Measuring the CMB spectral distortions with COSMO: the multi-mode antenna system ...
In this work, we present the design and manufacturing of the two multi-mode antenna arrays of the COSMO experiment and the preliminary beam pattern measurements of their fundamental mode compared with simulations. COSMO is a cryogenic Martin-Puplett Fourier Transform Spectrometer that aims at measur...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Report |
Language: | unknown |
Published: |
arXiv
2024
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Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.2406.09349 https://arxiv.org/abs/2406.09349 |
Summary: | In this work, we present the design and manufacturing of the two multi-mode antenna arrays of the COSMO experiment and the preliminary beam pattern measurements of their fundamental mode compared with simulations. COSMO is a cryogenic Martin-Puplett Fourier Transform Spectrometer that aims at measuring the isotropic y-type spectral distortion of the Cosmic Microwave Background from Antarctica, by performing differential measurements between the sky and an internal, cryogenic reference blackbody. To reduce the atmospheric contribution, a spinning wedge mirror performs fast sky-dips at varying elevations while fast, low-noise Kinetic Inductance detectors scan the interferogram. Two arrays of antennas couple the radiation to the detectors. Each array consists of nine smooth-walled multi-mode feed-horns, operating in the $120-180$ GHz and $210-300$ GHz range, respectively. The multi-mode propagation helps increase the instrumental sensitivity without employing large focal planes with hundreds of detectors. The ... : To appear in Proceedings of the SPIE Astronomical Telescopes + Instrumentation, 2024 ... |
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