A chemically etched corrugated feedhorn array for D-band CMB observations
arXiv:2006.14889 · doi:10.1007/s10686-021-09698-9
Abstract
We present the design, manufacturing, and testing of a 37-element array of corrugated feedhorns for Cosmic Microwave Background (CMB) measurements between and GHz. The array was designed to be coupled to Kinetic Inductance Detector arrays, either directly (for total power measurements) or through an orthomode transducer (for polarization measurements). We manufactured the array in platelets by chemically etching aluminum plates of mm and mm thickness. The process is fast, low-cost, scalable, and yields high-performance antennas compared to other techniques in the same frequency range. Room temperature electromagnetic measurements show excellent repeatability with an average cross polarization level about dB, return loss about dB, first sidelobes below dB and far sidelobes below dB. Our results qualify this process as a valid candidate for state-of-the-art CMB experiments, where large detector arrays with high sensitivity and polarization purity are of paramount importance in the quest for the discovery of CMB polarization -modes.
References in corpus (9)
- Statistics of Cosmic Microwave Background Polarization
- A Measurement of the Cosmic Microwave Background B-Mode Polarization Power Spectrum at Sub-Degree Scales with POLARBEAR
- BICEP2 / Keck Array VIII: Measurement of gravitational lensing from large-scale B-mode polarization
- A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg of SPTpol Temperature and Polarization Data
- Horn Coupled Multichroic Polarimeters for the Atacama Cosmology Telescope Polarization Experiment
- Kinetic Inductance Detectors for the OLIMPO experiment: in--flight operation and performance
- Kinetic Inductance Detectors for the OLIMPO experiment: design and pre-flight characterization
- Thermal kinetic inductance detectors for ground-based millimeter-wave cosmology
- The NIKA instrument: results and perspectives towards a permanent KID based camera for the Pico Veleta observatory