Large Format Antenna Coupled Micorwave Kinetic Iinductance Detector Arrays for Radioastronomy

被引：0

作者：

Baryshev, Andrey M. ^{[1
,2
,3
]}

Baselmans, Jochem J. A. ^{[1
,2
,4
]}

Yates, Stephen J. C. ^{[1
,2
]}

Ferrari, Lorenza ^{[1
,2
]}

Bisigello, Laura ^{[1
,2
,3
]}

Janssen, Reinier M. J. ^{[4
]}

Endo, Akira ^{[4
]}

Klapwijk, Teun M. ^{[4
]}

Klein, Bernd ^{[5
]}

Heyminck, Stefan ^{[5
]}

Guesten, Rolf ^{[5
]}

机构：

[1] Netherlands Inst Space Res SRON, NL-9700 AV Groningen, Netherlands

[2] Netherlands Inst Space Res SRON, NL-9700 AV Utrecht, Netherlands

[3] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Utrecht, Netherlands

[4] Delft Univ Technol, Kavli Inst NanoSci, NL-2628 CJ Delft, Netherlands

[5] Max Planck Inst Radioastron, D-53121 Bonn, Germany

来源：

2014 39TH INTERNATIONAL CONFERENCE ON INFRARED, MILLIMETER, AND TERAHERTZ WAVES (IRMMW-THZ) | 2014年

关键词：

D O I：

暂无

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

The realization of large format fully sampled sensitive focal plane arrays of direct detectors is a long standing development goal for advanced astrophysical instrumentation for submillimeter wavelengths. Recently a superconducting microwave kinetic inductors detector (MKID) technology has been developed which offers high sensitivity and unprecedented multiplexing ratio. We report on development of MKID antenna coupled MKID arrays for 350 m and 850 m atmospheric transmission windows each containing of order of 5000 and 1000 detectors per superconducting chip respectively. We present design and measurement results on first detector chips including pixel responsivity, noise distribution and detector yields.

引用

页数：1

共 28 条

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