Search for high-energy muon neutrinos from the "naked-eye" GRB 080319B with the IceCube neutrino telescope

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Search for high-energy muon neutrinos from the "naked-eye" GRB 080319B with the IceCube neutrino telescope. / Abbasi, R.; Abdou, Y.; Abu-Zayyad, T.; Adams, J.; Aguilar, J.A.; Koskinen, David Jason.

In: Astrophysical Journal, Vol. 701, No. 2, 1721, 02.07.2009.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Abbasi, R, Abdou, Y, Abu-Zayyad, T, Adams, J, Aguilar, JA & Koskinen, DJ 2009, 'Search for high-energy muon neutrinos from the "naked-eye" GRB 080319B with the IceCube neutrino telescope', Astrophysical Journal, vol. 701, no. 2, 1721. https://doi.org/10.1088/0004-637X/701/2/1721

APA

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J. A., & Koskinen, D. J. (2009). Search for high-energy muon neutrinos from the "naked-eye" GRB 080319B with the IceCube neutrino telescope. Astrophysical Journal, 701(2), [1721]. https://doi.org/10.1088/0004-637X/701/2/1721

Vancouver

Abbasi R, Abdou Y, Abu-Zayyad T, Adams J, Aguilar JA, Koskinen DJ. Search for high-energy muon neutrinos from the "naked-eye" GRB 080319B with the IceCube neutrino telescope. Astrophysical Journal. 2009 Jul 2;701(2). 1721. https://doi.org/10.1088/0004-637X/701/2/1721

Author

Abbasi, R. ; Abdou, Y. ; Abu-Zayyad, T. ; Adams, J. ; Aguilar, J.A. ; Koskinen, David Jason. / Search for high-energy muon neutrinos from the "naked-eye" GRB 080319B with the IceCube neutrino telescope. In: Astrophysical Journal. 2009 ; Vol. 701, No. 2.

Bibtex

@article{707eb11532674cd49f88e412eba0a17d,
title = "Search for high-energy muon neutrinos from the {"}naked-eye{"} GRB 080319B with the IceCube neutrino telescope",
abstract = "We report on a search with the IceCube detector for high-energy muon neutrinos from GRB 080319B, one of the brightest gamma-ray bursts (GRBs) ever observed. The fireball model predicts that a mean of 0.1 events should be detected by IceCube for a bulk Lorentz boost of the jet of 300. In both the direct on-time window of 66 s and an extended window of about 300 s around the GRB, no excess was found above background. The 90% CL upper limit on the number of track-like events from the GRB is 2.7, corresponding to a muon neutrino fluence limit of 9.5x10^-3 erg cm^-2 in the energy range between 120 TeV and 2.2 PeV, which contains 90% of the expected events.",
keywords = "astro-ph.HE",
author = "R. Abbasi and Y. Abdou and T. Abu-Zayyad and J. Adams and J.A. Aguilar and Koskinen, {David Jason}",
year = "2009",
month = jul,
day = "2",
doi = "10.1088/0004-637X/701/2/1721",
language = "English",
volume = "701",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Search for high-energy muon neutrinos from the "naked-eye" GRB 080319B with the IceCube neutrino telescope

AU - Abbasi, R.

AU - Abdou, Y.

AU - Abu-Zayyad, T.

AU - Adams, J.

AU - Aguilar, J.A.

AU - Koskinen, David Jason

PY - 2009/7/2

Y1 - 2009/7/2

N2 - We report on a search with the IceCube detector for high-energy muon neutrinos from GRB 080319B, one of the brightest gamma-ray bursts (GRBs) ever observed. The fireball model predicts that a mean of 0.1 events should be detected by IceCube for a bulk Lorentz boost of the jet of 300. In both the direct on-time window of 66 s and an extended window of about 300 s around the GRB, no excess was found above background. The 90% CL upper limit on the number of track-like events from the GRB is 2.7, corresponding to a muon neutrino fluence limit of 9.5x10^-3 erg cm^-2 in the energy range between 120 TeV and 2.2 PeV, which contains 90% of the expected events.

AB - We report on a search with the IceCube detector for high-energy muon neutrinos from GRB 080319B, one of the brightest gamma-ray bursts (GRBs) ever observed. The fireball model predicts that a mean of 0.1 events should be detected by IceCube for a bulk Lorentz boost of the jet of 300. In both the direct on-time window of 66 s and an extended window of about 300 s around the GRB, no excess was found above background. The 90% CL upper limit on the number of track-like events from the GRB is 2.7, corresponding to a muon neutrino fluence limit of 9.5x10^-3 erg cm^-2 in the energy range between 120 TeV and 2.2 PeV, which contains 90% of the expected events.

KW - astro-ph.HE

U2 - 10.1088/0004-637X/701/2/1721

DO - 10.1088/0004-637X/701/2/1721

M3 - Journal article

VL - 701

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 1721

ER -

ID: 98038284