Reduced-Scale Transition-Edge Sensor Detectors for Solar and X-Ray Astrophysics

We have developed large-format, close-packed X-ray microcalorimeter arrays fabricated on solid substrates, designed to achieve high energy resolution with count rates up to a few hundred counts per second per pixel for X-ray photon energies up to 8 keV. Our most recent arrays feature 31-micron absor...

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Veröffentlicht in:IEEE transactions on applied superconductivity 2017-06, Vol.27 (4), p.1-5
Hauptverfasser: Datesman, Aaron M., Adams, Joseph S., Bandler, Simon R., Betancourt-Martinez, Gabriele L., Meng-Ping Chang, Chervenak, James A., Eckart, Megan E., Ewin, Audrey E., Finkbeiner, Fred M., Jong Yoon Ha, Kelley, Richard L., Kilbourne, Caroline A., Miniussi, Antoine R., Porter, Frederick S., Sadleir, John E., Sakai, Kazuhiro, Smith, Stephen J., Wakeham, Nicholas A., Williams, Elissa H., Wassell, Edward J., Wonsik Yoon
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container_end_page 5
container_issue 4
container_start_page 1
container_title IEEE transactions on applied superconductivity
container_volume 27
creator Datesman, Aaron M.
Adams, Joseph S.
Bandler, Simon R.
Betancourt-Martinez, Gabriele L.
Meng-Ping Chang
Chervenak, James A.
Eckart, Megan E.
Ewin, Audrey E.
Finkbeiner, Fred M.
Jong Yoon Ha
Kelley, Richard L.
Kilbourne, Caroline A.
Miniussi, Antoine R.
Porter, Frederick S.
Sadleir, John E.
Sakai, Kazuhiro
Smith, Stephen J.
Wakeham, Nicholas A.
Williams, Elissa H.
Wassell, Edward J.
Wonsik Yoon
description We have developed large-format, close-packed X-ray microcalorimeter arrays fabricated on solid substrates, designed to achieve high energy resolution with count rates up to a few hundred counts per second per pixel for X-ray photon energies up to 8 keV. Our most recent arrays feature 31-micron absorbers on a 35-micron pitch, reducing the size of pixels by about a factor of two. This change will enable an instrument with significantly higher angular resolution. In order to wire out large format arrays with an increased density of smaller pixels, we have reduced the lateral size of both the microstrip wiring and the Mo/Au transition-edge sensors (TES). We report on the key physical properties of these small TESs and the fine Nb leads attached, including the critical currents and weak-link properties associated with the longitudinal proximity effect.
doi_str_mv 10.1109/TASC.2017.2649839
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recordid cdi_crossref_primary_10_1109_TASC_2017_2649839
source IEEE/IET Electronic Library (IEL)
subjects Arrays
Astrophysics
Detectors
Fabrication
Instrumentation And Photography
Lead
low temperature detectors
microcalor-imeters
Microstrip
Niobium
Superconducting transition temperature
Temperature measurement
transition-edge sensors (TES)
X-ray spectroscopy
title Reduced-Scale Transition-Edge Sensor Detectors for Solar and X-Ray Astrophysics
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