We present the design of ALMA Band 5 sideband separation SIS mixer and experimental results for the double side band mixer and first measurement results 2SB mixer. In this mixer, the LO injection circuitry is integrated on the mixer substrate using a directional coupler, combining microstrip lines with slot-line branches in the ground plane. The isolated port of the LO coupler is terminated by wideband floating elliptical termination. The mixer employs two SIS junctions with junction area of 3 μm2 each, in the twin junction configuration, followed by a quarter wave transformer to match the RF probe. 2SB mixer uses two identical but mirrored chips, whereas each DSB mixer has the same end-piece configuration. The 2S mixer has modular design s...
In this article we present the design, modeling and construction of a side-band-separating (2SB) het...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
The ALMA Band 6 (211-275 GHz) receivers use sideband-separating SIS mixer-preamplifiers with dual 4-...
We present the design of ALMA Band 5 sideband separation SIS mixer and experimental results for the ...
We present the design of ALMA Band 5 sideband separation mixer based on Niobium superconducting SIS ...
This licentiate is focused on the design and development of Superconductor-Insulator-Superconductor ...
The ALMA Band 9 receiver cartridge (600-720 GHz) based on Dual Sideband (DSB) superconductor-insulat...
The ALMA Band 9 receiver cartridge (600-720 GHz) based on Dual Sideband (DSB) superconductor-insulat...
For high-frequency observational bands like ALMA (Atacama Large Millimeter Array) Band 9 (600—720 GH...
This thesis presents work done in developing instrumentation for mm-wave radio astronomy. The main s...
Following the design for a sideband-separating mixer using a quadrature waveguide hybrid and an in-p...
This work presents results of the development and measurements of a heterodyne sideband separating S...
We present results of the development and measurements of a heterodyne sideband separating SIS mixer...
Here we present the realization of a side-band-separating (2SB) heterodyne mixer for the frequency r...
In this article we present the design, modeling and construction of a side-band-separating (2SB) het...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
The ALMA Band 6 (211-275 GHz) receivers use sideband-separating SIS mixer-preamplifiers with dual 4-...
We present the design of ALMA Band 5 sideband separation SIS mixer and experimental results for the ...
We present the design of ALMA Band 5 sideband separation mixer based on Niobium superconducting SIS ...
This licentiate is focused on the design and development of Superconductor-Insulator-Superconductor ...
The ALMA Band 9 receiver cartridge (600-720 GHz) based on Dual Sideband (DSB) superconductor-insulat...
The ALMA Band 9 receiver cartridge (600-720 GHz) based on Dual Sideband (DSB) superconductor-insulat...
For high-frequency observational bands like ALMA (Atacama Large Millimeter Array) Band 9 (600—720 GH...
This thesis presents work done in developing instrumentation for mm-wave radio astronomy. The main s...
Following the design for a sideband-separating mixer using a quadrature waveguide hybrid and an in-p...
This work presents results of the development and measurements of a heterodyne sideband separating S...
We present results of the development and measurements of a heterodyne sideband separating SIS mixer...
Here we present the realization of a side-band-separating (2SB) heterodyne mixer for the frequency r...
In this article we present the design, modeling and construction of a side-band-separating (2SB) het...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
The ALMA Band 6 (211-275 GHz) receivers use sideband-separating SIS mixer-preamplifiers with dual 4-...