Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA)
The Askaryan Radio Array (ARA) is a ground-based radio detector at the South Pole designed to capture Askaryan emission from ultra-high energy neutrinos interacting within the Antarctic ice. The newest ARA station has been equipped with a phased array trigger, in which radio signals in multiple ante...
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Proceedings of Science
2022
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ftucl:oai:eprints.ucl.ac.uk.OAI2:10162516 2023-12-24T10:10:05+01:00 Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA) Hughes, K Allison, P Archambault, S Beatty, JJ Beheler-Amass, M Besson, DZ Beydler, M Chen, CH Chen, YC Chen, P Clark, BA Clay, W Connolly, A Cremonesi, L Dasgupta, P Davies, J de Kockere, S de Vries, KD Deaconu, C DuVernois, MA Flaherty, J Friedman, E Gaior, R Hanson, J Hanson, K Harty, N Hendricks, B Hoffman, KD Hokanson-Fasig, B Hong, E Hsu, SY Huang, JJ Huang, MH Ishihara, A Karle, A Kelley, JL Khandelwal, R Kim, KC Kim, MC Kravchenko, I Krebs, R Ku, Y Kuo, CY Kurusu, K Landsman, H Latif, UA Laundrie, A Liu, TC Lu, MY Madison, B Mase, K Meures, T Nam, J Nichol, RJ Nir, G Novikov, A Nozdrina, A Oberla, E ÓMurchadha, A Osborn, J Pan, Y Pfendner, C Punsuebsay, N Roth, J Sandstrom, P Seckel, D Shiao, YS Shultz, A Smith, D Toscano, S Torres, J Touart, J van Eijndhoven, N Varner, GS Vieregg, A Wang, MZ Wang, SH Wang, YH Wissel, SA Yoshida, S Young, R 2022-03-18 application/pdf https://discovery.ucl.ac.uk/id/eprint/10162516/1/ICRC2021_1153.pdf https://discovery.ucl.ac.uk/id/eprint/10162516/ eng eng Proceedings of Science https://discovery.ucl.ac.uk/id/eprint/10162516/1/ICRC2021_1153.pdf https://discovery.ucl.ac.uk/id/eprint/10162516/ open In: Proceedings of the 37th International Cosmic Ray Conference (ICRC2021). (pp. pp. 1-9). Proceedings of Science (2022) Proceedings paper 2022 ftucl 2023-11-27T13:07:36Z The Askaryan Radio Array (ARA) is a ground-based radio detector at the South Pole designed to capture Askaryan emission from ultra-high energy neutrinos interacting within the Antarctic ice. The newest ARA station has been equipped with a phased array trigger, in which radio signals in multiple antennas are summed in predetermined directions prior to the trigger. In this way, impulsive signals add coherently, while noise likely does not, allowing the trigger threshold to be lower than a traditional ARA station. Early results on just a fraction of available data from this new system prove the feasibility of a low-threshold analysis. Report Antarc* Antarctic South pole South pole University College London: UCL Discovery Antarctic The Antarctic South Pole |
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University College London: UCL Discovery |
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ftucl |
language |
English |
description |
The Askaryan Radio Array (ARA) is a ground-based radio detector at the South Pole designed to capture Askaryan emission from ultra-high energy neutrinos interacting within the Antarctic ice. The newest ARA station has been equipped with a phased array trigger, in which radio signals in multiple antennas are summed in predetermined directions prior to the trigger. In this way, impulsive signals add coherently, while noise likely does not, allowing the trigger threshold to be lower than a traditional ARA station. Early results on just a fraction of available data from this new system prove the feasibility of a low-threshold analysis. |
format |
Report |
author |
