2012
DOI: 10.1007/s10909-012-0511-0
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Ultra Low Background Cryogenic Test Facility for Far-Infrared Radiation Detectors

Abstract: The next generation of far infrared radiation detectors is aimed to reach photon noise limited performance in space based observatories such as SPICA and BLISS. These detectors operate at loading powers of the astronomical signal of a few Attowatt (10 −18 W) or less, corresponding to a sensitivity expressed in noise equivalent power as low as NEP = 2 × 10 −20 W/ √ Hz. We have developed a cryogenic test setup for microwave Kinetic Inductance Detectors (MKIDs) that aims to reach these ultra-low background levels… Show more

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Cited by 34 publications
(34 citation statements)
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“…The samples are cooled in a pulse tube pre-cooled adiabatic demagnetization refrigerator. Special care has been taken to make the setup light tight [4,9], presented in detail in an accompanying paper [10]. The complex transmission of the microwave circuit is measured with a quadrature mixer and traces out a circle in the complex plane [1,11].…”
Section: Microwave Resonator Experimentsmentioning
confidence: 99%
“…The samples are cooled in a pulse tube pre-cooled adiabatic demagnetization refrigerator. Special care has been taken to make the setup light tight [4,9], presented in detail in an accompanying paper [10]. The complex transmission of the microwave circuit is measured with a quadrature mixer and traces out a circle in the complex plane [1,11].…”
Section: Microwave Resonator Experimentsmentioning
confidence: 99%
“…Care was taken to make the sample stage light-tight as described in Ref. [19], which is crucial to eliminating excess quasiparticles due to stray light. The complex transmission S 21 of the microwave circuit was measured with a vector network analyzer.…”
mentioning
confidence: 99%
“…The sample is mounted in a sample holder inside a light-tight box, in a box-in-a-box configuration [20]. The 350 GHz radiation illuminating the KIDs is coming from a cryogenic black The KIDs are mounted in a sample box thermally anchored to the base temperature plate of the ADR (∼ 100 mK).…”
mentioning
confidence: 99%