We describe the design, fabrication and test results of a multi-channel heterodyne receiver operating at room temperature across the 2.3-8.2 GHz Radio Frequency (RF) band. Such a “Warm Section” (WS) receiver is part of a Phased Array Feed (PAF) demonstrator that is being built for radio astronomy application. The WS receiver is cascaded to the PAF cryogenic section that incorporates an antenna array with low noise pre-amplification stages. The WS receiver consists of four rack-mountable modules, each of which can process eight RF inputs. Four modules are arranged in a standard 19” rack to allow handling a total of 32 RF signals. The modules perform filtering (through four-way switch filter bank) and down-conversion (to the 375-650 MHz IF ba...
We present the upGREAT THz heterodyne arrays for far-infrared astronomy. The low-frequency array (LF...
We describe the design of an integrated cryogenic receiver module based on an “active” waveguide Ort...
Current and future large arrays for radio astronomy are compared and the Next Generation Very Large ...
This paper describes the design, fabrication, and test results of a room temperature multi-channel h...
We describe the design and architecture of PHAROS2, a cryogenically cooled 4-8 GHz Phased Array Feed...
This project entitled "Implementation of a multi-channel RF front-end for space-time processing syst...
Phased array feed (PAF) receivers used on radio astronomy telescopes offer the promise of increased ...
This master thesis presents the design and implementation of a super heterodyne 5.8 GHz receiver sys...
Our group has designed a heterodyne submillimeter receiver that offers a very wide IF bandwidth of 1...
HEMT-based receiver arrays with excellent noise and scalability are already starting to be manufactu...
Sub-millimetre wave or terahertz heterodyne receivers operating above 300 GHz are key instruments fo...
Contains research objectives.National Science Foundation (Grant AST79-20984)National Aeronautics and...
This research work proposes a novel approach and topology of a compact two-pixel heterodyne integrat...
We report on the development of W-band (75–110 GHz) heterodyne receiver technology for large-format ...
The noise temperature of existing millimeter-wave receivers is already within two or three times qua...
We present the upGREAT THz heterodyne arrays for far-infrared astronomy. The low-frequency array (LF...
We describe the design of an integrated cryogenic receiver module based on an “active” waveguide Ort...
Current and future large arrays for radio astronomy are compared and the Next Generation Very Large ...
This paper describes the design, fabrication, and test results of a room temperature multi-channel h...
We describe the design and architecture of PHAROS2, a cryogenically cooled 4-8 GHz Phased Array Feed...
This project entitled "Implementation of a multi-channel RF front-end for space-time processing syst...
Phased array feed (PAF) receivers used on radio astronomy telescopes offer the promise of increased ...
This master thesis presents the design and implementation of a super heterodyne 5.8 GHz receiver sys...
Our group has designed a heterodyne submillimeter receiver that offers a very wide IF bandwidth of 1...
HEMT-based receiver arrays with excellent noise and scalability are already starting to be manufactu...
Sub-millimetre wave or terahertz heterodyne receivers operating above 300 GHz are key instruments fo...
Contains research objectives.National Science Foundation (Grant AST79-20984)National Aeronautics and...
This research work proposes a novel approach and topology of a compact two-pixel heterodyne integrat...
We report on the development of W-band (75–110 GHz) heterodyne receiver technology for large-format ...
The noise temperature of existing millimeter-wave receivers is already within two or three times qua...
We present the upGREAT THz heterodyne arrays for far-infrared astronomy. The low-frequency array (LF...
We describe the design of an integrated cryogenic receiver module based on an “active” waveguide Ort...
Current and future large arrays for radio astronomy are compared and the Next Generation Very Large ...