LUNASKA simultaneous neutrino searches with multiple telescopes

The most sensitive method for detecting neutrinos at the very highest energies is the lunar Cherenkov technique, which employs the Moon as a target volume, using conventional radio telescopes to monitor it for nanosecond-scale pulses of Cherenkov radiation from particle cascades in its regolith. Mul...

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Main Authors: Bray, J., Ekers, Ronald, James, C., Roberts, P., Brown, A., Phillips, C., Protheroe, R., Reynolds, J., McFadden, R., Aartsen, M.
Format: Journal Article
Published: 2011
Online Access:http://hdl.handle.net/20.500.11937/22009
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author Bray, J.
Ekers, Ronald
James, C.
Roberts, P.
Brown, A.
Phillips, C.
Protheroe, R.
Reynolds, J.
McFadden, R.
Aartsen, M.
author_facet Bray, J.
Ekers, Ronald
James, C.
Roberts, P.
Brown, A.
Phillips, C.
Protheroe, R.
Reynolds, J.
McFadden, R.
Aartsen, M.
author_sort Bray, J.
building Curtin Institutional Repository
collection Online Access
description The most sensitive method for detecting neutrinos at the very highest energies is the lunar Cherenkov technique, which employs the Moon as a target volume, using conventional radio telescopes to monitor it for nanosecond-scale pulses of Cherenkov radiation from particle cascades in its regolith. Multiple-antenna radio telescopes are difficult to effectively combine into a single detector for this purpose, while single antennas are more susceptible to false events from radio interference, which must be reliably excluded for a credible detection to be made. We describe our progress in excluding such interference in our observations with the single-antenna Parkes radio telescope, and our most recent experiment (taking place the week before the ICRC) using it in conjunction with the Australia Telescope Compact Array, exploiting the advantages of both types of telescope.
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format Journal Article
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T07:41:48Z
publishDate 2011
recordtype eprints
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spelling curtin-20.500.11937-220092017-09-13T13:52:24Z LUNASKA simultaneous neutrino searches with multiple telescopes Bray, J. Ekers, Ronald James, C. Roberts, P. Brown, A. Phillips, C. Protheroe, R. Reynolds, J. McFadden, R. Aartsen, M. The most sensitive method for detecting neutrinos at the very highest energies is the lunar Cherenkov technique, which employs the Moon as a target volume, using conventional radio telescopes to monitor it for nanosecond-scale pulses of Cherenkov radiation from particle cascades in its regolith. Multiple-antenna radio telescopes are difficult to effectively combine into a single detector for this purpose, while single antennas are more susceptible to false events from radio interference, which must be reliably excluded for a credible detection to be made. We describe our progress in excluding such interference in our observations with the single-antenna Parkes radio telescope, and our most recent experiment (taking place the week before the ICRC) using it in conjunction with the Australia Telescope Compact Array, exploiting the advantages of both types of telescope. 2011 Journal Article http://hdl.handle.net/20.500.11937/22009 10.7529/ICRC2011/V04/0240 restricted
spellingShingle Bray, J.
Ekers, Ronald
James, C.
Roberts, P.
Brown, A.
Phillips, C.
Protheroe, R.
Reynolds, J.
McFadden, R.
Aartsen, M.
LUNASKA simultaneous neutrino searches with multiple telescopes
title LUNASKA simultaneous neutrino searches with multiple telescopes
title_full LUNASKA simultaneous neutrino searches with multiple telescopes
title_fullStr LUNASKA simultaneous neutrino searches with multiple telescopes
title_full_unstemmed LUNASKA simultaneous neutrino searches with multiple telescopes
title_short LUNASKA simultaneous neutrino searches with multiple telescopes
title_sort lunaska simultaneous neutrino searches with multiple telescopes
url http://hdl.handle.net/20.500.11937/22009