Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X

Caroline A. Kilbourne, W. Bertrand Doriese, Simon R. Bandler, Regis P. Brekosky, Ari David Brown, James A. Chervenak, Megan E. Eckart, Fred M. Finkbeiner, Gene C. Hilton, Kent D. Irwin, Naoko Iyomoto, Richard L. Kelley, F. Scott Porter, Carl D. Reintsema, Stephen J. Smith, Joel N. Ullom

Research output: Chapter in Book/Report/Conference proceedingConference contribution

37 Citations (Scopus)

Abstract

Following our development of a superconducting transition-edge-sensor (TES) microcalorimeter design that enables reproducible, high performance (routinely better than 3 eV FWHM energy resolution at 6 keV) and is compatible with high-fill-factor arrays, we have directed our efforts towards demonstrating arrays of identical pixels using the multiplexed read-out concept needed for instrumenting the Constellation-X X-ray Microcalorimeter Spectrometer (XMS) focal plane array. We have used a state-of-the-art, time-division SQUID multiplexer system to demonstrate 2×8 multiplexing (16 pixels read out with two signal channels) with an acceptably modest level of degradation in the energy resolution. The average resolution for the 16 multiplexed pixels was 2.9 eV, and the distribution of resolution values had a relative standard deviation of 5%. The performance of the array while multiplexed is well understood. The technical path to realizing multiplexing for the XMS instrument on the scale of 32 pixels per signal channel includes increasing the system bandwidth by a factor of four and reducing the non-multiplexed SQUID noise by a factor of two. In this paper we discuss the characteristics of a uniform 8×8 array and its performance when read out nonmultiplexed and with various degrees of multiplexing. We present data acquired through the readout chain from the multiplexer electronics, through the real-time demultiplexer software, to storage for later signal processing. We also report on a demonstration of real-time data processing. Finally, because the multiplexer provides unprecedented simultaneous access to the pixels of the array, we were able to measure the array-scale uniformity of TES calorimeter parameters such as the individual thermal conductances and superconducting transition temperatures of the pixels. Detector uniformity is essential for optimal operation of a multiplexed array, and we found that the distributions of thermal conductances, transition temperatures, and transition slopes were sufficiently tight to avoid significant compromises in the operation of any pixel.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation 2008
Subtitle of host publicationUltraviolet to Gamma Ray
Volume7011
DOIs
Publication statusPublished - Dec 1 2008
Externally publishedYes
EventSpace Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray - Marseille, France
Duration: Jun 23 2008Jun 28 2008

Other

OtherSpace Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray
CountryFrance
CityMarseille
Period6/23/086/28/08

Fingerprint

Constellation-X
calorimeters
readout
Pixels
pixels
Pixel
X rays
Sensor
sensors
Sensors
multiplexing
Multiplexing
x rays
X ray spectrometers
SQUID
SQUIDs
Superconducting transition temperature
Conductance
Spectrometer
Uniformity

All Science Journal Classification (ASJC) codes

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Cite this

Kilbourne, C. A., Doriese, W. B., Bandler, S. R., Brekosky, R. P., Brown, A. D., Chervenak, J. A., ... Ullom, J. N. (2008). Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X. In Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray (Vol. 7011). [701104] https://doi.org/10.1117/12.790027

Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X. / Kilbourne, Caroline A.; Doriese, W. Bertrand; Bandler, Simon R.; Brekosky, Regis P.; Brown, Ari David; Chervenak, James A.; Eckart, Megan E.; Finkbeiner, Fred M.; Hilton, Gene C.; Irwin, Kent D.; Iyomoto, Naoko; Kelley, Richard L.; Porter, F. Scott; Reintsema, Carl D.; Smith, Stephen J.; Ullom, Joel N.

Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. Vol. 7011 2008. 701104.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Kilbourne, CA, Doriese, WB, Bandler, SR, Brekosky, RP, Brown, AD, Chervenak, JA, Eckart, ME, Finkbeiner, FM, Hilton, GC, Irwin, KD, Iyomoto, N, Kelley, RL, Porter, FS, Reintsema, CD, Smith, SJ & Ullom, JN 2008, Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X. in Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. vol. 7011, 701104, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, Marseille, France, 6/23/08. https://doi.org/10.1117/12.790027
Kilbourne CA, Doriese WB, Bandler SR, Brekosky RP, Brown AD, Chervenak JA et al. Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X. In Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. Vol. 7011. 2008. 701104 https://doi.org/10.1117/12.790027
Kilbourne, Caroline A. ; Doriese, W. Bertrand ; Bandler, Simon R. ; Brekosky, Regis P. ; Brown, Ari David ; Chervenak, James A. ; Eckart, Megan E. ; Finkbeiner, Fred M. ; Hilton, Gene C. ; Irwin, Kent D. ; Iyomoto, Naoko ; Kelley, Richard L. ; Porter, F. Scott ; Reintsema, Carl D. ; Smith, Stephen J. ; Ullom, Joel N. / Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X. Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. Vol. 7011 2008.
@inproceedings{516dbdfa06bb486f94729a6375dbaf19,
title = "Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X",
abstract = "Following our development of a superconducting transition-edge-sensor (TES) microcalorimeter design that enables reproducible, high performance (routinely better than 3 eV FWHM energy resolution at 6 keV) and is compatible with high-fill-factor arrays, we have directed our efforts towards demonstrating arrays of identical pixels using the multiplexed read-out concept needed for instrumenting the Constellation-X X-ray Microcalorimeter Spectrometer (XMS) focal plane array. We have used a state-of-the-art, time-division SQUID multiplexer system to demonstrate 2×8 multiplexing (16 pixels read out with two signal channels) with an acceptably modest level of degradation in the energy resolution. The average resolution for the 16 multiplexed pixels was 2.9 eV, and the distribution of resolution values had a relative standard deviation of 5{\%}. The performance of the array while multiplexed is well understood. The technical path to realizing multiplexing for the XMS instrument on the scale of 32 pixels per signal channel includes increasing the system bandwidth by a factor of four and reducing the non-multiplexed SQUID noise by a factor of two. In this paper we discuss the characteristics of a uniform 8×8 array and its performance when read out nonmultiplexed and with various degrees of multiplexing. We present data acquired through the readout chain from the multiplexer electronics, through the real-time demultiplexer software, to storage for later signal processing. We also report on a demonstration of real-time data processing. Finally, because the multiplexer provides unprecedented simultaneous access to the pixels of the array, we were able to measure the array-scale uniformity of TES calorimeter parameters such as the individual thermal conductances and superconducting transition temperatures of the pixels. Detector uniformity is essential for optimal operation of a multiplexed array, and we found that the distributions of thermal conductances, transition temperatures, and transition slopes were sufficiently tight to avoid significant compromises in the operation of any pixel.",
author = "Kilbourne, {Caroline A.} and Doriese, {W. Bertrand} and Bandler, {Simon R.} and Brekosky, {Regis P.} and Brown, {Ari David} and Chervenak, {James A.} and Eckart, {Megan E.} and Finkbeiner, {Fred M.} and Hilton, {Gene C.} and Irwin, {Kent D.} and Naoko Iyomoto and Kelley, {Richard L.} and Porter, {F. Scott} and Reintsema, {Carl D.} and Smith, {Stephen J.} and Ullom, {Joel N.}",
year = "2008",
month = "12",
day = "1",
doi = "10.1117/12.790027",
language = "English",
isbn = "9780819472212",
volume = "7011",
booktitle = "Space Telescopes and Instrumentation 2008",

}

TY - GEN

T1 - Multiplexed readout of uniform arrays of TES X-ray microcalorimeters suitable for Constellation-X

AU - Kilbourne, Caroline A.

AU - Doriese, W. Bertrand

AU - Bandler, Simon R.

AU - Brekosky, Regis P.

AU - Brown, Ari David

AU - Chervenak, James A.

AU - Eckart, Megan E.

AU - Finkbeiner, Fred M.

AU - Hilton, Gene C.

AU - Irwin, Kent D.

