A modular sideband-separating (2SB) receiver for 600-720 GHz has been built and tested. The used modular design allows to characterize all the parts separately, including testing of the superconductor-insulator-superconductor (SIS) junctions individually in a double-sideband mode before building them in to the 2SB assembly. The developed 2SB mixer has a single side-band noise temperature below 380 K in the entire operating band and reaches a level of 200Kin the best point. At the same time, the image rejection ratio (IRR) was demonstrated to be better than 11.5 dB over the entire band. However, we have found a discrepancy between the observed and expected performance. To investigate this problem, we have developed and applied methods to cha...
The sideband separating SIS receivers are known as the most sensitive instruments for millimeter and...
Superconductor-insulator-superconductor (SIS) mixers are the most sensitive heterodyne receivers for...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
A modular sideband-separating (2SB) receiver for 600-720 GHz has been built and tested. The used mod...
A modular sideband-separating (2SB) receiver for 600-720 GHz has been built and tested. The used mod...
We present the design and results of characterization of a new sideband separating (2SB) mixer for 8...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
The ALMA Band 9 receiver cartridge (600-720 GHz) based on Dual Sideband (DSB) superconductor-insulat...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
The thesis presents work done in improving the sideband rejection ratio for 2SB cryogenic radio astr...
We have developed a Sideband Separating (2SB) Mixer based on superconductor-insulator-superconductor...
This thesis presents work done in developing instrumentation for mm-wave radio astronomy. The main s...
Artículo de publicación ISIWe present the design, modeling, construction, and characterization of a ...
The sideband separating SIS receivers are known as the most sensitive instruments for millimeter and...
Superconductor-insulator-superconductor (SIS) mixers are the most sensitive heterodyne receivers for...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
A modular sideband-separating (2SB) receiver for 600-720 GHz has been built and tested. The used mod...
A modular sideband-separating (2SB) receiver for 600-720 GHz has been built and tested. The used mod...
We present the design and results of characterization of a new sideband separating (2SB) mixer for 8...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
The ALMA Band 9 receiver cartridge (600-720 GHz) based on Dual Sideband (DSB) superconductor-insulat...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
The thesis presents work done in improving the sideband rejection ratio for 2SB cryogenic radio astr...
We have developed a Sideband Separating (2SB) Mixer based on superconductor-insulator-superconductor...
This thesis presents work done in developing instrumentation for mm-wave radio astronomy. The main s...
Artículo de publicación ISIWe present the design, modeling, construction, and characterization of a ...
The sideband separating SIS receivers are known as the most sensitive instruments for millimeter and...
Superconductor-insulator-superconductor (SIS) mixers are the most sensitive heterodyne receivers for...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...