Design of Ultra-Wideband Phased Array Feed for Radio Telescope
Paper in proceeding, 2020
This paper presents an ultra-wideband Phased Array Feed (PAF) based on novel flat bend crossed dipole fed by 50Ohm coaxial line. The PAF is dual-polarized and made from all-metal to minimize Ohmic losses and simplify cryogenic integration. It is optimized for 1-2 GHz band and can be good PAF candidate for the Five hundred meter Aperture Spherical Telescope (FAST) and Qi Tai Telescope (QTT) as well as other radio telescopes.
Author
Jin Fan
Chinese Academy of Sciences
Yihua Yan
Chinese Academy of Sciences
Kai Zhu
Chinese Academy of Sciences
Heng Qian Gan
Chinese Academy of Sciences
Linjie Chen
Chinese Academy of Sciences
Jian Yang
Chalmers, Electrical Engineering, Communication, Antennas and Optical Networks
Hailin Cao
Chongqing University
Bin Li
Shanghai Astronomical Observatory
Jun Ma
Chinese Academy of Sciences
2020 33rd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2020
9232362
9789463968003 (ISBN)
33rd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2020
Rome, Italy,
Rome, Italy,
Subject Categories
Astronomy, Astrophysics and Cosmology
Other Physics Topics
Discrete Mathematics
DOI
10.23919/URSIGASS49373.2020.9232362