AU - Iyomoto, Naoko

AU - Kelley, Richard L.

AU - Porter, F. Scott

AU - Reintsema, Carl D.

AU - Smith, Stephen J.

AU - Ullom, Joel N.

PY - 2008/12/1

Y1 - 2008/12/1

N2 - Following our development of a superconducting transition-edge-sensor (TES) microcalorimeter design that enables reproducible, high performance (routinely better than 3 eV FWHM energy resolution at 6 keV) and is compatible with high-fill-factor arrays, we have directed our efforts towards demonstrating arrays of identical pixels using the multiplexed read-out concept needed for instrumenting the Constellation-X X-ray Microcalorimeter Spectrometer (XMS) focal plane array. We have used a state-of-the-art, time-division SQUID multiplexer system to demonstrate 2×8 multiplexing (16 pixels read out with two signal channels) with an acceptably modest level of degradation in the energy resolution. The average resolution for the 16 multiplexed pixels was 2.9 eV, and the distribution of resolution values had a relative standard deviation of 5%. The performance of the array while multiplexed is well understood. The technical path to realizing multiplexing for the XMS instrument on the scale of 32 pixels per signal channel includes increasing the system bandwidth by a factor of four and reducing the non-multiplexed SQUID noise by a factor of two. In this paper we discuss the characteristics of a uniform 8×8 array and its performance when read out nonmultiplexed and with various degrees of multiplexing. We present data acquired through the readout chain from the multiplexer electronics, through the real-time demultiplexer software, to storage for later signal processing. We also report on a demonstration of real-time data processing. Finally, because the multiplexer provides unprecedented simultaneous access to the pixels of the array, we were able to measure the array-scale uniformity of TES calorimeter parameters such as the individual thermal conductances and superconducting transition temperatures of the pixels. Detector uniformity is essential for optimal operation of a multiplexed array, and we found that the distributions of thermal conductances, transition temperatures, and transition slopes were sufficiently tight to avoid significant compromises in the operation of any pixel.

AB - Following our development of a superconducting transition-edge-sensor (TES) microcalorimeter design that enables reproducible, high performance (routinely better than 3 eV FWHM energy resolution at 6 keV) and is compatible with high-fill-factor arrays, we have directed our efforts towards demonstrating arrays of identical pixels using the multiplexed read-out concept needed for instrumenting the Constellation-X X-ray Microcalorimeter Spectrometer (XMS) focal plane array. We have used a state-of-the-art, time-division SQUID multiplexer system to demonstrate 2×8 multiplexing (16 pixels read out with two signal channels) with an acceptably modest level of degradation in the energy resolution. The average resolution for the 16 multiplexed pixels was 2.9 eV, and the distribution of resolution values had a relative standard deviation of 5%. The performance of the array while multiplexed is well understood. The technical path to realizing multiplexing for the XMS instrument on the scale of 32 pixels per signal channel includes increasing the system bandwidth by a factor of four and reducing the non-multiplexed SQUID noise by a factor of two. In this paper we discuss the characteristics of a uniform 8×8 array and its performance when read out nonmultiplexed and with various degrees of multiplexing. We present data acquired through the readout chain from the multiplexer electronics, through the real-time demultiplexer software, to storage for later signal processing. We also report on a demonstration of real-time data processing. Finally, because the multiplexer provides unprecedented simultaneous access to the pixels of the array, we were able to measure the array-scale uniformity of TES calorimeter parameters such as the individual thermal conductances and superconducting transition temperatures of the pixels. Detector uniformity is essential for optimal operation of a multiplexed array, and we found that the distributions of thermal conductances, transition temperatures, and transition slopes were sufficiently tight to avoid significant compromises in the operation of any pixel.

UR - http://www.scopus.com/inward/record.url?scp=67650421136&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=67650421136&partnerID=8YFLogxK

U2 - 10.1117/12.790027

DO - 10.1117/12.790027

M3 - Conference contribution

AN - SCOPUS:67650421136

SN - 9780819472212

VL - 7011

BT - Space Telescopes and Instrumentation 2008

ER -