Development of Mixers for the High Resolution Spectrometer of the Millimetron Space Observatory

I. V. Tretyakov; A. V. Khudchenko; K. I. Rudakov; I. V. Ivashentseva; N. S. Kaurova; B. M. Voronov; M. S. Kirsanova; T. I. Larchenkova; G. N. Goltsman; A. M. Baryshev; R. Hesper; F. V. Khan; E. S. Zhukova; A. M. Chekushkin; A. V. Melentev; K. V. Zhivetev; A. V. Terentiev; V. P. Koshelets; S. F. Likhachev

doi:10.1109/TTHZ.2024.3505592

Development of Mixers for the High Resolution Spectrometer of the Millimetron Space Observatory

I. V. Tretyakov^*, A. V. Khudchenko, K. I. Rudakov, I. V. Ivashentseva, N. S. Kaurova, B. M. Voronov, M. S. Kirsanova, T. I. Larchenkova, G. N. Goltsman, A. M. Baryshev, R. Hesper, F. V. Khan, E. S. Zhukova, A. M. Chekushkin, A. V. Melentev, K. V. Zhivetev, A. V. Terentiev, V. P. Koshelets, S. F. Likhachev

^*Corresponding author for this work

Astronomy

Research output: Contribution to journal › Article › Academic › peer-review

2 Downloads (Pure)

Abstract

The study of the origin and transport of water in the universe is an important part of the scientific program of the Millimetron space observatory. This will be made possible by observations conducted in single-dish mode using an onboard instrument - the High Resolution Spectrometer (HRS). This instrument incorporates heterodyne array receivers operating within the range 0.5 -2.7THz, comprising 3-pixel arrays of superconductor-insulator-superconductor (SIS) mixers operating at frequencies below 1.3 THz and 7-pixel matrix receivers based on NbN HEB mixers observing above 1.3 THz. This paper presents the current status of development for a mixers planned for use in the HRS instrument of the Millimetron space observatory.

Original language	English
Pages (from-to)	191-199
Number of pages	9
Journal	Ieee transactions on terahertz science and technology
Volume	15
Issue number	2
DOIs	https://doi.org/10.1109/TTHZ.2024.3505592
Publication status	Published - 25-Nov-2024

Keywords

Heterodyne receiver
matrix of detectors
NbN thin film
THz range

Access to Document

10.1109/TTHZ.2024.3505592

Development of Mixers for the High-Resolution Spectrometer of the Millimetron Space ObservatoryFinal publisher's version, 2.97 MBLicence: Taverne

Handle.net

Persistent link

Cite this

Tretyakov, I. V., Khudchenko, A. V., Rudakov, K. I., Ivashentseva, I. V., Kaurova, N. S., Voronov, B. M., Kirsanova, M. S., Larchenkova, T. I., Goltsman, G. N., Baryshev, A. M., Hesper, R., Khan, F. V., Zhukova, E. S., Chekushkin, A. M., Melentev, A. V., Zhivetev, K. V., Terentiev, A. V., Koshelets, V. P., & Likhachev, S. F. (2024). Development of Mixers for the High Resolution Spectrometer of the Millimetron Space Observatory. Ieee transactions on terahertz science and technology, 15(2), 191-199. https://doi.org/10.1109/TTHZ.2024.3505592

@article{51aa70c44c1d42f7841cba7e8e0d1e13,

title = "Development of Mixers for the High Resolution Spectrometer of the Millimetron Space Observatory",

abstract = "The study of the origin and transport of water in the universe is an important part of the scientific program of the Millimetron space observatory. This will be made possible by observations conducted in single-dish mode using an onboard instrument - the High Resolution Spectrometer (HRS). This instrument incorporates heterodyne array receivers operating within the range 0.5 -2.7THz, comprising 3-pixel arrays of superconductor-insulator-superconductor (SIS) mixers operating at frequencies below 1.3 THz and 7-pixel matrix receivers based on NbN HEB mixers observing above 1.3 THz. This paper presents the current status of development for a mixers planned for use in the HRS instrument of the Millimetron space observatory.",

