학술논문
Radio Antenna Design for Sky-Averaged 21cm Cosmology Experiments: The REACH Case
Document Type
Article
Author
Cumner, J.; de Lera Acedo, E.; de Villiers, D. I. L.; Anstey, D.; Kolitsidas, C. I.; Gurdon, B.; Fagnoni, N.; Alexander, P.; Bernardi, G.; Bevins, H. T. J.; Carey, S.; Cavillot, J.; Chiello, R.; Craeye, C.; Croukamp, W.; Ely, J. A.; Fialkov, A.; Gessey-Jones, T.; Gueuning, Q.; Handley, W.; Hills, R.; Josaitis, A. T.; Kulkarni, G.; Magro, A.; Maiolino, R.; Meerburg, P. D.; Mittal, S.; Pritchard, J. R.; Puchwein, E.; Razavi-Ghods, N.; Roque, I. L. V.; Saxena, A.; Scheutwinkel, K. H.; Shen, E.; Sims, P. H.; Smirnov, O.; Spinelli, M.; Zarb-Adami, K.
Source
Journal of Astronomical Instrumentation; March 2022, Vol. 11 Issue: 1
Subject
Language
ISSN
22511717; 22511725
Abstract
Following the reported detection of an absorption profile associated with the 21cm sky-averaged signal from the Cosmic Dawn by the EDGES experiment in 2018, a number of experiments have been set up to verify this result. This paper discusses the design process used for global 21cm experiments, focusing specifically on the Radio Experiment for the Analysis of Cosmic Hydrogen (REACH). This experiment will seek to understand and compensate for systematic errors present using detailed modeling and characterization of the instrumentation. Detailed quantitative figures of merit and numerical modeling are used to assist the design process of the REACH dipole antenna (one of the two antenna designs for REACH Phase I). This design process produced a 2.5:1 frequency bandwidth dipole. The aim of this design was to balance spectral smoothness and low impedance reflections with the ability to describe and understand the antenna response to the sky signal to inform the critically important calibration during observation and data analysis.