Abstract
We present the results of a search for astrophysical sources of brief transient neutrino emission using Ice Cube and Deep Core data acquired between 2012 May 15 and 2013 April 30. While the search methods employed in this analysis are similar to those used in previous Ice Cube point source searches, the data set being examined consists of a sample of predominantly sub-TeV muon-neutrinos from the Northern Sky (-5° < δ < 90°) obtained through a novel event selection method. This search represents a first attempt by Ice Cube to identify astrophysical neutrino sources in this relatively unexplored energy range. The reconstructed direction and time of arrival of neutrino events are used to search for any significant self-correlation in the data set. The data revealed no significant source of transient neutrino emission. This result has been used to construct limits at timescales ranging from roughly 1 s to 10 days for generic soft-spectra transients. We also present limits on a specific model of neutrino emission from soft jets in core-collapse supernovae.
| Original language | English (US) |
|---|---|
| Article number | 75 |
| Journal | Astrophysical Journal |
| Volume | 816 |
| Issue number | 2 |
| DOIs | |
| State | Published - Jan 10 2016 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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In: Astrophysical Journal, Vol. 816, No. 2, 75, 10.01.2016.
Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - THE SEARCH for TRANSIENT ASTROPHYSICAL NEUTRINO EMISSION with ICECUBE-DEEPCORE
AU - Aartsen, M. G.
AU - Abraham, K.
AU - Ackermann, M.
AU - Adams, J.
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AU - Terliuk, A.
AU - Tešić, G.
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AU - Toale, P. A.
AU - Tobin, M. N.
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AU - Tselengidou, M.
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AU - Unger, E.
AU - Usner, M.
AU - Vallecorsa, S.
AU - Vandenbroucke, J.
AU - Eijndhoven, N. Van
AU - Vanheule, S.
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AU - Wille, L.
AU - Williams, D. R.
AU - Wissing, H.
AU - Wolf, M.
AU - Wood, T. R.
AU - Woschnagg, K.
AU - Xu, D. L.
AU - Xu, X. W.
AU - Xu, Y.
AU - Yanez, J. P.
AU - Yodh, G.
AU - Yoshida, S.
AU - Zoll, M.
N1 - Funding Information: We acknowledge the support from the following agencies: U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin-Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada, WestGrid and Compute/Calcul Canada; Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom; Marsden Fund, New Zealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Danish National Research Foundation, Denmark (DNRF). Publisher Copyright: © 2016. The American Astronomical Society. All rights reserved.
PY - 2016/1/10
Y1 - 2016/1/10
N2 - We present the results of a search for astrophysical sources of brief transient neutrino emission using Ice Cube and Deep Core data acquired between 2012 May 15 and 2013 April 30. While the search methods employed in this analysis are similar to those used in previous Ice Cube point source searches, the data set being examined consists of a sample of predominantly sub-TeV muon-neutrinos from the Northern Sky (-5° < δ < 90°) obtained through a novel event selection method. This search represents a first attempt by Ice Cube to identify astrophysical neutrino sources in this relatively unexplored energy range. The reconstructed direction and time of arrival of neutrino events are used to search for any significant self-correlation in the data set. The data revealed no significant source of transient neutrino emission. This result has been used to construct limits at timescales ranging from roughly 1 s to 10 days for generic soft-spectra transients. We also present limits on a specific model of neutrino emission from soft jets in core-collapse supernovae.
AB - We present the results of a search for astrophysical sources of brief transient neutrino emission using Ice Cube and Deep Core data acquired between 2012 May 15 and 2013 April 30. While the search methods employed in this analysis are similar to those used in previous Ice Cube point source searches, the data set being examined consists of a sample of predominantly sub-TeV muon-neutrinos from the Northern Sky (-5° < δ < 90°) obtained through a novel event selection method. This search represents a first attempt by Ice Cube to identify astrophysical neutrino sources in this relatively unexplored energy range. The reconstructed direction and time of arrival of neutrino events are used to search for any significant self-correlation in the data set. The data revealed no significant source of transient neutrino emission. This result has been used to construct limits at timescales ranging from roughly 1 s to 10 days for generic soft-spectra transients. We also present limits on a specific model of neutrino emission from soft jets in core-collapse supernovae.
UR - http://www.scopus.com/inward/record.url?scp=84955099522&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84955099522&partnerID=8YFLogxK
U2 - 10.3847/0004-637X/816/2/75
DO - 10.3847/0004-637X/816/2/75
M3 - Article
AN - SCOPUS:84955099522
SN - 0004-637X
VL - 816
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 75
ER -