Searching for Extraterrestrial Intelligence with the Square Kilometre Array

@inproceedings{Siemion2014SearchingFE,
  title={Searching for Extraterrestrial Intelligence with the Square Kilometre Array},
  author={Andrew P. V. Siemion and James Gordon Benford and Jin Cheng-jin and Jayanth Chennamangalam and James M. Cordes and David R. DeBoer and Heino Falcke and Michael A. Garrett and Simon T. Garrington and Leonid I. Gurvits and Melvin Hoare and Eric J. Korpela and Joseph Lazio and David G. Messerschmitt and Ian S. Morrison and Tim O'Brien and Zsolt Paragi and Alan John Penny and Laura G. Spitler and Jill Tarter and Dan Werthimer},
  year={2014}
}
AASKA14 : Advancing Astrophysics with the Square Kilometre Array June 8-13, 2014 Giardini Naxos, Italy 

Figures from this paper

AN OPPORTUNISTIC SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE (SETI) WITH THE MURCHISON WIDEFIELD ARRAY

A spectral line image cube generated from 115 minutes of MWA data that covers a field of view of 400 sq, deg. around the Galactic Center is used to perform the first Search for ExtraTerrestrial

GPU-accelerated Signal Processing for Search of Pulsars

TLDR
The accelerated signal processing for the search of radio pulsars recorded by Big Scanning Antenna telescope at Pushchino Radio Astronomy Observatory by parallelization of computations on multiprocessor systems and, especially, on Graphics Processing Units.

SETI OBSERVATIONS OF EXOPLANETS WITH THE ALLEN TELESCOPE ARRAY

We report radio SETI observations on a large number of known exoplanets and other nearby star systems using the Allen Telescope Array (ATA). Observations were made over about 19000 hr from 2009 May

The Search for Extra-Galactic Intelligence Signals Synchronized with Binary Neutron Star Mergers

We discuss the possibility of receiving a radio signal from extra-Galactic intelligence, around the time when we observe a binary neutron star merger in their galaxy. High-precession measurements of

SETI VIA LEAKAGE FROM LIGHT SAILS IN EXOPLANETARY SYSTEMS

The primary challenge of rocket propulsion is the burden of needing to accelerate the spacecraft’s own fuel, resulting in only a logarithmic gain in maximum speed as propellant is added to the

MANTIS: The Mid-Frequency Aperture Array Transient and Intensity-Mapping System

The objective of this paper is to present the main characteristics of a wide-field MFAA precursor that we envisage to be built at the SKA site in South Africa. Known as MANTIS (the Mid-Frequency

Pulsar positioning system: a quest for evidence of extraterrestrial engineering

  • C. Vidal
  • Physics
    International Journal of Astrobiology
  • 2017
Abstract Pulsars have at least two impressive applications. First, they can be used as highly accurate clocks, comparable in stability to atomic clocks; secondly, a small subset of pulsars,

All-sky Radio SETI

TLDR
It is argued 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.

A Search for Optical Laser Emission Using Keck HIRES

We present a search for laser emissions coming from point sources in the vicinity of 2796 stars, including 1368 Kepler objects-of-interest (KOIs) that host one or more exoplanets. We search for

References

SHOWING 1-5 OF 5 REFERENCES

Panoramic Radio Astronomy : Wide-field 1-2 GHz research on galaxy evolution

In this contribution we give a brief overview of the Panoramic Radio Astronomy (PRA) conference held on 2-5 June 2009 in Groningen, the Netherlands. The conference was motivated by the on-going

Note on the Optimum Search Strategy for Uniformly Distributed CW Transmitters. [implications for Project Seti

The relative probability of detecting randomly distributed CW transmitters as a function of the fraction of the sky which is searched (in a fixed time) is given. It is shown that the probability of