Antenna design for the SKA1-LOW and HERA super radio telescopes
arXiv:2003.10733 · doi:10.1109/ICEAA.2018.8520395
Abstract
This paper summarizes the design process and metrics for the latest antenna design for 2 radio telescopes, SKALA4 for the SKA1-LOW instrument and the V-feed for the HERA telescope. In the paper we briefly describe the main features of the antenna element design and the most important figures of merit for both instruments. Finally, we show the response of both designs against some of these figures of merit.
arXiv comment4 pages
References in corpus (4)
- Hydrogen Epoch of Reionization Array (HERA)
- SKALA, a log-periodic array antenna for the SKA-low instrument: design, simulations, tests and system considerations
- The Hydrogen Epoch of Reionization Array Dish II: Characterization of Spectral Structure with Electromagnetic Simulations and its science Implications
- Spectral performance of SKA Log-periodic Antennas I: Mitigating spectral artefacts in SKA1-LOW 21-cm cosmology experiments
Cited by in corpus (5)
- Validation of the HERA Phase I Epoch of Reionization 21 cm Power Spectrum Software Pipeline
- What is the SKA-Low Sensitivity for Your Favourite Radio Source ?
- Probing Compensated Isocurvature with the 21-cm Signal during Cosmic Dawn
- Statistical Detection of IGM Structures during Cosmic Reionization using Absorption of the Redshifted 21 cm line by HI against Compact Background Radio Sources
- Deep learning-driven likelihood-free parameter inference for 21-cm forest observations