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A prototype of digital frequency multiplexing electronics allowing the real time monitoring of kinetic inductance detector (KIDs) arrays for mm-wave astronomy has been developed. It requires only 2 coaxial cables for instrumenting a large…

天体物理仪器与方法 · 物理学 2015-03-18 O. Bourrion , A. Bideaud , A. Benoit , A. Cruciani , J. F. Macias-Perez , A. Monfardini , M. Roesch , L. Swenson , C. Vescovi

Future astrophysics and cosmic microwave background space missions operating in the far-infrared to millimetre part of the spectrum will require very large arrays of ultra-sensitive detectors in combination with high multiplexing factors…

Microwave Kinetic Inductance Detectors (MKIDs) are the most attractive radiation detectors for far-infrared and sub-mm astronomy: They combine ultimate sensitivity with the possibility to create very large detector arrays, in excess of 10…

天体物理仪器与方法 · 物理学 2016-04-04 Joris van Rantwijk , Martin Grim , Dennis van Loon , Stephen Yates , Andrey Baryshev , Jochem Baselmans

Microwave Kinetic Inductance Detectors (MKID) are a promising solution for spaceborne mm-wave astronomy. To optimize their design and make them insensitive to the ballistic phonons created by cosmic-ray interactions in the substrate, the…

天体物理仪器与方法 · 物理学 2013-12-10 O. Bourrion , C. Vescovi , A. Catalano , M. Calvo , A. D'Addabbo , J. Goupy , N. Boudou , J. F. Macias-Perez , A. Monfardini

Microwave Kinetic Inductance Detectors (MKIDs) are superconducting detectors capable of counting single photons and measuring their energy in the UV, optical, and near-IR. MKIDs feature intrinsic frequency domain multiplexing (FDM) at…

天体物理仪器与方法 · 物理学 2013-07-29 Sean McHugh , Benjamin A. Mazin , Bruno Serfass , Seth Meeker , Kieran O'Brien , Ran Duan , Rick Raffanti , Dan Werthimer

This work presents Ti/Al bi-layer Microwave Kinetic Inductance Detectors (MKIDs) based on lens-coupled spiral absorbers as the quasi-optical coupling mechanism for millimeter-wavelength radiation detection. From simulations, the…

The New Iram Kid Arrays-2 (NIKA2) instrument has recently been installed at the IRAM 30 m telescope. NIKA2 is a state-of-art instrument dedicated to mm-wave astronomy using microwave kinetic inductance detectors (KID) as sensors. The three…

Current generation millimeter wavelength detectors suffer from scaling limits imposed by complex cryogenic readout electronics. To circumvent this it is imperative to investigate technologies that intrinsically incorporate strong…

We have fabricated 2024 pixel microwave kinetic inductance detector (MKID) arrays in the ultraviolet/optical/near-IR (UVOIR) regime that are currently in use in astronomical instruments. In order to make MKIDs desirable for novel…

仪器与探测器 · 物理学 2017-11-23 P. Szypryt , B. A. Mazin , B. Bumble , H. G. Leduc , L. Baker

We present a method of spatially mapping microwave kinetic inductance detector (MKID) arrays, in a dark setup. MKIDs are superconducting natively multiplexed resonators which enable kilopixel arrays, such as for the proposed Probe…

Microwave Kinetic Inductance Detector (MKID) arrays are currently being developed and deployed for astronomical applications in the visible and near infrared and for sub-millimetre astronomy. One of the main drawbacks of MKIDs is that large…

天体物理仪器与方法 · 物理学 2022-04-13 Mario De Lucia , Eoin Baldwin , Gerhard Ulbricht , Colm Bracken , Plamen Stamenov , Tom Ray

Future generation of astronomical imaging spectrometers are targeting the far infrared wavelengths to close the THz astronomy gap. Similar to lens antenna coupled Microwave Kinetic Inductance Detectors (MKIDs), lens absorber coupled MKIDs…

In the next decades millimeter and sub-mm astronomy requires large format imaging arrays and broad-band spectrometers to complement the high spatial and spectral resolution of the Atacama Large Millimeter/sub-millimeter Array. The desired…

天体物理仪器与方法 · 物理学 2014-08-15 R. M. J. Janssen , J. J. A. Baselmans , A. Endo , L. Ferrari , S. J. C. Yates , A. M. Baryshev , T. M. Klapwijk

We are developing superconducting Microwave Kinetic Inductance Detectors to operate at near infrared and optical wavelengths for astronomy. In order to efficiently meet with the requirements of astronomical applications, we propose to…

天体物理仪器与方法 · 物理学 2019-01-30 S. Beldi , F. Boussaha , C. Chaumont , S. Mignot , F. Reix , A. Tartari , T. Vacelet , A. Traini , M. Piat , P. Bonifacio

We describe the on-line algorithms developed to probe Lumped Element Kinetic Inductance Detectors (LEKID) in this paper. LEKIDs are millimeter wavelength detectors for astronomy. LEKID arrays are currently operated in different instruments…

For X-ray imaging spectroscopy, high spatial resolution over a large field of view is often as important as high energy resolution, but current X-ray detectors do not provide both in the same device. Thermal Kinetic Inductance Detectors…

天体物理仪器与方法 · 物理学 2015-06-26 Gerhard Ulbricht , Benjamin A. Mazin , Paul Szypryt , Alex B. Walter , Clint Bockstiegel , Bruce Bumble

Microwave Kinetic Inductance Detectors, or MKIDs, have proven to be a powerful cryogenic detector technology due to their sensitivity and the ease with which they can be multiplexed into large arrays. A MKID is an energy sensor based on a…

天体物理仪器与方法 · 物理学 2012-02-03 Benjamin A. Mazin , Bruce Bumble , Seth R. Meeker , Kieran O'Brien , Sean McHugh , Eric Langman

The kinetic inductance detector (KID) is a versatile and scalable detector technology with a wide range of applications. These superconducting detectors offer significant advantages: simple and robust fabrication, intrinsic multiplexing…

仪器与探测器 · 物理学 2022-03-31 Peter S. Barry , Clarence. C. Chang , Sunil Golwala , Erik Shirokoff

We report on the development of scalable prototype microwave kinetic inductance detector (MKID) arrays tailored for future multi-kilo-pixel experiments that are designed to simultaneously characterize the polarization properties of both the…

Microwave kinetic inductance detector (MKID) provides a way to build large ground based sub-mm instruments such as NIKA and A-MKID. For such instruments, therefore, it is important to understand and characterize the response to ensure good…

天体物理仪器与方法 · 物理学 2016-02-15 L. Bisigello , S. J. C. Yates , V. Murugesan , J. J. A. Baselmans , A. M. Baryshev
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