We present a multi-chroic kinetic inductance detector (KID) pixel design integrated with a broadband hierarchical phased-array antenna. Each low-frequency pixel consists of four high-frequency pixels. Four passbands are designed from 125 to 365 GHz according to the atmospheric windows. The lumped element KIDs consist of 100-nm thick AlMn inductors and Nb parallel plate capacitors with hydrogenated amorphous Si dielectric. Two different coupling structures are designed to couple millimeter-wave from microstrip lines to KIDs. The KID designs are optimized for a 10-m-class telescope at a high, dry site, for example, the Leighton Chajnantor Telescope. Preliminary measurement results using Al KIDs are discussed.Comment: 6 pages, 4 figures, Journ...
We discuss the design, fabrication, and testing of prototype horn-coupled, lumped-element kinetic in...
Kinetic inductance detectors (KIDs) are a promising technology for astronomical observations over a ...
We present recent developments in Kinetic Inductance Detectors (KID) for large arrays of detectors. ...
We present a design for an array of kinetic inductance detectors (KIDs) integrated with phased array...
Current generation millimeter wavelength detectors suffer from scaling limits imposed by complex cry...
Focal plane arrays consisting of low-noise, polarisation-sensitive detectors have made possible the ...
Throughout the last decades, development of low-temperat- ure detectors focused mainly on the design...
Kinetic inductance detectors (KIDs) are a type of athermal pair-breaking superconductingdetectors. S...
Kinetic inductance detectors (KID) have great potential in astronomical observation, such as searchi...
Lumped-element kinetic inductance detectors (LEKIDs) have recently shown considerable promise as dir...
Millimetre-wave astronomical observations have an enormous discovery potential for the study of the...
Context. Current generation millimeter wavelength detectors suffer from scaling limits imposed by co...
Millimetre-wave astronomical observations have an enormous discovery potential for the study of the ...
Very large arrays of Microwave Kinetic Inductance Detectors (MKIDs) have the potential to revolution...
We discuss the design, fabrication, and testing of prototype horn-coupled, lumped-element kinetic in...
Kinetic inductance detectors (KIDs) are a promising technology for astronomical observations over a ...
We present recent developments in Kinetic Inductance Detectors (KID) for large arrays of detectors. ...
We present a design for an array of kinetic inductance detectors (KIDs) integrated with phased array...
Current generation millimeter wavelength detectors suffer from scaling limits imposed by complex cry...
Focal plane arrays consisting of low-noise, polarisation-sensitive detectors have made possible the ...
Throughout the last decades, development of low-temperat- ure detectors focused mainly on the design...
Kinetic inductance detectors (KIDs) are a type of athermal pair-breaking superconductingdetectors. S...
Kinetic inductance detectors (KID) have great potential in astronomical observation, such as searchi...
Lumped-element kinetic inductance detectors (LEKIDs) have recently shown considerable promise as dir...
Millimetre-wave astronomical observations have an enormous discovery potential for the study of the...
Context. Current generation millimeter wavelength detectors suffer from scaling limits imposed by co...
Millimetre-wave astronomical observations have an enormous discovery potential for the study of the ...
Very large arrays of Microwave Kinetic Inductance Detectors (MKIDs) have the potential to revolution...
We discuss the design, fabrication, and testing of prototype horn-coupled, lumped-element kinetic in...
Kinetic inductance detectors (KIDs) are a promising technology for astronomical observations over a ...
We present recent developments in Kinetic Inductance Detectors (KID) for large arrays of detectors. ...