keywords = "Heterodyne receiver, matrix of detectors, NbN thin film, THz range",

author = "Tretyakov, {I. V.} and Khudchenko, {A. V.} and Rudakov, {K. I.} and Ivashentseva, {I. V.} and Kaurova, {N. S.} and Voronov, {B. M.} and Kirsanova, {M. S.} and Larchenkova, {T. I.} and Goltsman, {G. N.} and Baryshev, {A. M.} and R. Hesper and Khan, {F. V.} and Zhukova, {E. S.} and Chekushkin, {A. M.} and Melentev, {A. V.} and Zhivetev, {K. V.} and Terentiev, {A. V.} and Koshelets, {V. P.} and Likhachev, {S. F.}",

note = "Publisher Copyright: {\textcopyright} 2011-2012 IEEE.",

year = "2024",

month = nov,

day = "25",

doi = "10.1109/TTHZ.2024.3505592",

language = "English",

volume = "15",

pages = "191--199",

journal = "Ieee transactions on terahertz science and technology",

issn = "2156-342X",

publisher = "IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC",

number = "2",

}

Tretyakov, IV, Khudchenko, AV, Rudakov, KI, Ivashentseva, IV, Kaurova, NS, Voronov, BM, Kirsanova, MS, Larchenkova, TI, Goltsman, GN, Baryshev, AM , Hesper, R, Khan, FV, Zhukova, ES, Chekushkin, AM, Melentev, AV, Zhivetev, KV, Terentiev, AV, Koshelets, VP & Likhachev, SF 2024, 'Development of Mixers for the High Resolution Spectrometer of the Millimetron Space Observatory', Ieee transactions on terahertz science and technology, vol. 15, no. 2, pp. 191-199. https://doi.org/10.1109/TTHZ.2024.3505592

TY - JOUR

T1 - Development of Mixers for the High Resolution Spectrometer of the Millimetron Space Observatory

AU - Tretyakov, I. V.

AU - Khudchenko, A. V.

AU - Rudakov, K. I.

AU - Ivashentseva, I. V.

AU - Kaurova, N. S.

AU - Voronov, B. M.

AU - Kirsanova, M. S.

AU - Larchenkova, T. I.

AU - Goltsman, G. N.

AU - Baryshev, A. M.

AU - Hesper, R.

AU - Khan, F. V.

AU - Zhukova, E. S.

AU - Chekushkin, A. M.

AU - Melentev, A. V.

AU - Zhivetev, K. V.

AU - Terentiev, A. V.

AU - Koshelets, V. P.

AU - Likhachev, S. F.

PY - 2024/11/25

Y1 - 2024/11/25

N2 - The study of the origin and transport of water in the universe is an important part of the scientific program of the Millimetron space observatory. This will be made possible by observations conducted in single-dish mode using an onboard instrument - the High Resolution Spectrometer (HRS). This instrument incorporates heterodyne array receivers operating within the range 0.5 -2.7THz, comprising 3-pixel arrays of superconductor-insulator-superconductor (SIS) mixers operating at frequencies below 1.3 THz and 7-pixel matrix receivers based on NbN HEB mixers observing above 1.3 THz. This paper presents the current status of development for a mixers planned for use in the HRS instrument of the Millimetron space observatory.

AB - The study of the origin and transport of water in the universe is an important part of the scientific program of the Millimetron space observatory. This will be made possible by observations conducted in single-dish mode using an onboard instrument - the High Resolution Spectrometer (HRS). This instrument incorporates heterodyne array receivers operating within the range 0.5 -2.7THz, comprising 3-pixel arrays of superconductor-insulator-superconductor (SIS) mixers operating at frequencies below 1.3 THz and 7-pixel matrix receivers based on NbN HEB mixers observing above 1.3 THz. This paper presents the current status of development for a mixers planned for use in the HRS instrument of the Millimetron space observatory.

KW - Heterodyne receiver

KW - matrix of detectors

KW - NbN thin film

KW - THz range

UR - http://www.scopus.com/inward/record.url?scp=85210924571&partnerID=8YFLogxK

U2 - 10.1109/TTHZ.2024.3505592

DO - 10.1109/TTHZ.2024.3505592

M3 - Article

AN - SCOPUS:85210924571

SN - 2156-342X

VL - 15

SP - 191

EP - 199

JO - Ieee transactions on terahertz science and technology

JF - Ieee transactions on terahertz science and technology

IS - 2

ER -

Development of Mixers for the High Resolution Spectrometer of the Millimetron Space Observatory

Abstract

Keywords

Access to Document

Handle.net

Other files and links

Fingerprint

Cite this