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@ARTICLE{Aartsen:207119,
author = {Aartsen, M. G. and Ackermann, Markus and Adams, J. and
Aguilar, J. A. and Ahlers, M. and Ahrens, M. and Altmann, D.
and Anderson, T. and Arguelles, C. and Arlen, T. C. and
Auffenberg, J. and Bai, X. and Barwick, S. W. and Baum, V.
and Beatty, J. J. and Becker Tjus, J. Becker and Becker, K.
-H. and BenZvi, S. and Berghaus, P. and Berley, D. and
Bernardini, E. and Bernhard, A. and Besson, D. Z. and
Binder, G. and Bindig, D. and Bissok, M. and Blaufuss, E.
and Blumenthal, J. and Boersma, D. J. and Bohm, C. and Bos,
F. and Bose, D. and Böser, S. and Botner, O. and Brayeur,
L. and Bretz, Hans-Peter and Brown, A. M. and Casey, J. and
Casier, M. and Cheung, E. and Chirkin, D. and Christov, A.
and Christy, B. and Clark, K. and Classen, L. and
Clevermann, F. and Coenders, S. and Cowen, D. F. and Cruz
Silva, Angel Humberto and Danninger, M. and Daughhetee, J.
and Davis, J. C. and Day, M. and de André, J. P. A. M. and
De Clercq, C. and De Ridder, S. and Desiati, P. and de
Vries, K. D. and de With, M. and DeYoung, T. and
Díaz-Vélez, J. C. and Dunkman, M. and Eagan, R. and
Eberhardt, B. and Eichmann, B. and Eisch, J. and Euler, S.
and Evenson, P. A. and Fadiran, O. and Fazely, A. R. and
Fedynitch, A. and Feintzeig, J. and Felde, J. and Feusels,
T. and Filimonov, K. and Finley, C. and Fischer-Wasels, T.
and Flis, S. and Franckowiak, A. and Frantzen, K. and Fuchs,
T. and Gaisser, T. K. and Gallagher, J. and Gerhardt, L. and
Gier, D. and Gladstone, L. and Glüsenkamp, T. and
Goldschmidt, A. and Golup, G. and Gonzalez, J. G. and
Goodman, J. A. and Góra, D. and Grandmont, D. T. and Grant,
D. and Gretskov, P. and Groh, J. C. and Groß, A. and Ha, C.
and Haack, C. and Ismail, A. Haj and Hallen, P. and
Hallgren, A. and Halzen, F. and Hanson, K. and Hebecker, D.
and Heereman, D. and Heinen, D. and Helbing, K. and
Hellauer, R. and Hellwig, D. and Hickford, S. and Hill, G.
C. and Hoffman, K. D. and Hoffmann, R. and Homeier, A. and
Hoshina, K. and Huang, F. and Huelsnitz, W. and Hulth, P. O.
and Hultqvist, K. and Hussain, S. and Ishihara, A. and
Jacobi, E. and Jacobsen, J. and Jagielski, K. and Japaridze,
G. S. and Jero, K. and Jlelati, O. and Jurkovic, M. and
Kaminsky, B. and Kappes, A. and Karg, T. and Karle, A. and
Kauer, M. and Kelley, J. L. and Kheirandish, A. and Kiryluk,
J. and Kläs, J. and Klein, S. R. and Köhne, J. -H. and
Kohnen, G. and Kolanoski, Hermann and Koob, A. and Köpke,
L. and Kopper, C. and Kopper, S. and Koskinen, D. J. and
Kowalski, M. and Kriesten, A. and Krings, K. and Kroll, G.
and Kroll, M. and Kunnen, J. and Kurahashi, N. and Kuwabara,
T. and Labare, M. and Larsen, D. T. and Larson, M. J. and
Lesiak-Bzdak, M. and Leuermann, M. and Leute, J. and
Lünemann, J. and Macías, O. and Madsen, J. and Maggi, G.
and Maruyama, R. and Mase, K. and Matis, H. S. and Maunu, R.
and McNally, F. and Meagher, K. and Medici, M. and Meli, A.
and Meures, T. and Miarecki, S. and Middell, E. and
Middlemas, E. and Milke, N. and Miller, J. and Mohrmann, L.
and Montaruli, T. and Morse, R. and Nahnhauer, R. and
Naumann, U. and Niederhausen, H. and Nowicki, S. C. and
Nygren, D. R. and Obertacke, A. and Odrowski, S. and Olivas,
A. and Omairat, A. and O'Murchadha, A. and Palczewski, T.
and Paul, L. and Penek, Ö. and Pepper, J. A. and Pérez de
los Heros, C. and Pfendner, C. and Pieloth, D. and Pinat, E.
and Posselt, J. and Price, P. B. and Przybylski, G. T. and
Pütz, J. and Quinnan, M. and Rädel, L. and Rameez, M. and
Rawlins, K. and Redl, P. and Rees, I. and Reimann, R. and
Resconi, E. and Rhode, W. and Richman, M. and Riedel, B. and
Robertson, S. and Rodrigues, J. P. and Rongen, M. and Rott,
C. and Ruhe, T. and Ruzybayev, B. and Ryckbosch, D. and
Saba, S. M. and Sander, H. -G. and Sandroos, J. and
Santander, M. and Sarkar, S. and Schatto, K. and Scheriau,
F. and Schmidt, T. and Schmitz, M. and Schoenen, S. and
Schöneberg, S. and Schönwald, A. and Schukraft, A. and
Schulte, L. and Schulz, O. and Seckel, D. and Sestayo, Y.
