% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@ARTICLE{Abbasi:490275,
author = {Abbasi, R. and Ackermann, Markus and Adams, J. and Aguilar,
J. A. and Ahlers, M. and Ahrens, M. and Alameddine, J. M.
and Alves, Jr. A. A. and Amin, N. M. and Andeen, K. and
Anderson, T. and Anton, G. and Argüelles, C. and Ashida, Y.
and Athanasiadou, S. and Axani, S. and Bai, X. and
Balagopal, V. A. and Baricevic, M. and Barwick, S. W. and
Basu, V. and Baur, S. and Bay, R. and Beatty, J. J. and
Becker, K.-H. and Becker Tjus, J. and Beise, J. and
Bellenghi, C. and Benda, S. and BenZvi, S. and Berley, D.
and Bernardini, E. and Besson, D. Z. and Binder, G. and
Bindig, D. and Blaufuss, E. and Blot, Summer and Boddenberg,
M. and Bontempo, F. and Book, J. Y. and Borowka, J. and
Böser, S. and Botner, O. and Böttcher, J. and Bourbeau, E.
and Bradascio, F. and Braun, J. and Brinson, B. and Bron, S.
and Brostean-Kaiser, Jannes and Burley, R. T. and Busse, R.
S. and Campana, M. A. and Carnie-Bronca, E. G. and Chen, C.
and Chen, Z. and Chirkin, D. and Choi, K. and Clark, B. A.
and Clark, K. and Classen, L. and Coleman, A. and Collin, G.
H. and Connolly, A. and Conrad, J. M. and Coppin, P. and
Correa, P. and Cowen, D. F. and Cross, R. and Dappen, C. and
Dave, P. and De Clercq, C. and DeLaunay, J. J. and Delgado
López, D. and Dembinski, H. and Deoskar, K. and Desai, A.
and Desiati, P. and de Vries, K. D. and de Wasseige, G. and
DeYoung, T. and Diaz, A. and Díaz-Vélez, J. C. and
Dittmer, M. and Dujmovic, H. and DuVernois, M. A. and
Ehrhardt, T. and Eller, P. and Engel, R. and Erpenbeck, H.
and Evans, J. and Evenson, P. A. and Fan, K. L. and Fazely,
A. R. and Fedynitch, A. and Feigl, N. and Fiedlschuster, S.
and Fienberg, A. T. and Finley, C. and Fischer, Leander and
Fox, D. and Franckowiak, A. and Friedman, E. and Fritz, A.
and Fürst, P. and Gaisser, T. K. and Gallagher, J. and
Ganster, E. and Garcia, A. and Garrappa, Simone and
Gerhardt, L. and Ghadimi, A. and Glaser, C. and Glauch, T.
and Glüsenkamp, T. and Goehlke, N. and Gonzalez, J. G. and
Goswami, S. and Grant, D. and Grégoire, T. and Griswold, S.
and Günther, C. and Gutjahr, P. and Haack, C. and Hallgren,
A. and Halliday, R. and Halve, L. and Halzen, F. and
Hamdaoui, H. and Ha Minh, M. and Hanson, K. and Hardin, J.
and Harnisch, A. A. and Haungs, A. and Helbing, K. and
Hellrung, J. and Henningsen, F. and Hettinger, E. C. and
Heuermann, L. and Hickford, S. and Hignight, J. and Hill, C.
and Hill, G. C. and Hoffman, K. D. and Hoshina, K. and Hou,
W. and Huber, M. and Huber, T. and Hultqvist, K. and
Hünnefeld, M. and Hussain, R. and Hymon, K. and In, S. and
Iovine, N. and Ishihara, A. and Jansson, M. and Japaridze,
G. S. and Jeong, M. and Jin, M. and Jones, B. J. P. and
Kang, D. and Kang, W. and Kang, X. and Kappes, A. and
Kappesser, D. and Kardum, L. and Karg, T. and Karl, M. and
Karle, A. and Katz, U. and Kauer, M. and Kellermann, M. and
Kelley, J. L. and Kheirandish, A. and Kin, K. and Kiryluk,
J. and Klein, S. R. and Kochocki, A. and Koirala, R. and
Kolanoski, H. and Kontrimas, T. and Köpke, L. and Kopper,
C. and Kopper, S. and Koskinen, D. J. and Koundal, P. and
Kovacevich, M. and Kowalski, M. and Kozynets, T. and
Krupczak, E. and Kun, E. and Kurahashi, N. and Lad, Neha
Navnitkumar and Gualda, C. Lagunas and Larson, M. J. and
Lauber, F. and Lazar, J. P. and Lee, J. W. and Leonard, K.
and Leszczyńska, A. and Li, Y. and Lincetto, M. and Liu, Q.
R. and Liubarska, M. and Lohfink, E. and Lozano Mariscal, C.
J. and Lu, L. and Lucarelli, F. and Ludwig, A. and Luszczak,
W. and Lyu, Y. and Ma, Wing Yan and Madsen, J. and Mahn, K.
B. M. and Makino, Y. and Mancina, S. and Sainte, W. Marie
and Mariş, I. C. and Martinez-Soler, I. and Maruyama, R.
and McCarthy, S. and McElroy, T. and McNally, F. and Mead,
J. V. and Meagher, K. and Mechbal, Sarah and Medina, A. and
Meier, M. and Meighen-Berger, S. and Merckx, Y. and
Micallef, J. and Mockler, D. and Montaruli, T. and Moore, R.
