All-sky Radio SETI

TL;DR

This paper discusses the development of all-sky radio SETI using aperture arrays like MANTIS, which could significantly enhance the detection of rare and transient extraterrestrial signals at GHz frequencies.

Contribution

It introduces MANTIS as a prototype for all-sky radio SETI, leveraging aperture array technology to improve detection capabilities at GHz frequencies.

Findings

MANTIS enables wide-field, GHz-frequency SETI observations.

Aperture arrays offer advantages for detecting transient signals.

All-sky capability could transform SETI research.

Abstract

Over the last decade, Aperture Arrays (AA) have successfully replaced parabolic dishes as the technology of choice at low radio frequencies - good examples are the MWA, LWA and LOFAR. Aperture Array based telescopes present several advantages, including sensitivity to the sky over a very wide field-of-view. As digital and data processing systems continue to advance, an all-sky capability is set to emerge, even at GHz frequencies. We argue that assuming SETI events are both rare and transitory in nature, an instrument with a large field-of-view, operating around the so-called water-hole (1-2 GHz), might offer several advantages over contemporary searches. Sir Arthur C. Clarke was the first to recognise the potential importance of an all-sky radio SETI capability, as presented in his book, Imperial Earth. As part of the global SKA (Square Kilometre Array) project, a Mid-Frequency Aperture Array (MFAA) prototype known as MANTIS (Mid- Frequency Aperture Array Transient and Intensity-Mapping System) is now being considered as a precursor for SKA-2. MANTIS can be seen as a first step towards an all-sky radio SETI capability at GHz frequencies. This development has the potential to transform the field of SETI research, in addition to several other scientific programmes.