Eight-meter-wavelength Transient Array (ETA)



Overview: The Eight-meter-wavelength Transient Array (ETA) is a joint project of Virginia Tech Departments of Electrical & Computer Engineering and Physics. ETA is a radio telescope array operating in the band 29-47 MHz that continuously monitors virtually the entire sky for transients from a variety of high-energy astrophysical phenomena including primordial black holes, gamma ray bursts, supernovae, and compact object mergers. It is supported through an NSF Advanced Techniques & Instrumentation (ATI) grant and was hosted at the Pisgah Astronomical Research Institute (PARI) near Balsam Grove, NC from 2005 through 2008. A new mobile version of ETA is currently under construction. ETA people at VT currently include: Steve Ellingson (ECE), Cameron Patterson (ECE), John Simonetti (Physics), and students.

Quick Primer on ETA: We suggest starting with our URSI NRSM presentation "Searching for Low Frequency Radio Transients Using ETA" (Jan 2008) and also a recent Nature article "Astronomers look for exploding black holes: Extra dimensions in spacetime could trigger blast", Nature News [online], 1 Feb 2008. Then check out "Last 5 Updates", below.

This page is http://www.ece.vt.edu/swe/eta/
Maintainer: Steve Ellingson
Last 5 Updates:
2008 Nov 05: Added JCAP paper, also minor editing.
2008 Oct 19: Added ACM TRETS paper; also minor editing.
2008 Feb 02: Added reference to recent PBH articles in astro-ph and Nature Online.
2008 Jan 03: Added URSI 2008 NRSM (Boulder CO) presentation.
2007 Mar 25: Added FPL 2007 paper submission.


Table of Contents


Publications

In reverse chronological order.


Presentations

In reverse chronological order.


ETA People

Currently active: Past Contributors:


Test Reports & Progress

In reverse chronological order.


Design Info

In no particular order... warning: becoming badly out of date.


Media Stories About ETA

In reverse chronological order. In reverse chronological order.


NSF Acknowledgment and Disclaimer

This material is based upon work supported by the National Science Foundation under Grant No. AST-0504677. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.