2008
DOI: 10.1117/12.787764
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Modelling and reduction of noise in transition edge sensor detectors

Abstract: Current and future astronomical detectors based on Transition Edge Sensors (TESs) need to achieve theoretically predicted current noise performance determined by the sum of contributions from thermal noise in the link to the heat bath, Johnson noise in the sensor itself and noise in the electrical readout circuit. Present TES geometries can have noise levels significantly above this limit. Our Mo/Cu bilayer TESs are fabricated on long, narrow, thermally isolating silicon nitride structures and are designed for… Show more

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Cited by 4 publications
(2 citation statements)
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References 14 publications
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“…According to (38), the n'th element of the leading diagonal of H corresponds to the total power absorbed when single source n illuminates the sample. The off-diagonal terms describe the fringe when a pair of phase coherent sources n and n ′ are used.…”
Section: B Interferometrymentioning
confidence: 99%
See 1 more Smart Citation
“…According to (38), the n'th element of the leading diagonal of H corresponds to the total power absorbed when single source n illuminates the sample. The off-diagonal terms describe the fringe when a pair of phase coherent sources n and n ′ are used.…”
Section: B Interferometrymentioning
confidence: 99%
“…Our own preferred approach is to attach the SUT to a micromachined SiN membrane, which also supports a thin-film temperature sensor. Such devices have been developed extensively for astronomical detectors, and when used at low temperatures can achieve extreme sensitivity [37,38]. Our detectors [39] can detect absorbed powers of much less than 1 fW with noise levels of 1x10 −19 WHz −1/2 , making extreme thermometry of thin-film structures entirely possible.…”
Section: Practical Considerationsmentioning
confidence: 99%