We present a broadband and low noise heterodyne receiver for 1.4-1.7 THz designed for the Hershel Space Observatory. A phonon- cooled NbN HEB mixer was integrated with a normal metal double- slot antenna and an elliptical silicon lens. DSB receiver noise temperature Tr was measured from 1 GHz through 8GHz intermediate frequency band with 50 MHz instantaneous bandwidth. At 4.2 K bath temperature and at 1.6 THz LO frequency Tr is 800 K with the receiver noise bandwidth of 5 GHz. While at 2 K bath temperature Tr was as low as 700 K. At 0.6 THz and 1.1 THz a spiral antenna integrated NbN HEB mixer showed the receiver noise temperature 500 K and 800 K, though no antireflection coating was used in this case. Tr of 1100 K was achieved at 2.5 THz w...
The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy hetero...
NbN hot-electron bolometer mixers have reached the leve of 10 hv/k in terms of the input noise tempe...
NbN HEB mixers represent a promising approach for achieving receiver noise temperatures of a few tim...
Abstract: Low noise receivers using quasi-optical superconducting niobium nitride (NbN) hot electron...
The performance of NbN based HEB mixers has been investigated at THz fre-quencies in a receiver with...
During the past decade major advances have been made regarding low noise mixers for terahertz (THz) ...
We report on low noise terahertz mixers (1.4–1.9 THz) developed for the heterodyne spectrometer onbo...
Hot Electron Bolometric (HEB) mixers have recently demonstrated the lowest receiver noise tem-peratu...
We report on low noise terahertz mixers (1.4–1.9 THz) developed for the heterodyne spectrometer onbo...
We have characterized a heterodyne receiver based on an NbN hot electron bolometer integrated with s...
Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments ...
We report the measured sensitivities of a superconducting NbN hot electron bolometer (HEB) heterodyn...
We have characterized a heterodyne receiver based on an NbN hot electron bolometer integrated with s...
We report the measured sensitivities of a superconducting NbN hot electron bolometer (HEB) heterodyn...
The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy hetero...
The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy hetero...
NbN hot-electron bolometer mixers have reached the leve of 10 hv/k in terms of the input noise tempe...
NbN HEB mixers represent a promising approach for achieving receiver noise temperatures of a few tim...
Abstract: Low noise receivers using quasi-optical superconducting niobium nitride (NbN) hot electron...
The performance of NbN based HEB mixers has been investigated at THz fre-quencies in a receiver with...
During the past decade major advances have been made regarding low noise mixers for terahertz (THz) ...
We report on low noise terahertz mixers (1.4–1.9 THz) developed for the heterodyne spectrometer onbo...
Hot Electron Bolometric (HEB) mixers have recently demonstrated the lowest receiver noise tem-peratu...
We report on low noise terahertz mixers (1.4–1.9 THz) developed for the heterodyne spectrometer onbo...
We have characterized a heterodyne receiver based on an NbN hot electron bolometer integrated with s...
Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments ...
We report the measured sensitivities of a superconducting NbN hot electron bolometer (HEB) heterodyn...
We have characterized a heterodyne receiver based on an NbN hot electron bolometer integrated with s...
We report the measured sensitivities of a superconducting NbN hot electron bolometer (HEB) heterodyn...
The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy hetero...
The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy hetero...
NbN hot-electron bolometer mixers have reached the leve of 10 hv/k in terms of the input noise tempe...
NbN HEB mixers represent a promising approach for achieving receiver noise temperatures of a few tim...