Mele, L., Battistelli, E.S., de Bernardis, P., Bersanelli, M., Columbro, F., Coppi, G., Coppolecchia, A., D’Alessandro, G., De Petris, M., Franceschet, F., Gervasi, M., Lamagna, L., Limonta, A., Manzan, E., Marchitelli, E., Masi, S., Mennella, A., Nati, F., Paiella, A., Pettinari, G., Piacentini, F., Piccirillo, L., Pisano, G., Realini, S., Tucker, Carole ![]() ![]() |
![]() |
PDF
- Published Version
Available under License Creative Commons Attribution. Download (1MB) |
Abstract
COSMO is a ground-based instrument to measure the spectral distortions (SD) of the Cosmic Microwave Background (CMB). In this paper, we present preliminary results of electromagnetic simulations of its reference blackbody calibrator. HFSS simulations provide a calibrator reflection coefficient of $$R\sim 10^{-6}$$ R ∼ 10 - 6 , corresponding to an emissivity $$\epsilon =1-R=0.999999$$ ϵ = 1 - R = 0.999999 . We also provide a forecast for the instrument performance by using an ILC-based simulation. We show that COSMO can extract the isotropic Comptonization parameter (modeled as $$|y|=1.77 \cdot 10^{-6}$$ | y | = 1.77 · 10 - 6 ) as $$|y|=(1.79\pm 0.19)\cdot 10^{-6}$$ | y | = ( 1.79 ± 0.19 ) · 10 - 6 , in the presence of the main Galactic foreground (thermal dust) and of CMB anisotropies, and assuming perfect atmospheric emission removal....
Item Type: | Article |
---|---|
Date Type: | Published Online |
Status: | Published |
Schools: | Physics and Astronomy |
Date of First Compliant Deposit: | 13 February 2023 |
Date of Acceptance: | 5 September 2022 |
Last Modified: | 03 May 2023 08:12 |
URI: | https://orca.cardiff.ac.uk/id/eprint/156618 |
Actions (repository staff only)
![]() |
Edit Item |