Add to ORKGSMILES is a heterodyne sub-millimeter receiver which will be installed on the ELM-ES platform of the Japanese Experimental Module on the International Space Station in 2003. For the scientific side, the advantage of SIS technology is the up to five times lower system noise temperature of the receiver compared with conventional ones and therefore provides a much better resolution, both in time and space.Upprättat; 1999; 20070514 (pafi)</p
The concept of the fully Superconducting Integrated Receiver (SIR) has been developed and experiment...
A superconducting integrated receiver (SIR) comprises in a single chip a planar antenna combined wit...
We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, ...
SMILES is a heterodyne sub-millimeter receiver which will be installed on the ELM-ES platform of the...
A new generation of sub-millimeter-wave receivers employing sensitive SIS (Superconductor-Insulator-...
Communications Research Laboratory and National Space Development Agency of Japan are collaborating ...
A 230 GHz SIS tunnel junction receiver has been being developed for radio astronomy in Nagoya Univer...
The submillimeter-wave limb-emission sounder called SMILES is currently being developed for the Japa...
successfully launched and attached to the Japanese Experiment Module (JEM) on the International Spac...
Recent progress in sub-millimeter wave receiver technology gives the possibility to drastically impr...
A broadband, low noise heterodyne receiver, suitable for astronomical use, has been built using a Pb...
Our group has designed a heterodyne submillimeter receiver that offers a very wide IF bandwidth of 1...
The development of SIS mixers at 640 GHz band is a key issue of JENI/SNIILES mission [1], which is a...
Abstract: The developments in the field of low-noise receiving systems in the sub-THz range, perform...
We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, ...
The concept of the fully Superconducting Integrated Receiver (SIR) has been developed and experiment...
A superconducting integrated receiver (SIR) comprises in a single chip a planar antenna combined wit...
We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, ...
SMILES is a heterodyne sub-millimeter receiver which will be installed on the ELM-ES platform of the...
A new generation of sub-millimeter-wave receivers employing sensitive SIS (Superconductor-Insulator-...
Communications Research Laboratory and National Space Development Agency of Japan are collaborating ...
A 230 GHz SIS tunnel junction receiver has been being developed for radio astronomy in Nagoya Univer...
The submillimeter-wave limb-emission sounder called SMILES is currently being developed for the Japa...
successfully launched and attached to the Japanese Experiment Module (JEM) on the International Spac...
Recent progress in sub-millimeter wave receiver technology gives the possibility to drastically impr...
A broadband, low noise heterodyne receiver, suitable for astronomical use, has been built using a Pb...
Our group has designed a heterodyne submillimeter receiver that offers a very wide IF bandwidth of 1...
The development of SIS mixers at 640 GHz band is a key issue of JENI/SNIILES mission [1], which is a...
Abstract: The developments in the field of low-noise receiving systems in the sub-THz range, perform...
We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, ...
The concept of the fully Superconducting Integrated Receiver (SIR) has been developed and experiment...
A superconducting integrated receiver (SIR) comprises in a single chip a planar antenna combined wit...
We report on research in the field of low-noise receiving systems in the sub-terahertz (THz) range, ...