W. and Morse, R. and Moulai, M. and Mukherjee, T. and Naab,
Richard and Nagai, R. and Naumann, U. and Necker, J. and
Nguyễn, L. V. and Niederhausen, H. and Nisa, M. U. and
Nowicki, S. C. and Pollmann, A. Obertacke and Oehler, M. and
Oeyen, B. and Olivas, A. and Osborn, J. and O'Sullivan, E.
and Pandya, H. and Pankova, D. V. and Park, N. and Parker,
G. K. and Paudel, E. N. and Paul, L. and de los Heros, C.
Pérez and Peters, L. and Peterson, J. and Philippen, S. and
Pieper, S. and Pizzuto, A. and Plum, M. and Popovych, Y. and
Porcelli, A. and Rodriguez, M. Prado and Pries, B. and
Przybylski, G. T. and Raab, C. and Rack-Helleis, J. and
Raissi, A. and Rameez, M. and Rawlins, K. and Rea, I. C. and
Rechav, Z. and Rehman, A. and Reichherzer, P. and Reimann,
R. and Renzi, G. and Resconi, E. and Reusch, Simeon and
Rhode, W. and Richman, M. and Riedel, B. and Roberts, E. J.
and Robertson, S. and Roellinghoff, G. and Rongen, M. and
Rott, C. and Ruhe, T. and Ryckbosch, D. and Cantu, D.
Rysewyk and Safa, I. and Saffer, J. and Salazar-Gallegos, D.
and Sampathkumar, P. and Herrera, S. E. Sanchez and
Sandrock, A. and Santander, M. and Sarkar, S. and Sarkar, S.
and Satalecka, Konstancja and Schaufel, M. and Schieler, H.
and Schindler, S. and Schmidt, T. and Schneider, A. and
Schneider, J. and Schröder, F. G. and Schumacher, L. and
Schwefer, G. and Sclafani, S. and Seckel, D. and Seunarine,
S. and Sharma, A. and Shefali, S. and Shimizu, N. and Silva,
M. and Skrzypek, B. and Smithers, B. and Snihur, R. and
Soedingrekso, J. and Sogaard, A. and Soldin, D. and
Spannfellner, C. and Spiczak, G. M. and Spiering, Christian
and Stamatikos, M. and Stanev, T. and Stein, Robert and
Stettner, J. and Stezelberger, T. and Stürwald, T. and
Stuttard, T. and Sullivan, G. W. and Taboada, I. and
Ter-Antonyan, S. and Thwaites, J. and Tilav, S. and
Tischbein, F. and Tollefson, K. and Tönnis, C. and Toscano,
S. and Tosi, D. and Trettin, Alexander and Tselengidou, M.
and Tung, C. F. and Turcati, A. and Turcotte, R. and
Twagirayezu, J. P. and Ty, B. and Unland Elorrieta, M. A.
and Upshaw, K. and Valtonen-Mattila, N. and Vandenbroucke,
J. and van Eijndhoven, N. and Vannerom, D. and Santen, Jakob
van and Veitch-Michaelis, J. and Verpoest, S. and Walck, C.
and Wang, W. and Watson, T. B. and Weaver, C. and Weigel, P.
and Weindl, A. and Weldert, J. and Wendt, C. and Werthebach,
J. and Weyrauch, M. and Whitehorn, N. and Wiebusch, C. H.
and Willey, N. and Williams, D. R. and Wolf, M. and Wrede,
G. and Wulff, J. and Xu, X. W. and Yanez, J. P. and
Yildizci, E. and Yoshida, S. and Yu, S. and Yuan, T. and
Zhang, Z. and Zhelnin, P. and Goldstein, Adam and Wood,
Joshua},
collaboration = {{IceCube Collaboration} and Fermi Gamma-ray Burst {Monitor
Collaboration}},
title = {{S}earches for {N}eutrinos from {G}amma-{R}ay {B}ursts
{U}sing the {I}ce{C}ube {N}eutrino {O}bservatory},
reportid = {PUBDB-2022-07608, arXiv:2205.11410},
year = {2022},
note = {ISSN 1538-4357 not unique: **2 hits**.},
abstract = {Gamma-ray bursts (GRBs) are considered as promising sources
of ultra-high-energy cosmic rays (UHECRs) due to their large
power output. Observing a neutrino flux from GRBs would
offer evidence that GRBs are hadronic accelerators of
UHECRs. Previous IceCube analyses, which primarily focused
on neutrinos arriving in temporal coincidence with the
prompt gamma-rays, found no significant neutrino excess. The
four analyses presented in this paper extend the region of
interest to 14 days before and after the prompt phase,
including generic extended time windows and targeted
precursor searches. GRBs were selected between 2011 May and
2018 October to align with the data set of candidate
muon-neutrino events observed by IceCube. No evidence of
correlation between neutrino events and GRBs was found in
these analyses. Limits are set to constrain the contribution
of the cosmic GRB population to the diffuse astrophysical
neutrino flux observed by IceCube. Prompt neutrino emission
from GRBs is limited to $≲1\%$ of the observed diffuse
neutrino flux, and emission on timescales up to 10$^{4}$ s
is constrained to 24\% of the total diffuse flux.},
keywords = {gamma ray: burst (INSPIRE) / cosmic radiation: UHE
(INSPIRE) / neutrino: flux (INSPIRE) / IceCube (INSPIRE) /
observatory (INSPIRE) / accelerator (INSPIRE) / muon
(INSPIRE) / correlation (INSPIRE)},
cin = {$Z_ICE$},
ddc = {520},
cid = {$I:(DE-H253)Z_ICE-20210408$},
pnm = {613 - Matter and Radiation from the Universe (POF4-613)},
pid = {G:(DE-HGF)POF4-613},
experiment = {EXP:(DE-H253)IceCube-20150101},
typ = {PUB:(DE-HGF)25},
eprint = {2205.11410},
howpublished = {arXiv:2205.11410},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2205.11410;\%\%$},
url = {https://bib-pubdb1.desy.de/record/490275},
}