Subarrays for Phased Aperture Array Radio Telescopes
Journal article, 2025

One of the operation modes established for the new generation radio telescopes, such as SKA-low and LOFAR, is based on the synthesis of subarrays. A subarray consists of a subset of antennas composing an array, or station, of phased array radio telescopes. This operation mode offers larger field of view and shorter baselines meeting some of the scientific requirements. In this contribution, we aim presenting this functionality implemented in the new radio telescopes operating at low frequencies. In particular, we will investigate the effect of the mutual coupling between the antennas nearest to the edge of a subarray and, finally, we present a study focused on the trade-off between the sensitivity and the number of subarrays simultaneously synthesizable within one array of the radio telescope. A Square Kilometre Array prototype operating at low frequencies is taken as case study.

Beamforming

Sensitivity

Mutual coupling

Radio telescope

Phased Aperture Array

Correlated noise

Author

Paola Di Ninni

Arcetri Astrophysical Observatory

Tobia Carozzi

Chalmers, Space, Earth and Environment, Onsala Space Observatory

G. Comoretto

Arcetri Astrophysical Observatory

Proceedings of the International Conference on Electromagnetics in Advanced Applications, ICEAA

28351355 (ISSN) 27662284 (eISSN)

898-903

Subject Categories (SSIF 2025)

Astronomy, Astrophysics, and Cosmology

DOI

10.1109/ICEAA65662.2025.11305784

More information

Latest update

3/19/2026