% 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:585987,
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 Chau, N. 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, 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
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 Heyer,
N. 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
Khatee Zathul, A. 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, 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 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 Pontén, A. 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, Simeon 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
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 Schlüter, F. 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, Alexander 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 Santen, Jakob van 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-energy {N}eutrino {E}mission from
{S}upernovae with {I}ce{C}ube},
journal = {The astrophysical journal / 2},
volume = {949},
number = {1},
issn = {2041-8205},
address = {London},
publisher = {Institute of Physics Publ.},
reportid = {PUBDB-2023-03726, arXiv:2303.03316},
pages = {L12},
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
as well as 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. All scenarios were tested against the
background expectation and together yield an overall p-value
of $93\%;$ therefore, they show consistency with the
background only. The derived upper limits on the total
energy emitted in neutrinos are 1.7 × 10$^{48}$ erg for
stripped-envelope supernovae, 2.8 × 10$^{48}$ erg for type
IIP, and 1.3 × 10$^{49}$ erg for type IIn SNe, the latter
disfavoring models with optimistic assumptions for neutrino
production in interacting supernovae. We conclude that
stripped-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 = {$Z_ICE$},
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)16},
eprint = {2303.03316},
howpublished = {arXiv:2303.03316},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2303.03316;\%\%$},
UT = {WOS:000992548500001},
doi = {10.3847/2041-8213/acd2c9},
url = {https://bib-pubdb1.desy.de/record/585987},
}
guest ::