rays to measure the polarization of the cosmic microwave background. 217 GHz prototype pixels have previously been characterized and showed promising per-formance1. Our design uses a double slot dipole antenna and an integrated mi-crostrip band defining filter. New devices have been tested which include on-chip test structures to improve our understanding of detector performance and guide future development. In parallel with this, large arrays of bolometers based on the prototype pixel design have also been constructed. The array pixels are a hetero-geneous mixture of single band pixels at 90 GHz, 150 GHz, and 220 GHz and now incorporate dual-polarization antennas2. Preliminary results from optical testing of array pixels are presented. The...
We describe the design and simulation of a novel dual-polarized multi-frequency singlepixel for next...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
Characterization of the minute cosmic microwave background polarization signature requires multi-fre...
We are building antenna-coupled Transition Edge Sensor bolometer arrays to measure the polarization ...
Characterization of the Cosmic Microwave Background (CMB) B-mode polarization signal will test model...
Characterization of the Cosmic Microwave Background (CMB) B-mode polarization signal will test model...
New technology has rapidly advanced the field of observational cosmology over the last 30 years. Th...
We describe the design, fabrication, and laboratory-demonstration of a novel dual-polarized multichr...
We describe the design, fabrication, and laboratory-demonstration of a novel dual-polarized multichr...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Bac...
We are developing multi-chroic antenna-coupled Transition Edge Sensor (TES) focal planes for Cosmic ...
We are developing multi-chroic antenna-coupled Transition Edge Sensor (TES) focal planes for Cosmic ...
We describe the design and simulation of a novel dual-polarized multi-frequency singlepixel for next...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
Characterization of the minute cosmic microwave background polarization signature requires multi-fre...
We are building antenna-coupled Transition Edge Sensor bolometer arrays to measure the polarization ...
Characterization of the Cosmic Microwave Background (CMB) B-mode polarization signal will test model...
Characterization of the Cosmic Microwave Background (CMB) B-mode polarization signal will test model...
New technology has rapidly advanced the field of observational cosmology over the last 30 years. Th...
We describe the design, fabrication, and laboratory-demonstration of a novel dual-polarized multichr...
We describe the design, fabrication, and laboratory-demonstration of a novel dual-polarized multichr...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Bac...
We are developing multi-chroic antenna-coupled Transition Edge Sensor (TES) focal planes for Cosmic ...
We are developing multi-chroic antenna-coupled Transition Edge Sensor (TES) focal planes for Cosmic ...
We describe the design and simulation of a novel dual-polarized multi-frequency singlepixel for next...
We describe the development of an antenna-coupled bolometer array for use in a Cosmic Microwave Back...
Characterization of the minute cosmic microwave background polarization signature requires multi-fre...