and Seunarine, S. and Shanidze, R. and Sheremata, C. and
Smith, M. W. E. and Soldin, D. and Spiczak, G. M. and
Spiering, C. and Stamatikos, M. and Stanev, T. and Stanisha,
N. A. and Stasik, A. and Stezelberger, T. and Stokstad, R.
G. and Stößl, A. and Strahler, E. A. and Ström, R. and
Strotjohann, N. L. and Sullivan, G. W. and Taavola, H. and
Taboada, I. and Tamburro, A. and Tepe, A. and Ter-Antonyan,
S. and Terliuk, A. and Tešić, G. and Tilav, S. and Toale,
P. A. and Tobin, M. N. and Tosi, D. and Tselengidou, M. and
Unger, E. and Usner, M. and Vallecorsa, S. and van
Eijndhoven, N. and Vandenbroucke, J. and van Santen, J. and
Vehring, M. and Voge, M. and Vraeghe, M. and Walck, C. and
Wallraff, M. and Weaver, Ch. and Wellons, M. and Wendt, C.
and Westerhoff, S. and Whelan, B. J. and Whitehorn, N. and
Wichary, C. and Wiebe, K. and Wiebusch, C. H. and Williams,
D. R. and Wissing, H. and Wolf, M. and Wood, T. R. and
Woschnagg, K. and Xu, D. L. and Xu, X. W. and Yanez, J. P.
and Yodh, G. and Yoshida, S. and Zarzhitsky, P. and Ziemann,
J. and Zierke, S. and Zoll, M.},
collaboration = {{IceCube Collaboration}},
title = {{S}earches for {E}xtended and {P}oint-like {N}eutrino
{S}ources with {F}our {Y}ears of {I}ce{C}ube {D}ata},
journal = {The astrophysical journal},
volume = {796},
number = {2},
issn = {1538-4357},
address = {Chicago, Ill. [u.a.]},
publisher = {Univ.11032},
reportid = {PUBDB-2015-01104, arXiv:1406.6757},
pages = {109},
year = {2014},
note = {OA},
abstract = {We present results on searches for point-like sources of
neutrinos using four years of IceCube data, including the
first year of data from the completed 86-string detector.
The total livetime of the combined dataset is 1,373 days.
For an E$^{-2}$ spectrum the median sensitivity at 90\\%
C.L. is $\sim 10^{-12}$ TeV$^{-1}$cm$^{-2}$s$^{-1}$ for
energies between 1 TeV$-$1 PeV in the northern sky and $\sim
10^{-11}$ TeV$^{-1}$cm$^{-2}$s$^{-1}$ for energies between
100 TeV $-$ 100 PeV in the southern sky. The sensitivity has
improved from both the additional year of data and the
introduction of improved reconstructions compared to
previous publications. In addition, we present the first
results from an all-sky search for extended sources of
neutrinos. We update results of searches for neutrino
emission from stacked catalogs of sources, and test five new
catalogs; two of Galactic supernova remnants and three of
active galactic nuclei. In all cases, the data are
compatible with the background-only hypothesis, and upper
limits on the flux of muon neutrinos are reported for the
sources considered.We present results on searches for
point-like sources of neutrinos using four years of IceCube
data, including the first year of data from the completed 86
string detector. The total livetime of the combined data set
is 1373Â days. For an E (â)(2) spectrum, the observed
90\% C.L. flux upper limits are
~10(â)(12)Â TeV(â)(1)Â cm(â)(2)Â s(â)(1)
for energies between 1Â TeV and 1Â PeV in the northern
sky and
~10(â)(11)Â TeV(â)(1)Â cm(â)(2)Â s(â)(1)
for energies between 100Â TeV and 100Â PeV in the
southern sky. This represents a 40\% improvement compared to
previous publications, resulting from both the additional
year of data and the introduction of improved
reconstructions. In addition, we present the first results
from an all-sky search for extended sources of neutrinos. We
update the results of searches for neutrino emission from
stacked catalogs of sources and test five new catalogs, two
of Galactic supernova remnants and three of active galactic
nuclei. In all cases, the data are compatible with the
background-only hypothesis, and upper limits on the flux of
muon neutrinos are reported for the sources considered.},
cin = {ZEU-ICE},
ddc = {520},
cid = {I:(DE-H253)ZEU-ICE-20160806},
pnm = {522 - High-energy neutrino astrophysics (POF2-522)},
pid = {G:(DE-HGF)POF2-522},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)16 / PUB:(DE-HGF)15},
eprint = {1406.6757},
howpublished = {arXiv:1406.6757},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1406.6757;\%\%$},
doi = {10.1088/0004-637X/796/2/109},
url = {https://bib-pubdb1.desy.de/record/207119},
}
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