2014 39th International Conference on Infrared, Millimeter, and Terahertz Waves (IRMMW-THz) 2014
DOI: 10.1109/irmmw-thz.2014.6956148
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Waveguide hot electron bolometer mixer development for upGREAT

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Cited by 4 publications
(5 citation statements)
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“…However, due to their physical working principle, they inherently possess a roll-off of their gain bandwidth, which can be associated with the cooling rate of "hot" electrons [2]. Consequently, the usable IF band of state-of-the-art receivers still remains limited to typically 0.2-5 GHz [3], [4], [5], which may not be sufficient for spectroscopic observations of distant, fast moving objects due to spectral line broadening and restricts the efficient use of observation time. In recent years, the prospective use of MgB 2 with high critical temperature (Tc) of 39 K for HEB mixer applications has become a promising candidate to boost the IF bandwidth performance due to its fast thermal relaxation time.…”
Section: Introductionmentioning
confidence: 99%
“…However, due to their physical working principle, they inherently possess a roll-off of their gain bandwidth, which can be associated with the cooling rate of "hot" electrons [2]. Consequently, the usable IF band of state-of-the-art receivers still remains limited to typically 0.2-5 GHz [3], [4], [5], which may not be sufficient for spectroscopic observations of distant, fast moving objects due to spectral line broadening and restricts the efficient use of observation time. In recent years, the prospective use of MgB 2 with high critical temperature (Tc) of 39 K for HEB mixer applications has become a promising candidate to boost the IF bandwidth performance due to its fast thermal relaxation time.…”
Section: Introductionmentioning
confidence: 99%
“…In the latter IF and noise bandwidth measurements were performed at 1.3 THz with waveguide balanced configuration of the mixers. This represents a significant improvement to commonly used NbN HEBs on silicon substrates [9,10].…”
Section: Signal To Noise Bandwidthmentioning
confidence: 97%
“…However, they continue to suffer from a relatively narrow IF bandwidth, which limits the effectiveness of the heterodyne operation. The typical value of the gain and noise bandwidths for NbN-based HEB mixers on conventional substrates such as sapphire is about 3-4 GHz [7][8][9][10]. Those working in the HEB field know from experience that changes in the embedding of the device does not show up in IF-performance.…”
Section: Introductionmentioning
confidence: 99%
“…At present,HEB mixers and direct detectors have proved themselves as perfect tools for radioastronomy and terahertz spectroscopy [1][2][3][4]. Frequency independence of the response formation mechanism of an HEB-based detector to radiation within a wide frequency range in conjunction with a sufficiently high sensitivity and relatively small response time [5][6][7][8][9] make the HEB the most attractive candidate for observations above 1 THz.…”
Section: Hot Electron Phenomena In a Superconducting Film: Discovery ...mentioning
confidence: 99%
“…It is worth mentioning that being historically the first type of HEB device developed, thephonon-cooled HEB mixer has to date confirmedits suitability for practical heterodyne instruments, e.g. the Heinrich Hertz Telescope [22], the Receiver Lab Telescope [262], APEX [146], SOFIA [4,5], Hershel [1,2].…”
Section: Phonon-cooled Hebmentioning
confidence: 99%