TY - JOUR
T1 - Non-linear effects in transition edge sensors for X-ray detection
AU - Bandler, S. R.
AU - Figueroa-Feliciano, E.
AU - Iyomoto, Naoko
AU - Kelley, R. L.
AU - Kilbourne, C. A.
AU - Murphy, K. D.
AU - Porter, F. S.
AU - Saab, T.
AU - Sadleir, J.
PY - 2006/4/14
Y1 - 2006/4/14
N2 - In a microcalorimeter that uses a transition-edge sensor to detect energy depositions, the small signal energy resolution improves with decreasing heat capacity. This improvement remains true up to the point where non-linear and saturation effects become significant. This happens when the energy deposition causes a significant change in the sensor resistance. Not only does the signal size become a non-linear function of the energy deposited, but also the noise becomes non-stationary over the duration of the pulse. Algorithms have been developed that can calculate the optimal performance given this non-linear behavior that typically requires significant processing and calibration work-both of which are impractical for space missions. We have investigated the relative importance of the various non-linear effects, with the hope that a computationally simple transformation can overcome the largest of the non-linear and non-stationary effects, producing a highly linear "gain" for pulse-height versus energy, and close to the best energy resolution at all energies when using a Wiener filter.
AB - In a microcalorimeter that uses a transition-edge sensor to detect energy depositions, the small signal energy resolution improves with decreasing heat capacity. This improvement remains true up to the point where non-linear and saturation effects become significant. This happens when the energy deposition causes a significant change in the sensor resistance. Not only does the signal size become a non-linear function of the energy deposited, but also the noise becomes non-stationary over the duration of the pulse. Algorithms have been developed that can calculate the optimal performance given this non-linear behavior that typically requires significant processing and calibration work-both of which are impractical for space missions. We have investigated the relative importance of the various non-linear effects, with the hope that a computationally simple transformation can overcome the largest of the non-linear and non-stationary effects, producing a highly linear "gain" for pulse-height versus energy, and close to the best energy resolution at all energies when using a Wiener filter.
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U2 - 10.1016/j.nima.2005.12.149
DO - 10.1016/j.nima.2005.12.149
M3 - Article
AN - SCOPUS:33645887234
SN - 0168-9002
VL - 559
SP - 817
EP - 819
JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
IS - 2
ER -