| Author |
Title |
Year |
Publication |
Volume |
Pages |
| Käufl, H. U.; Rothermal, H.; Drapatz, S. |
Investigation of the Martian atmosphere by 10 micron heterodyne spectroscopy |
1984 |
Astron. Astrophys. |
136 |
319-325 |
| Rothermel, H.; Käufl, H. U.; Yu, Y. |
A heterodyne spectrometer for astronomical measurements at 10 micrometers |
1983 |
Astron. Astrophys. |
126 |
387-392 |
| Betz, A. L.; Johnson, M. A.; McLaren, R. A.; Sutton, E. C. |
Heterodyne detection of CO2 emission lines and wind velocities in the atmosphere of Venus |
1976 |
Astrophys. J. |
208 |
L141-L144 |
| Масленников, Сергей Николаевич |
Смесители на эффекте электронного разогрева для терагерцового и инфракрасного диапазонов |
2007 |
М. МПГУ |
|
|
| Soifer, B. T.; Pipher, J. L. |
Instrumentation for infrared astronomy |
1978 |
Annual Rev. Astron. Astrophys. |
16 |
335-369 |
| Thiébeau, C.; Courtois, D.; Delahaigue, A.; Corre, H.; Mouanda, J. C.; Fayt, A. |
Dual-beam laser heterodyne spectrometer: Ethylene absorption spectrum in the 10 μm range |
1988 |
Applied Physics B: Photophysics and Laser Chemistry |
47 |
313-318 |
| Verevkin, A.; Slysz, W.; Pearlman, A.; Zhang, J.; Sobolewski, R.; Okunev, O.; Korneev, A.; Kouminov, P.; Smirnov, K.; Chulkova, G.; Gol’tsman, G. N.; Currie, M. |
Real-time GHz-rate counting of infrared photons using nanostructured NbN superconducting detectors |
2003 |
CLEO/QELS |
|
CThM8 |
| Parrott, Edward P. J.; Zeitler, J. Axel; Fris<cc><152>c<cc><152>ic<cc><81>, Tomislav; Pepper, Michael; Jones, William; Day, Graeme M.; Gladden, Lynn F. |
Testing the sensitivity of terahertz spectroscopy to changes in molecular and supramolecular structure: a study of structurally similar cocrystals |
2009 |
Crystal Growth & Design |
9 |
1452-1460 |
| Финкель, М. И. |
Терагерцовые смесители на эффекте электронного разогрева в ультратонких плёнках NbN и NbTiN |
2006 |
М. МПГУ |
|
|
| Kawakami, A; Saito, S.; Hyodo, M. |
Fabrication of nano-antennas for superconducting Infrared detectors |
2011 |
IEEE Trans. Appl. Supercond. |
21 |
632-635 |
