A chemically etched corrugated feedhorn array for D-band CMB observations

Autor: Giorgio Pettinari, A. Volpe, E. Tommasi, D. Viganò, Massimo Gervasi, A. Passerini, F. Piacentini, E. Manzan, Alessandro Paiella, Marco Castellano, Cristian Franceschet, Luca Lamagna, S. Mandelli, A. Limonta, Marco Bersanelli, Mario Zannoni, Francesco Cavaliere, P. de Bernardis, Silvia Masi, Alessandro Coppolecchia, Angelo Cruciani, A. Mennella
Přispěvatelé: Mandelli, S, Manzan, E, Mennella, A, Cavaliere, F, Viganò, D, Franceschet, C, de Bernardis, P, Bersanelli, M, Castellano, M, Coppolecchia, A, Cruciani, A, Gervasi, M, Lamagna, L, Limonta, A, Masi, S, Paiella, A, Passerini, A, Pettinari, G, Piacentini, F, Tommasi, E, Volpe, A, Zannoni, M
Rok vydání: 2020
Předmět:
Zdroj: Experimental astronomy
(2021). doi:10.1007/s10686-021-09698-9
info:cnr-pdr/source/autori:Mandelli, S.; Manzan, E.; Mennella, A.; Cavaliere, F.; Viganò, D.; Franceschet, C.; de Bernardis, P.; Bersanelli, M.; Castellano, M. G.; Coppolecchia, A.; Cruciani, A.; Gervasi, M.; Lamagna, L.; Limonta, A.; Masi, S.; Paiella, A.; Passerini, A.; Pettinari, G.; Piacentini, F.; Tommasi, E.; Volpe, A.; Zannoni, M./titolo:A chemically etched corrugated feedhorn array for D-band CMB observations/doi:10.1007%2Fs10686-021-09698-9/rivista:Experimental astronomy (Print)/anno:2021/pagina_da:/pagina_a:/intervallo_pagine:/volume
DOI: 10.48550/arxiv.2006.14889
Popis: We present the design, manufacturing, and testing of a 37-element array of corrugated feedhorns for Cosmic Microwave Background CMB) measurements between 140 and 170 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 0.3 mm and 0.4 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 − 20 dB, return loss about − 25 dB, first sidelobes below − 25 dB and far sidelobes below − 35 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 polarizationB-modes.
Databáze: OpenAIRE