being compatible with the bandwidth requirements of the state-of-the art multiplexed readout schemes, thus making a 100,000 pixel microcalorimeter instrument a realistic goal.

CC BY: © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.

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Stephen J. Smith, Joseph S. Adams, Simon R. Bandler, James A. Chervenak, Aaron M. Datesman, Megan E. Eckart, Fred M. Finkbeiner, Ruslan Hummatov, Richard L. Kelley, Caroline A. Kilbourne, Antoine R. Miniussi, Frederick S. Porter, John E. Sadleir, Kazuhiro Sakai, Nicholas A. Wakeham, and Edward J. Wassell "Multiabsorber transition-edge sensors for x-ray astronomy," Journal of Astronomical Telescopes, Instruments, and Systems 5(2), 021008 (8 April 2019). https://doi.org/10.1117/1.JATIS.5.2.021008

Received: 1 November 2018; Accepted: 18 March 2019; Published: 8 April 2019

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