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23 results on '"Demirors, L."'

1. Search for Neutrino‐induced Cascades from Gamma‐Ray Bursts with AMANDA

Author

Achterberg, A., Ackermann, M., Adams, J., Ahrens, J., Andeen, K., Auffenberg, J., Bahcall, J. N., Bai, X., Baret, B., Barwick, S. W., Bay, R., Beattie, K., Becka, T., Becker, J. K., Becker, K.-H., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Blaufuss, E., Boersma, D. J., Bohm, C., Bolmont, J., Boser, S., Botner, O., Bouchta, A., Braun, J., Burgess, C., Burgess, T., Castermans, T., Chirkin, D., Christy, B., Clem, J., Cowen, D. F., D'Agostino, M. V., Davour, A., Day, C. T., De Clercq, C., Demirors, L., Descamps, F., Desiati, P., DeYoung, T., Diaz-Velez, J. C., Dreyer, J., Dumm, J. P., Duvoort, M. R., Edwards, W. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Evenson, P. A., Fadiran, O., Fazely, A. R., Filimonov, K., Foerster, M. M., Fox, B. D., Franckowiak, A., Gaisser, T. K., Gallagher, J., Ganugapati, R., Geenen, H., Gerhardt, L., Goldschmidt, A., Goodman, J. A., Gozzini, R., Griesel, T., Grullon, S., Gross, A., Gunasingha, R. M., Gurtner, M., Hallgren, A., Halzen, F., Han, K., Hanson, K., Hardtke, D., Hardtke, R., Hart, J. E., Hasegawa, Y., Hauschildt, T., Hays, D., Heise, J., Helbing, K., Hellwig, M., Herquet, P., Hill, G. C., Hodges, J., Hoffman, K. D., Hommez, B., Hoshina, K., Hubert, D., Hughey, B., Hulth, P. O., Hultqvist, K., Hulss, J.-P., Hundertmark, S., Inaba, M., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Jones, A., Joseph, J. M., Kampert, K.-H., Karg, T., Karle, A., Kawai, H., Kelley, J. L., Kitamura, N., Klein, S. R., Klepser, S., Kohnen, G., Kolanoski, H., Kopke, L., Kowalski, M., Kowarik, T., Krasberg, M., Kuehn, K., Labare, M., Landsman, H., Leich, H., Leier, D., Liubarsky, I., Lundberg, J., Lunemann, J., Madsen, J., Mase, K., Matis, H. S., McCauley, T., McParland, C. P., Meli, A., Messarius, T., Meszaros, P., Miyamoto, H., Mokhtarani, A., Montaruli, T., Morey, A., Morse, R., Movit, S. M., Muenich, K., Nahnhauer, R., Nam, J. W., Niessen, P., Nygren, D. R., Ogelman, H., Olivas, A., Patton, S., Pena-Garay, C., Perez de los Heros, C., Piegsa, A., Pieloth, D., Pohl, A. C., Porrata, R., Pretz, J., Price, P. B., Przybylski, G. T., Rawlins, K., Razzaque, S., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Robbins, S., Roth, P., Rott, C., Rutledge, D., Ryckbosch, D., Sander, H.-G., Sarkar, S., Schlenstedt, S., Schmidt, T., Schneider, D., Seckel, D., Semburg, B., Seo, S. H., Seunarine, S., Silvestri, A., Smith, A. J., Solarz, M., Song, C., Sopher, J. E., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Steffen, P., