| Records |
| Author |
Maddison, B. J.; Martin, R. J.; Oldfield, M. L.; Mann, C. M.; Matheson, D. N.; Ellison, B. N.; Thornton, J.; Hall, W. J.; Lamarre, D. M. |
| Title |
A compact 500 GHz planar schottky siode receiver with a wide instantaneous bandwidth |
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Conference Article |
| Year |
1998 |
Publication |
Proc. 9th Int. Symp. Space Terahertz Technol. |
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367 |
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no |
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RPLAB @ s @ schottky_Tn_4800_at_p5THz |
Serial |
286 |
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| Author |
Brown, Robert. L. |
| Title |
Technical specification of the Millimeter Array |
Type |
Conference Article |
| Year |
1998 |
Publication |
Proc. SPIE, Advanced Technology MMW, Radio, and Terahertz Telescopes, vol. 3357 |
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231-237 |
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Phillips, Thomas G. |
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Address is unknown |
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no |
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RPLAB @ s @ ALMA_tech |
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287 |
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| Author |
Dahl, H.; Metz, H. J.; Wriedt, T. |
| Title |
Light scattering of silver halide crystals |
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Conference Article |
| Year |
1998 |
Publication |
Proc. 3rd Workshop on Electromagnetic and Light Scattering |
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51-58 |
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Universität Bremen |
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no |
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504 |
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| Author |
Dieleman, Piter |
| Title |
Fundamental limitations of THz niobium and niobiumnitride SIS mixers |
Type |
Book Whole |
| Year |
1998 |
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SIS |
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Ph.D. thesis |
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Rijksuniversiteit, Groningen |
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no |
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529 |
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| Author |
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 |
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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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35-43 |
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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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572 |
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