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Author Meledin, D. V.; Marrone, D. P.; Tong, C.-Y. E.; Gibson, H.; Blundell, R.; Paine, S. N.; Papa, D.C.; Smith, M.; Hunter, T. R.; Battat, J.; Voronov, B.; Gol'tsman, G.
Title A 1-THz superconducting hot-electron-bolometer receiver for astronomical observations Type Journal Article
Year 2004 Publication IEEE Trans. Microwave Theory Techn. Abbreviated Journal (up) IEEE Trans. Microwave Theory Techn.
Volume 52 Issue 10 Pages 2338-2343
Keywords NbN HEB mixer, applications
Abstract In this paper, we describe a superconducting hot-electron-bolometer mixer receiver developed to operate in atmospheric windows between 800-1300 GHz. The receiver uses a waveguide mixer element made of 3-4-nm-thick NbN film deposited over crystalline quartz. This mixer yields double-sideband receiver noise temperatures of 1000 K at around 1.0 THz, and 1600 K at 1.26 THz, at an IF of 3.0 GHz. The receiver was successfully tested in the laboratory using a gas cell as a spectral line test source. It is now in use on the Smithsonian Astrophysical Observatory terahertz test telescope in northern Chile.
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Language Summary Language Original Title
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Series Volume Series Issue Edition
ISSN 0018-9480 ISBN Medium
Area Expedition Conference
Notes Approved no
Call Number Serial 1484
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Author Mehdi, I.; Gol'tsman, G.; Putz, P.
Title Introduction to the mini-special-issue on the 25th international symposium on space terahertz technology (ISSTT) Type Miscellaneous
Year 2015 Publication IEEE Trans. THz Sci. Technol. Abbreviated Journal (up) IEEE Trans. THz Sci. Technol.
Volume 5 Issue 1 Pages 14-15
Keywords
Abstract THE 25th International Symposium on Space Terahertz Technology (ISSTT) was held in Moscow, Russia, between April 27–30, 2014. The conference was organized by Moscow State Pedagogical University and the Higher School of Economics (National Research University) and Chaired by Professor Gregory Gol'tsman of Moscow State Pedagogical University. The conference was attended by roughly 150 participants from 15 countries. The technology covered by ISSTT includes detectors, devices, circuits and systems in various areas of THz science and technology. Each year this symposium brings together the global THz space science technology community, and as such, emphasizes the broad international collaboration that is required to execute these large complicated instrument programs that dominate this field. However, talks covering technologies for balloon, aircraft, and ground-based telescopes were also presented.

In this special section of IEEE Transactions on Terahertz Science and Technology, we include eight expanded papers from the 25th ISSTT symposium. The papers range from development of SIS mixers to optical adjustment systems for radio telescopes. The 26th ISSTT will be held in Boston, MA, USA, during March 16–18, 2015. Researchers and scientist involved in THz research are invited to attend this symposium (more details are at http://www.cfa.harvard.edu/events/2015/isstt2015/).

You can access the full list of papers presented at the ISSTT symposia from the National Radio Astronomy Observatory website: http://www.nrao.edu/meetings/isstt/index.shtml

Yours sincerely
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Language Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 2156-342X ISBN Medium
Area Expedition Conference
Notes Approved no
Call Number Serial 1353
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Author Gol'tsman, G. N.
Title Hot electron bolometric mixers: new terahertz technology Type Journal Article
Year 1999 Publication Infrared Physics & Technology Abbreviated Journal (up) Infrared Physics & Technology
Volume 40 Issue 3 Pages 199-206
Keywords NbN HEB mixers
Abstract This paper presents an overview of recent results for NbN phonon-cooled hot electron bolometric (HEB) mixers. The noise temperature of the receivers based on both quasioptical and waveguide versions of HEB mixers has crossed the level of 1 K GHz−1 at 430 GHz (410 K), 600–650 GHz (480 K), 750 GHz (600 K), 810 GHz (780 K) and is close to that level at 1.1 THz (1250 K) and 2.5 THz (4500 K). The gain bandwidth measured for quasioptical HEB mixer at 620 GHz reached 4 GHz and the noise temperature bandwidth was almost 8 GHz. Local oscillator power requirements are about 1 μW for mixers made by photolithography and about 100 nW for mixers made by e-beam lithography. A waveguide version of 800 GHz receiver was installed at the Submillimeter Telescope Observatory on Mt. Graham, AZ, to conduct astronomical observations of known submillimeter lines (CO, J=7→6, CI, J=2→1). It was proved that the receiver works as a practical instrument.
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Language Summary Language Original Title
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Series Volume Series Issue Edition
ISSN 1350-4495 ISBN Medium
Area Expedition Conference
Notes Approved no
Call Number Serial 1570
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Author Slysz, W.; Wegrzecki, M.; Papis, E.; Gol'tsman, G. N.; Verevkin, A.; Sobolewski, R.
Title A method of optimization of the NbN superconducting single-photon detector Type Miscellaneous
Year 2004 Publication INIS Abbreviated Journal (up) INIS
Volume 36 Issue 27 Pages 1-2
Keywords NbN SSPD, SNSPD
Abstract
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Area Expedition Conference 5-th International Symposium Ion Implantation and Other Applications of Ions and Electrons, ION
Notes Reference num. 36060124 Approved no
Call Number Serial 1485
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Author Slysz, W.; Wegrzecki, M.; Bar, J.; Grabiec, P.; Gol'tsman, G. N.; Verevkin, M.; Sobolewski, R.
Title NbN superconducting single-photon detectors coupled with a communication fiber Type Miscellaneous
Year 2004 Publication INIS Abbreviated Journal (up) INIS
Volume 37 Issue 2 Pages 1-2
Keywords NbN SSPD, SNSPD
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Address Stare Jablonki, Poland
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Area Expedition Conference 8-th Electron Technology Conference ELTE
Notes Approved no
Call Number Serial 1486
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