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@ARTICLE{Abbasi:491465,
author = {Abbasi, R. and Ackermann, Markus and Adams, J. and
Aggarwal, N. and Aguilar, J. A. and Ahlers, 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, Sofia 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 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 Bontempo, F. and Book, J.
Y. and Borowka, J. 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, 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 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 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
Gray, S. J. 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 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
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
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 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
Lincetto, M. and Liu, Q. R. and Liubarska, M. and Lohfink,
E. and Love, C. and Mariscal, C. J. Lozano 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 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 Nayerhoda, A. and Necker, Jannis David and
Neumann, M. and Niederhausen, H. and Nisa, M. U. and Noell,
A. and Nowicki, S. C. and Pollmann, A. Obertacke and Oehler,
M. and Oeyen, B. and Olivas, A. and Orsoe, R. 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 Procter-Murphy, R. and Przybylski, G. T.
and Raab, C. and Rack-Helleis, J. and Rameez, M. 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 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 Savelberg, J. and
Schaufel, M. and Schieler, H. and Schindler, S. and
Schlueter, B. and Schmidt, T. and Schneider, J. and
Schröder, F. G. and Schumacher, L. and Schwefer, G. and
Sclafani, S. 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 Spannfellner, C. and
Spiczak, G. M. and Spiering, Christian 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 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 Verpoest, S. and
Veske, D. 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.},
collaboration = {{IceCube Collaboration}},
title = {{C}onstraints on populations of neutrino sources from
searches in the directions of {I}ce{C}ube neutrino alerts},
reportid = {PUBDB-2023-00174, arXiv:2210.04930},
year = {2022},
note = {22 pages, 9 figures 2 Tables},
abstract = {Beginning in 2016, the IceCube Neutrino Observatory has
sent out alerts in real time containing the information of
high-energy ($E \gtrsim 100$~TeV) neutrino candidate events
with moderate-to-high ($\gtrsim 30$\%) probability of
astrophysical origin. In this work, we use a recent catalog
of such alert events, which, in addition to events announced
in real-time, includes events that were identified
retroactively, and covers the time period of 2011-2020. We
also search for additional, lower-energy, neutrinos from the
arrival directions of these IceCube alerts. We show how
performing such an analysis can constrain the contribution
of rare populations of cosmic neutrino sources to the
diffuse astrophysical neutrino flux. After searching for
neutrino emission coincident with these alert events on
various timescales, we find no significant evidence of
either minute-scale or day-scale transient neutrino emission
or of steady neutrino emission in the direction of these
alert events. This study also shows how numerous a
population of neutrino sources has to be to account for the
complete astrophysical neutrino flux. Assuming sources have
the same luminosity, an $E^{-2.5}$ neutrino spectrum and
number densities that follow star-formation rates, the
population of sources has to be more numerous than $7\times
10^{-9}~\textrm{Mpc}^{-3}$. This number changes to $3\times
10^{-7}~\textrm{Mpc}^{-3}$ if number densities instead have
no cosmic evolution.},
keywords = {neutrino: particle source (INSPIRE) / neutrino: flux
(INSPIRE) / neutrino: spectrum (INSPIRE) / neutrino: energy
spectrum (INSPIRE) / IceCube (INSPIRE) / density (INSPIRE) /
observatory (INSPIRE) / neutrino: VHE (INSPIRE) / neutrino:
UHE (INSPIRE) / TeV (INSPIRE)},
cin = {ZEU-ICE},
cid = {I:(DE-H253)ZEU-ICE-20160806},
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 = {2210.04930},
howpublished = {arXiv:2210.04930},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2210.04930;\%\%$},
doi = {10.3204/PUBDB-2023-00174},
url = {https://bib-pubdb1.desy.de/record/491465},
}
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