Hughes, K Allison, P Archambault, S Beatty, JJ Beheler-Amass, M Besson, DZ Beydler, M Chen, CH Chen, YC Chen, P Clark, BA Clay, W Connolly, A Cremonesi, L Dasgupta, P Davies, J de Kockere, S de Vries, KD Deaconu, C DuVernois, MA Flaherty, J Friedman, E Gaior, R Hanson, J Hanson, K Harty, N Hendricks, B Hoffman, KD Hokanson-Fasig, B Hong, E Hsu, SY Huang, JJ Huang, MH Ishihara, A Karle, A Kelley, JL Khandelwal, R Kim, KC Kim, MC Kravchenko, I Krebs, R Ku, Y Kuo, CY Kurusu, K Landsman, H Latif, UA Laundrie, A Liu, TC Lu, MY Madison, B Mase, K Meures, T Nam, J Nichol, RJ Nir, G Novikov, A Nozdrina, A Oberla, E ÓMurchadha, A Osborn, J Pan, Y Pfendner, C Punsuebsay, N Roth, J Sandstrom, P Seckel, D Shiao, YS Shultz, A Smith, D Toscano, S Torres, J Touart, J van Eijndhoven, N Varner, GS Vieregg, A Wang, MZ Wang, SH Wang, YH Wissel, SA Yoshida, S Young, R |
spellingShingle |
Hughes, K Allison, P Archambault, S Beatty, JJ Beheler-Amass, M Besson, DZ Beydler, M Chen, CH Chen, YC Chen, P Clark, BA Clay, W Connolly, A Cremonesi, L Dasgupta, P Davies, J de Kockere, S de Vries, KD Deaconu, C DuVernois, MA Flaherty, J Friedman, E Gaior, R Hanson, J Hanson, K Harty, N Hendricks, B Hoffman, KD Hokanson-Fasig, B Hong, E Hsu, SY Huang, JJ Huang, MH Ishihara, A Karle, A Kelley, JL Khandelwal, R Kim, KC Kim, MC Kravchenko, I Krebs, R Ku, Y Kuo, CY Kurusu, K Landsman, H Latif, UA Laundrie, A Liu, TC Lu, MY Madison, B Mase, K Meures, T Nam, J Nichol, RJ Nir, G Novikov, A Nozdrina, A Oberla, E ÓMurchadha, A Osborn, J Pan, Y Pfendner, C Punsuebsay, N Roth, J Sandstrom, P Seckel, D Shiao, YS Shultz, A Smith, D Toscano, S Torres, J Touart, J van Eijndhoven, N Varner, GS Vieregg, A Wang, MZ Wang, SH Wang, YH Wissel, SA Yoshida, S Young, R Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA) |
author_facet |
Hughes, K Allison, P Archambault, S Beatty, JJ Beheler-Amass, M Besson, DZ Beydler, M Chen, CH Chen, YC Chen, P Clark, BA Clay, W Connolly, A Cremonesi, L Dasgupta, P Davies, J de Kockere, S de Vries, KD Deaconu, C DuVernois, MA Flaherty, J Friedman, E Gaior, R Hanson, J Hanson, K Harty, N Hendricks, B Hoffman, KD Hokanson-Fasig, B Hong, E Hsu, SY Huang, JJ Huang, MH Ishihara, A Karle, A Kelley, JL Khandelwal, R Kim, KC Kim, MC Kravchenko, I Krebs, R Ku, Y Kuo, CY Kurusu, K Landsman, H Latif, UA Laundrie, A Liu, TC Lu, MY Madison, B Mase, K Meures, T Nam, J Nichol, RJ Nir, G Novikov, A Nozdrina, A Oberla, E ÓMurchadha, A Osborn, J Pan, Y Pfendner, C Punsuebsay, N Roth, J Sandstrom, P Seckel, D Shiao, YS Shultz, A Smith, D Toscano, S Torres, J Touart, J van Eijndhoven, N Varner, GS Vieregg, A Wang, MZ Wang, SH Wang, YH Wissel, SA Yoshida, S Young, R |
author_sort |
Hughes, K |
title |
Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA) |
title_short |
Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA) |
title_full |
Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA) |
title_fullStr |
Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA) |
title_full_unstemmed |
Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA) |
title_sort |
implementing a low-threshold analysis with the askaryan radio array (ara) |
publisher |
Proceedings of Science |
publishDate |
2022 |
url |
https://discovery.ucl.ac.uk/id/eprint/10162516/1/ICRC2021_1153.pdf https://discovery.ucl.ac.uk/id/eprint/10162516/ |
geographic |
Antarctic The Antarctic South Pole |
geographic_facet |
Antarctic The Antarctic South Pole |
genre |
Antarc* Antarctic South pole South pole |
genre_facet |
Antarc* Antarctic South pole South pole |
op_source |
In: Proceedings of the 37th International Cosmic Ray Conference (ICRC2021). (pp. pp. 1-9). Proceedings of Science (2022) |
op_relation |
https://discovery.ucl.ac.uk/id/eprint/10162516/1/ICRC2021_1153.pdf https://discovery.ucl.ac.uk/id/eprint/10162516/ |
op_rights |
open |
_version_ |
1786212978464391168 |