| Records |
| Author |
Dahl, H.; Metz, H. J.; Wriedt, T. |
| Title |
Light scattering of silver halide crystals |
Type |
Conference Article |
| Year |
1998 |
Publication |
Proc. 3rd Workshop on Electromagnetic and Light Scattering |
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Issue |
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Pages |
51-58 |
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Place of Publication |
Universität Bremen |
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no |
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Serial  |
504 |
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| Author |
Bingham, S. J.; Börger, B.; Suter, D.; Thomson, A. J. |
| Title |
The design and sensitivity of microwave frequency optical heterodyne receivers |
Type |
Journal Article |
| Year |
1998 |
Publication |
Review of Scientific Instruments |
Abbreviated Journal |
Rev. Sci. Instrum. |
| Volume |
69 |
Issue |
9 |
Pages |
3403-3409 |
| Keywords |
optical mixing |
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0034-6748 |
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no |
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Serial |
508 |
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| Author |
Dieleman, Piter |
| Title |
Fundamental limitations of THz niobium and niobiumnitride SIS mixers |
Type |
Book Whole |
| Year |
1998 |
Publication |
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SIS |
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Ph.D. thesis |
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Place of Publication |
Rijksuniversiteit, Groningen |
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no |
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Serial |
529 |
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| Author |
Floet, D. Wilms; Baselmans, J. J. A.; Klapwijk, T. M.; Gao, J. R. |
| Title |
Resistive transition of niobium superconducting hot-electron bolometer mixers |
Type |
Journal Article |
| Year |
1998 |
Publication |
Applied Physics Letters |
Abbreviated Journal |
Appl. Phys. Lett. |
| Volume |
73 |
Issue |
19 |
Pages |
2826 |
| Keywords |
HEB |
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0003-6951 |
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no |
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543 |
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Kawamura, Jonathan; Blundell, Raymond; Tong, C.-Y. Edward; Papa, D. Cosmo; Hunter, Todd R.; Gol'tsman, Gregory; Cherednichenko, Sergei; Voronov, Boris; Gershenzon, Eugene |
| Title |
First light with an 800 GHz phonon-cooled HEB mixer receiver |
Type |
Conference Article |
| Year |
1998 |
Publication |
Proc. 9th Int. Symp. Space Terahertz Technol. |
Abbreviated Journal |
Proc. 9th Int. Symp. Space Terahertz Technol. |
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Issue |
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Pages |
35-43 |
| Keywords |
HEB, mixer, LO power, local oscillator power, saturation effect, dynamic range |
| Abstract |
Phonon-cooled superconductive hot-electron bolometric (HEB) mixers are incorporated in a waveguide receiver designed to operate near 800 Gliz. The mixer elements are thin-film nio- bium nitride microbridges with dimensions of 4 nm thickness, 0.2 to 0.3 p.m in length and 2 jun in width. At 780 GHz the best receiver noise temperature is 840 K (DSB). The mixer IF bandwidth is 2.0 GHz, the absorbed LO power is —0.1 1.1W. A fixed-tuned version of the re- ceiver was installed at the Submillimeter Telescope Observatory on Mt. Graham, Arizona, to conduct astronomical observations. These observations represent the first time that a receiver incorporating any superconducting HEB mixer has been used to detect a spectral line of celes- tial origin. |
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Pasadena, California, USA |
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no |
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Serial |
572 |
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