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@ARTICLE{Aartsen:434785,
author = {Aartsen, M. G. and Ackermann, M. and Adams, J. and Aguilar,
J. A. and Ahlers, M. and Ahrens, M. and Alispach, C. and
Altmann, D. and Andeen, K. and Anderson, T. and Ansseau, I.
and Anton, G. and Argüelles, C. and Auffenberg, J. and
Axani, S. and Backes, P. and Bagherpour, H. and Bai, X. and
Barbano, A. and Barwick, S. W. and Baum, V. and Bay, R. and
Beatty, J. J. and Becker, K.-H. and Becker Tjus, J. 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 Bohm, C. and Börner, M. and Böser, S. and Botner,
O. and Bourbeau, E. and Bourbeau, J. and Bradascio, F. and
Braun, J. and Bretz, H.-P. and Bron, S. and Brostean-Kaiser,
J. and Burgman, A. and Busse, R. S. and Carver, T. and Chen,
C. and Cheung, E. and Chirkin, D. and Clark, K. and Classen,
L. and Collin, G. H. and Conrad, J. M. and Coppin, P. and
Correa, P. and Cowen, D. F. and Cross, R. and Dave, P. and
de André, J. P. A. M. and De Clercq, C. and DeLaunay, J. J.
and Dembinski, H. and Deoskar, K. and De Ridder, S. and
Desiati, P. and de Vries, K. D. and de Wasseige, G. and de
With, M. and DeYoung, T. and Dí az-Vélez, J. C. and
Dujmovic, H. and Dunkman, M. and Dvorak, E. and Eberhardt,
B. and Ehrhardt, T. and Eller, P. and Evenson, P. A. and
Fahey, S. and Fazely, A. R. and Felde, J. and Filimonov, K.
and Finley, C. and Franckowiak, A. and Friedman, E. and
Fritz, A. and Gaisser, T. K. and Gallagher, J. and Ganster,
E. and Garrappa, S. and Gerhardt, L. and Ghorbani, K. and
Glauch, T. and Glüsenkamp, T. and Goldschmidt, A. and
Gonzalez, J. G. and Grant, D. and Griffith, Z. and Günder,
M. and Gündüz, M. and Haack, C. and Hallgren, A. and
Halve, L. and Halzen, F. and Hanson, K. and Hebecker, D. and
Heereman, D. and Helbing, K. and Hellauer, R. and
Henningsen, F. and Hickford, S. and Hignight, J. and Hill,
G. C. and Hoffman, K. D. and Hoffmann, R. and Hoinka, T. and
Hokanson-Fasig, B. and Hoshina, K. and Huang, F. and Huber,
M. and Hultqvist, K. and Hünnefeld, M. and Hussain, R. and
In, S. and Iovine, N. and Ishihara, A. and Jacobi, E. and
Japaridze, G. S. and Jeong, M. and Jero, K. and Jones, B. J.
P. and Kang, W. and Kappes, A. and Kappesser, D. and Karg,
T. and Karl, M. and Karle, A. and Katz, U. and Kauer, M. and
Keivani, A. and Kelley, J. L. and Kheirandish, A. and Kim,
J. and Kintscher, T. and Kiryluk, J. and Kittler, T. and
Klein, S. R. and Koirala, R. and Kolanoski, H. and Köpke,
L. and Kopper, C. and Kopper, S. and Koskinen, D. J. and
Kowalski, M. and Krings, K. and Krückl, G. and Kulacz, N.
and Kunwar, S. and Kurahashi, N. and Kyriacou, A. and
Labare, M. and Lanfranchi, J. L. and Larson, M. J. and
Lauber, F. and Lazar, J. P. and Leonard, K. and Leuermann,
M. and Liu, Q. R. and Lohfink, E. and Lozano Mariscal, C. J.
and Lu, L. and Lucarelli, F. and Lünemann, J. and Luszczak,
W. and Madsen, J. and Maggi, G. and Mahn, K. B. M. and
Makino, Y. and Mallot, K. and Mancina, S. and Mariş, I. C.
and Maruyama, R. and Mase, K. and Maunu, R. and Meagher, K.
and Medici, M. and Medina, A. and Meier, M. and
Meighen-Berger, S. and Menne, T. and Merino, G. and Meures,
T. and Miarecki, S. and Micallef, J. and Momenté, G. and
Montaruli, T. and Moore, R. W. and Moulai, M. and Nagai, R.
and Nahnhauer, R. and Nakarmi, P. and Naumann, U. and Neer,
G. and Niederhausen, H. and Nowicki, S. C. and Nygren, D. R.
and Obertacke Pollmann, A. and Olivas, A. and O'Murchadha,
A. and O'Sullivan, E. and Palczewski, T. and Pandya, H. and
Pankova, D. V. and Park, N. and Peiffer, P. and Pérez de
los Heros, C. and Pieloth, D. and Pinat, E. and Pizzuto, A.
and Plum, M. and Price, P. B. and Przybylski, G. T. and
Raab, C. and Raissi, A. and Rameez, M. and Rauch, L. and
Rawlins, K. and Rea, I. C. and Reimann, R. and Relethford,
B. and Renzi, G. and Resconi, E. and Rhode, W. and Richman,
M. and Robertson, S. and Rongen, M. and Rott, C. and Ruhe,
T. and Ryckbosch, D. and Rysewyk, D. and Safa, I. and
Sanchez Herrera, S. E. and Sandrock, A. and Sandroos, J. and
Santander, M. and Sarkar, S. and Sarkar, S. and Satalecka,
K. and Schaufel, M. and Schlunder, P. and Schmidt, T. and
Schneider, A. and Schneider, J. and Schumacher, L. and
Sclafani, S. and Seckel, D. and Seunarine, S. and Silva, M.
and Snihur, R. and Soedingrekso, J. and Soldin, D. and Song,
M. and Spiczak, G. M. and Spiering, C. and Stachurska, J.
and Stamatikos, M. and Stanev, T. and Stasik, A. and Stein,
R. and Stettner, J. and Steuer, A. and Stezelberger, T. and
Stokstad, R. G. and Stöß l, A. and Strotjohann, N. L. and
Ström, R. and Stuttard, T. and Sullivan, G. W. and
Sutherland, M. and Taboada, I. and Tenholt, F. and
Ter-Antonyan, S. and Terliuk, A. and Tilav, S. and
Tomankova, L. and Tönnis, C. and Toscano, S. and Tosi, D.
and Tselengidou, M. and Tung, C. F. and Turcati, A. and
Turcotte, R. and Turley, C. F. and Ty, B. and Unger, E. and
Unland Elorrieta, M. A. and Usner, M. and Vandenbroucke, J.
and Van Driessche, W. and van Eijk, D. and van Eijndhoven,
N. and Vanheule, S. and van Santen, J. and Vraeghe, M. and
Walck, C. and Wallace, A. and Wallraff, M. and Wandkowsky,
N. and Watson, T. B. and Weaver, C. and Weiss, M. J. and
Weldert, J. and Wendt, C. and Werthebach, J. and Westerhoff,
S. and Whelan, B. J. and Whitehorn, N. and Wiebe, K. and
Wiebusch, C. H. and Wille, L. and Williams, D. R. and Wills,
L. and Wolf, M. and Wood, J. and Wood, T. R. and Woschnagg,
K. and Wrede, G. and Xu, D. L. and Xu, X. W. and Xu, Y. and
Yanez, J. P. and Yodh, G. and Yoshida, S. and Yuan, T.},
collaboration = {{IceCube Collaboration}},
title = {{N}eutrinos below 100 {T}e{V} from the southern sky
employing refined veto techniques to {I}ce{C}ube data},
journal = {Astroparticle physics},
volume = {116},
issn = {0927-6505},
address = {Amsterdam [u.a.]},
publisher = {Elsevier Science},
reportid = {PUBDB-2020-00328, arXiv:1902.05792. arXiv:1902.05792},
pages = {102392 -},
year = {2020},
note = {19 pages, 17 figures, 2 tables},
abstract = {Many Galactic sources of gamma rays, such as supernova
remnants, are expected to produce neutrinos with a typical
energy cutoff well below 100 TeV. For the IceCube Neutrino
Observatory located at the South Pole, the southern sky,
containing the inner part of the Galactic plane and the
Galactic Center, is a particularly challenging region at
these energies, because of the large background of
atmospheric muons. In this paper, we present recent
advancements in data selection strategies for track-like
muon neutrino events with energies below 100 TeV from the
southern sky. The strategies utilize the outer detector
regions as veto and features of the signal pattern to reduce
the background of atmospheric muons to a level which, for
the first time, allows IceCube searching for point-like
sources of neutrinos in the southern sky at energies between
100 GeV and several TeV in the muon neutrino charged current
channel. No significant clustering of neutrinos above
background expectation was observed in four years of data
recorded with the completed IceCube detector. Upper limits
on the neutrino flux for a number of spectral hypotheses are
reported for a list of astrophysical objects in the southern
hemisphere.},
keywords = {muon: atmosphere (INSPIRE) / atmosphere: background
(INSPIRE) / neutrino: flux (INSPIRE) / neutrino: energy
(INSPIRE) / IceCube (INSPIRE) / galaxy (INSPIRE) / charged
current (INSPIRE) / observatory (INSPIRE) / gamma ray
(INSPIRE) / supernova (INSPIRE) / spectral (INSPIRE) / pole
(INSPIRE) / neutrino muon (INSPIRE) / Neutrinos (autogen) /
Point sources (autogen) / Veto techniques (autogen)},
cin = {ZEU-ICE},
ddc = {540},
cid = {I:(DE-H253)ZEU-ICE-20160806},
pnm = {613 - Matter and Radiation from the Universe (POF3-613)},
pid = {G:(DE-HGF)POF3-613},
experiment = {EXP:(DE-H253)IceCube-20150101},
typ = {PUB:(DE-HGF)16},
eprint = {1902.05792},
howpublished = {arXiv:1902.05792},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1902.05792;\%\%$},
UT = {WOS:000501416000004},
doi = {10.1016/j.astropartphys.2019.102392},
url = {https://bib-pubdb1.desy.de/record/434785},
}
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