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@ARTICLE{Abbasi:580606,
author = {Abbasi, R. and Ackermann, M. and Adams, J. and Agarwalla,
S. K. and Aguilar, J. A. and Ahlers, M. and Alameddine, J.
M. and Amin, N. M. and Andeen, K. and Anton, G. and
Argüelles, C. and Ashida, Y. and Athanasiadou, S. and
Axani, S. N. and Bai, X. and Balagopal, V. A. and Baricevic,
M. and Barwick, S. W. and Basu, V. and Bay, R. and Beatty,
J. J. and Becker, K.-H. and Becker Tjus, J. and Beise, J.
and Bellenghi, C. and BenZvi, S. and Berley, D. and
Bernardini, E. and Besson, D. Z. and Binder, G. and Bindig,
D. and Blaufuss, E. and Blot, S. and Bontempo, F. and Book,
J. Y. and Meneguolo, C. Boscolo and Böser, S. and Botner,
O. and Böttcher, J. and Bourbeau, E. and Braun, J. and
Brinson, B. and Brostean-Kaiser, J. and Burley, R. T. and
Busse, R. S. and Butterfield, D. and Campana, M. A. and
Carloni, K. and Carnie-Bronca, E. G. and Chattopadhyay, S.
and Chen, C. and Chen, Z. and Chirkin, D. and Choi, S. and
Clark, B. A. and Classen, L. and Coleman, A. and Collin, G.
H. and Connolly, A. and Conrad, J. M. and Coppin, P. and
Correa, P. and Countryman, S. and Cowen, D. F. 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
Domi, A. 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 Fang, K. and
Fazely, A. R. and Fedynitch, A. and Feigl, N. and
Fiedlschuster, S. 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, S. 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 Gray, S. J. and Griffin, S.
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 Hatch, P. and Haungs,
A. and Helbing, K. and Hellrung, J. and Henningsen, F. and
Heuermann, L. and Hickford, S. and Hidvegi, A. and Hill, C.
and Hill, G. C. and Hoffman, K. D. and Hoshina, K. and Hou,
W. 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 Jacquart, M. and Jansson, M. and Japaridze,
G. S. and Jayakumar, K. 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 Kelley, J.
L. and Zathul, A. Khatee 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 Koskinen, D. J. and Koundal, P. and
Kovacevich, M. and Kowalski, M. and Kozynets, T. and
Kruiswijk, K. and Krupczak, E. and Kumar, Anil and Kun, E.
and Kurahashi, N. and Lad, N. and Lagunas Gualda, C. and
Lamoureux, M. and Larson, M. J. and Lauber, F. and Lazar, J.
P. and Lee, J. W. and Leonard DeHolton, K. and Leszczyńska,
A. and Lincetto, M. and Liu, Q. R. and Liubarska, M. and
Lohfink, E. and Love, C. and Lozano Mariscal, C. J. and Lu,
L. and Lucarelli, F. and Ludwig, A. and Luszczak, W. and
Lyu, Y. and Ma, W. Y. and Madsen, J. and Mahn, K. B. M. and
Makino, Y. and Mancina, S. and Sainte, W. Marie and Mariş,
I. C. and Marka, S. and Marka, Z. and Marsee, M. and
Martinez-Soler, I. and Maruyama, R. and Mayhew, F. and
McElroy, T. and McNally, F. and Mead, J. V. and Meagher, K.
and Mechbal, S. and Medina, A. and Meier, M. and
Meighen-Berger, S. and Merckx, Y. and Merten, L. and
Micallef, J. and Mockler, D. and Montaruli, T. and Moore, R.
W. and Morii, Y. and Morse, R. and Moulai, M. and Mukherjee,
T. and Naab, R. and Nagai, R. and Nakos, M. and Naumann, U.
and Necker, J. and Neumann, M. and Niederhausen, H. and
Nisa, M. U. and Noell, A. and Nowicki, S. C. and Pollmann,
A. Obertacke and O'Dell, V. and Oehler, M. and Oeyen, B. and
Olivas, A. and Orsoe, R. and Osborn, J. and O'Sullivan, E.
and Pandya, H. and Park, N. and Parker, G. K. and Paudel, E.
N. and Paul, L. and de los Heros, C. Pérez and Peterson, J.
and Philippen, S. and Pieper, S. and Pizzuto, A. and Plum,
M. and Popovych, Y. and Rodriguez, M. Prado and Pries, B.
and Procter-Murphy, R. and Przybylski, G. T. and Raab, C.
and Rack-Helleis, J. and Rawlins, K. and Rechav, Z. and
Rehman, A. and Reichherzer, P. and Renzi, G. and Resconi, E.
and Reusch, S. and Rhode, W. and Richman, M. and Riedel, B.
and Roberts, E. J. and Robertson, S. and Rodan, S. and
Roellinghoff, G. and Rongen, M. and Rott, C. and Ruhe, T.
and Ruohan, L. and Ryckbosch, D. and Athanasiadou, S. 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
Savelberg, J. and Savina, P. and Schaufel, M. and Schieler,
H. and Schindler, S. and Schlüter, B. and Schmidt, T. 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 Søgaard, A. and Soldin, D. and
Sommani, G. and Spannfellner, C. and Spiczak, G. M. and
Spiering, C. and Stamatikos, M. and Stanev, T. and Stein,
Robert and Stezelberger, T. and Stürwald, T. and Stuttard,
T. and Sullivan, G. W. and Taboada, I. and Ter-Antonyan, S.
and Thompson, W. G. and Thwaites, J. and Tilav, S. and
Tollefson, K. and Tönnis, C. and Toscano, S. and Tosi, D.
and Trettin, A. and Tung, C. F. and Turcotte, R. and
Twagirayezu, J. P. and Ty, B. and Unland Elorrieta, M. A.
and Upadhyay, A. K. and Upshaw, K. and Valtonen-Mattila, N.
and Vandenbroucke, J. and van Eijndhoven, N. and Vannerom,
D. and van Santen, J. and Vara, J. and Veitch-Michaelis, J.
and Venugopal, M. and Verpoest, S. and Veske, D. and Walck,
C. 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, F. and Yu, S. and Yuan, T. and
Zhang, Z. and Zhelnin, P.},
collaboration = {{IceCube Collaboration}},
title = {{C}onstraining {H}igh-{E}nergy {N}eutrino {E}mission from
{S}upernovae with {I}ce{C}ube},
reportid = {PUBDB-2023-01341, arXiv:2303.03316},
year = {2023},
note = {Submitted to ApJ Letters},
abstract = {Core-collapse supernovae are a promising potential
high-energy neutrino source class. We test for correlation
between seven years of IceCube neutrino data and a catalog
containing more than 1000 core-collapse supernovae of types
IIn and IIP and a sample of stripped-envelope supernovae. We
search both for neutrino emission from individual
supernovae, and for combined emission from the whole
supernova sample through a stacking analysis. No significant
spatial or temporal correlation of neutrinos with the
cataloged supernovae was found. The overall deviation of all
tested scenarios from the background expectation yields a
p-value of $93\%$ which is fully compatible with background.
The derived upper limits on the total energy emitted in
neutrinos are $1.7\times 10^{48}$ erg for stripped-envelope
supernovae, $2.8\times 10^{48}$ erg for type IIP, and
$1.3\times 10^{49}$ erg for type IIn SNe, the latter
disfavouring models with optimistic assumptions for neutrino
production in interacting supernovae. We conclude that
strippe-envelope supernovae and supernovae of type IIn do
not contribute more than $14.6\\%$ and $33.9\\%$
respectively to the diffuse neutrino flux in the energy
range of about $10^3-10^5$ GeV, assuming that the neutrino
energy spectrum follows a power-law with an index of $-2.5$.
Under the same assumption, we can only constrain the
contribution of type IIP SNe to no more than $59.9\\%$. Thus
core-collapse supernovae of types IIn and stripped-envelope
supernovae can both be ruled out as the dominant source of
the diffuse neutrino flux under the given assumptions.},
keywords = {neutrino: flux (INSPIRE) / neutrino: particle source
(INSPIRE) / neutrino: energy spectrum (INSPIRE) / energy:
emission (INSPIRE) / neutrino: production (INSPIRE) /
supernova (INSPIRE) / background (INSPIRE) / correlation
(INSPIRE) / collapse (INSPIRE) / IceCube (INSPIRE) / GeV
(INSPIRE) / stacking (INSPIRE) / neutrino: VHE (INSPIRE) /
neutrino: UHE (INSPIRE) / neutrino: luminosity (INSPIRE) /
neutrino: energy (INSPIRE)},
cin = {$Z_ICE$},
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 = {2303.03316},
howpublished = {arXiv:2303.03316},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2303.03316;\%\%$},
doi = {10.3204/PUBDB-2023-01341},
url = {https://bib-pubdb1.desy.de/record/580606},
}
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