ABSTRACT- We are developing a heterodyne focal plane array with up to eight ele-ments to study lines of the interstellar medium and planetary atmospheres with frequencies of 2 THz and above. Our fabrication process utilizes selective ion milling techniques to pro-duce Nb Diffusion-Cooled Hot Electron Bolometeric (DHEB) mixers from a bi-layer thin film of Au/Nb deposited on a silicon substrate. A micro-bridge of 10 nm thick Nb forms the HEB device. The first generation of devices with lateral dimensions of 100 nm by 80 nm were fabricated at the feed of a broadband spiral antenna with a frequency response de-signed for up to 16 THz. Harmonic multiplier sources becoming available within the next few years should have sufficient power to provid...
Open AccessIn this paper, we present the development of the waveguide niobium titanium nitride (NbTi...
Abstract: Low noise receivers using quasi-optical superconducting niobium nitride (NbN) hot electron...
Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments ...
The goal of this project was to fabricate and test planar arrays of superconducting mixers for the 2...
We report on design and characterization of a superconducting Hot Electron Bolometer Mixer integrate...
Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments ...
NbN HEB mixers represent a promising approach for achieving receiver noise temperatures of a few tim...
The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy hetero...
ABSTRACT-In recent years, improvements in device development and quasi-optical coupling techniques u...
A 16 pixel heterodyne receiver for 2.5 THz has been developed based on NbN superconducting hot-elect...
NbN hot electron bolometer (HEB) mixers are at this moment the best heterodyne detectors for frequen...
Experimental work on the development of a quasi-optical heterodyne receiver for the THz frequency ra...
Abstract — A 16 pixel heterodyne receiver for 2.5 THz has been developed based on NbN superconductin...
We present recent advances in the development of NbN hot-electron bolometric (HEB) mixers for flying...
We report the sensitivity of a superconducting NbN hot electron bolometer mixer integrated with a ti...
Open AccessIn this paper, we present the development of the waveguide niobium titanium nitride (NbTi...
Abstract: Low noise receivers using quasi-optical superconducting niobium nitride (NbN) hot electron...
Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments ...
The goal of this project was to fabricate and test planar arrays of superconducting mixers for the 2...
We report on design and characterization of a superconducting Hot Electron Bolometer Mixer integrate...
Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments ...
NbN HEB mixers represent a promising approach for achieving receiver noise temperatures of a few tim...
The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy hetero...
ABSTRACT-In recent years, improvements in device development and quasi-optical coupling techniques u...
A 16 pixel heterodyne receiver for 2.5 THz has been developed based on NbN superconducting hot-elect...
NbN hot electron bolometer (HEB) mixers are at this moment the best heterodyne detectors for frequen...
Experimental work on the development of a quasi-optical heterodyne receiver for the THz frequency ra...
Abstract — A 16 pixel heterodyne receiver for 2.5 THz has been developed based on NbN superconductin...
We present recent advances in the development of NbN hot-electron bolometric (HEB) mixers for flying...
We report the sensitivity of a superconducting NbN hot electron bolometer mixer integrated with a ti...
Open AccessIn this paper, we present the development of the waveguide niobium titanium nitride (NbTi...
Abstract: Low noise receivers using quasi-optical superconducting niobium nitride (NbN) hot electron...
Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments ...