Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

Aartsen, M. G.; Santander, M.; Hill, G. C.; Meagher, K.; Huang, F.; Leonard, K.; Kim, J.; Günder, M.; Kunwar, S.; de André, J. P. A. M.; Nowicki, S. C.; Stettner, J.; Micallef, J.; Cross, R.; Schneider, J.; Lauber, F.; Bourbeau, E.; Backes, P.; Weldert, J.; Hickford, S.; Sandrock, A.; Gerhardt, L.; Westerhoff, S.; Conrad, J. M.; Wandkowsky, N.; Yoshida, S.; Bradascio, F.; Huber, M.; Mase, K.; Meier, M.; Sarkar, S.; Hignight, J.; Blot, S.; Stamatikos, M.; Wood, T. R.; Stachurska, J.; Pandya, H.; Aguilar, J. A.; Palczewski, T.; Pankova, D. V.; Braun, J.; Seunarine, S.; Nahnhauer, R.; Kittler, T.; Pinat, E.; van Santen, J.; Labare, M.; Tenholt, F.; Walck, C.; Moore, R. W.; Halzen, F.; Glauch, T.; Desiati, P.; Eller, P.; Safa, I.; Koirala, R.; Rawlins, K.; Mahn, K. B. M.; Sutherland, M.; Stasik, A.; Andeen, K.; Schumacher, L.; Friedman, E.; BenZvi, S.; Kolanoski, H.; Ty, B.; Turcati, A.; Song, M.; Gündüz, M.; Neer, G.; Luszczak, W.; Rameez, M.; Weiss, M. J.; De Clercq, C.; Meighen-Berger, S.; van Eijndhoven, N.; Anderson, T.; Gallagher, J.; Hünnefeld, M.; Haack, C.; Hoshina, K.; Hoffmann, R.; Sclafani, S.; Schmidt, T.; Wolf, M.; Wendt, C.; van Eijk, D.; de Wasseige, G.; Ahlers, M.; Garrappa, S.; Heereman, D.; Jacobi, E.; Stöß l, A.; Hussain, R.; Naumann, U.; Botner, O.; Gonzalez, J. G.; Unger, E.; Dembinski, H.; Burgman, A.; Xu, X. W.; Stezelberger, T.; Deoskar, K.; Maruyama, R.; Wallraff, M.; Pizzuto, A.; Koskinen, D. J.; Dvorak, E.; Maunu, R.; Rhode, W.; Becker Tjus, J.; Börner, M.; O'Murchadha, A.; Classen, L.; Tosi, D.; Woschnagg, K.; Price, P. B.; Griffith, Z.; Hanson, K.; Przybylski, G. T.; Clark, K.; Finley, C.; O'Sullivan, E.; Dí az-Vélez, J. C.; Satalecka, K.; Hebecker, D.; Makino, Y.; Grant, D.; Kintscher, T.; Chirkin, D.; Schaufel, M.; Medici, M.; Spiczak, G. M.; Argüelles, C.; Wiebe, K.; Beatty, J. J.; Halve, L.; Robertson, S.; Sandroos, J.; Rea, I. C.; Silva, M.; Franckowiak, A.; Vraeghe, M.; Katz, U.; Menne, T.; Ghorbani, K.; Auffenberg, J.; Unland Elorrieta, M. A.; Jeong, M.; Köpke, L.; Wiebusch, C. H.; Niederhausen, H.; Schlunder, P.; Kyriacou, A.; Plum, M.; Momenté, G.; Toscano, S.; Felde, J.; Hultqvist, K.; Karg, T.; Bourbeau, J.; Kiryluk, J.; Kappes, A.; Tselengidou, M.; Eberhardt, B.; Brostean-Kaiser, J.; Kopper, C.; Stuttard, T.; Kopper, S.; Taboada, I.; Bohm, C.; Bron, S.; Meures, T.; Bay, R.; Evenson, P. A.; Relethford, B.; Dunkman, M.; Barbano, A.; Klein, S. R.; Sullivan, G. W.; Steuer, A.; Adams, J.; Kappesser, D.; Nakarmi, P.; Filimonov, K.; Karle, A.; Pérez de los Heros, C.; Goldschmidt, A.; Glüsenkamp, T.; Moulai, M.; Kowalski, M.; Fahey, S.; Soedingrekso, J.; Ackermann, M.; Anton, G.; Kheirandish, A.; Axani, S.; Hallgren, A.; Wood, J.; Snihur, R.; Cowen, D. F.; Becker, K.-H.; Renzi, G.; Stokstad, R. G.; Bagherpour, H.; DeLaunay, J. J.; Mancina, S.; Blaufuss, E.; Henningsen, F.; Ahrens, M.; Yuan, T.; Yodh, G.; Rott, C.; Krings, K.; Turcotte, R.; Usner, M.; Fazely, A. R.; Hellauer, R.; Wallace, A.; Böser, S.; Bernardini, E.; Ström, R.; Larson, M. J.; Stanev, T.; Altmann, D.; Baum, V.; Merino, G.; Iovine, N.; Busse, R. S.; Barwick, S. W.; Binder, G.; Ehrhardt, T.; Berley, D.; DeYoung, T.; Collin, G. H.; Ansseau, I.; Bai, X.; Xu, D. L.; Liu, Q. R.; Pieloth, D.; Mariş, I. C.; Leuermann, M.; Bindig, D.; Rongen, M.; Vandenbroucke, J.; Nygren, D. R.; Raissi, A.; Lozano Mariscal, C. J.; Whelan, B. J.; Miarecki, S.; Tung, C. F.; Medina, A.; Ter-Antonyan, S.; Hoffman, K. D.; Turley, C. F.; Van Driessche, W.; Spiering, C.; Soldin, D.; Kurahashi, N.; Helbing, K.; Watson, T. B.; Seckel, D.; Strotjohann, N. L.; Kauer, M.; Japaridze, G. S.; Vanheule, S.; Correa, P.; Lu, L.; Terliuk, A.; De Ridder, S.; Williams, D. R.; de With, M.; Madsen, J.; Karl, M.; de Vries, K. D.; Montaruli, T.; Schneider, A.; Park, N.; Jones, B. J. P.; Wills, L.; Nagai, R.; Lazar, J. P.; Alispach, C.; Cheung, E.; Xu, Y.; Fritz, A.; Tilav, S.; IceCube Collaboration; Kang, W.; Lünemann, J.; Yanez, J. P.; Weaver, C.; In, S.; Sanchez Herrera, S. E.; Werthebach, J.; Rauch, L.; Mallot, K.; Jero, K.; Olivas, A.; Dave, P.; Whitehorn, N.; Coppin, P.; Peiffer, P.; Rysewyk, D.; Ryckbosch, D.; Chen, C.; Raab, C.; Lucarelli, F.; Dujmovic, H.; Besson, D. Z.; Keivani, A.; Kulacz, N.; Richman, M.; Resconi, E.; Maggi, G.; Obertacke Pollmann, A.; Ishihara, A.; Kelley, J. L.; Lanfranchi, J. L.; Bretz, H.-P.; Ruhe, T.; Hoinka, T.; Tomankova, L.; Krückl, G.; Reimann, R.; Hokanson-Fasig, B.; Carver, T.; Lohfink, E.; Stein, R.; Tönnis, C.; Ganster, E.; Gaisser, T. K.; Wille, L.; Wrede, G.

doi:10.1016/j.astropartphys.2019.102392

000434785 001__ 434785
000434785 005__ 20250729150052.0
000434785 0247_ $$2doi$$a10.1016/j.astropartphys.2019.102392
000434785 0247_ $$2ISSN$$a0927-6505
000434785 0247_ $$2ISSN$$a1873-2852
000434785 0247_ $$2arXiv$$aarXiv:1902.05792
000434785 0247_ $$2datacite_doi$$a10.3204/PUBDB-2020-00328
000434785 0247_ $$2altmetric$$aaltmetric:69620382
000434785 0247_ $$2inspire$$ainspire:1720434
000434785 0247_ $$2WOS$$aWOS:000501416000004
000434785 0247_ $$2openalex$$aopenalex:W2914085126
000434785 037__ $$aPUBDB-2020-00328
000434785 041__ $$aEnglish
000434785 082__ $$a540
000434785 088__ $$2arXiv$$aarXiv:1902.05792
000434785 088__ $$2arXiv$$aarXiv:1902.05792
000434785 0881_ $$aarXiv:1902.05792
000434785 1001_ $$0INSPIRE-00266703$$aAartsen, M. G.$$b0
000434785 245__ $$aNeutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data
000434785 260__ $$aAmsterdam [u.a.]$$bElsevier Science$$c2020
000434785 3367_ $$2DRIVER$$aarticle
000434785 3367_ $$2DataCite$$aOutput Types/Journal article
000434785 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1614077648_26581
000434785 3367_ $$2BibTeX$$aARTICLE
000434785 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000434785 3367_ $$00$$2EndNote$$aJournal Article
000434785 500__ $$a19 pages, 17 figures, 2 tables
000434785 520__ $$aMany 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.
000434785 536__ $$0G:(DE-HGF)POF3-613$$a613 - Matter and Radiation from the Universe (POF3-613)$$cPOF3-613$$fPOF III$$x0
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000434785 650_7 $$2INSPIRE$$amuon: atmosphere
000434785 650_7 $$2INSPIRE$$aatmosphere: background
000434785 650_7 $$2INSPIRE$$aneutrino: flux
000434785 650_7 $$2INSPIRE$$aneutrino: energy
000434785 650_7 $$2INSPIRE$$aIceCube
000434785 650_7 $$2INSPIRE$$agalaxy
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000434785 650_7 $$2autogen$$aNeutrinos
000434785 650_7 $$2autogen$$aPoint sources
000434785 650_7 $$2autogen$$aVeto techniques
000434785 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
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