THz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy

We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, carried out in recent years, aimed at developing receivers with quantum sensitivity for implementation in space and ground-based radio telescopes. Superconductor-Insulator-Superconductor (SIS) mixers...

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Autores principales: Kirill I. Rudakov, Andrey V. Khudchenko, Lyudmila V. Filippenko, Maxim E. Paramonov, Ronald Hesper, Daniele Aragão Ronsó da Costa Lima, Andrey M. Baryshev, Valery P. Koshelets
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Publicado: MDPI AG 2021
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Acceso en línea:https://doaj.org/article/929b45b4af0342a5ab29ab5d3d05682b
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spelling oai:doaj.org-article:929b45b4af0342a5ab29ab5d3d05682b2021-11-11T15:09:19ZTHz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy10.3390/app1121100872076-3417https://doaj.org/article/929b45b4af0342a5ab29ab5d3d05682b2021-10-01T00:00:00Zhttps://www.mdpi.com/2076-3417/11/21/10087https://doaj.org/toc/2076-3417We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, carried out in recent years, aimed at developing receivers with quantum sensitivity for implementation in space and ground-based radio telescopes. Superconductor-Insulator-Superconductor (SIS) mixers based on high-quality tunnel junctions are the key elements of the most sensitive sub-THz heterodyne receivers. Motivations and physical background for technology improvement and optimization, as well as fabrication details, are described. This article presents the results of the SIS receiver developments for the 211–275 GHz and 790–950 GHz frequency ranges with a noise temperature in the double sideband (DSB) mode of approximTELY 20 K and 200 K, respectively. These designs and achievements are implemented in the development of the receiving systems for the Russian Space Agency mission “Millimetron”, and for the ground-based APEX (Atacama Pathfinder EXperiment) telescope.Kirill I. RudakovAndrey V. KhudchenkoLyudmila V. FilippenkoMaxim E. ParamonovRonald HesperDaniele Aragão Ronsó da Costa LimaAndrey M. BaryshevValery P. KosheletsMDPI AGarticleradio astronomyniobium-based high-quality tunnel junctionslow-noise SIS receiversTHz range quantum-limited mixersTechnologyTEngineering (General). Civil engineering (General)TA1-2040Biology (General)QH301-705.5PhysicsQC1-999ChemistryQD1-999ENApplied Sciences, Vol 11, Iss 10087, p 10087 (2021)
institution DOAJ
collection DOAJ
language EN
topic radio astronomy
niobium-based high-quality tunnel junctions
low-noise SIS receivers
THz range quantum-limited mixers
Technology
T
Engineering (General). Civil engineering (General)
TA1-2040
Biology (General)
QH301-705.5
Physics
QC1-999
Chemistry
QD1-999
spellingShingle radio astronomy
niobium-based high-quality tunnel junctions
low-noise SIS receivers
THz range quantum-limited mixers
Technology
T
Engineering (General). Civil engineering (General)
TA1-2040
Biology (General)
QH301-705.5
Physics
QC1-999
Chemistry
QD1-999
Kirill I. Rudakov
Andrey V. Khudchenko
Lyudmila V. Filippenko
Maxim E. Paramonov
Ronald Hesper
Daniele Aragão Ronsó da Costa Lima
Andrey M. Baryshev
Valery P. Koshelets
THz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy
description We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, carried out in recent years, aimed at developing receivers with quantum sensitivity for implementation in space and ground-based radio telescopes. Superconductor-Insulator-Superconductor (SIS) mixers based on high-quality tunnel junctions are the key elements of the most sensitive sub-THz heterodyne receivers. Motivations and physical background for technology improvement and optimization, as well as fabrication details, are described. This article presents the results of the SIS receiver developments for the 211–275 GHz and 790–950 GHz frequency ranges with a noise temperature in the double sideband (DSB) mode of approximTELY 20 K and 200 K, respectively. These designs and achievements are implemented in the development of the receiving systems for the Russian Space Agency mission “Millimetron”, and for the ground-based APEX (Atacama Pathfinder EXperiment) telescope.
format article
author Kirill I. Rudakov
Andrey V. Khudchenko
Lyudmila V. Filippenko
Maxim E. Paramonov
Ronald Hesper
Daniele Aragão Ronsó da Costa Lima
Andrey M. Baryshev
Valery P. Koshelets
author_facet Kirill I. Rudakov
Andrey V. Khudchenko
Lyudmila V. Filippenko
Maxim E. Paramonov
Ronald Hesper
Daniele Aragão Ronsó da Costa Lima
Andrey M. Baryshev
Valery P. Koshelets
author_sort Kirill I. Rudakov
title THz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy
title_short THz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy
title_full THz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy
title_fullStr THz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy
title_full_unstemmed THz Range Low-Noise SIS Receivers for Space and Ground-Based Radio Astronomy
title_sort thz range low-noise sis receivers for space and ground-based radio astronomy
publisher MDPI AG
publishDate 2021
url https://doaj.org/article/929b45b4af0342a5ab29ab5d3d05682b
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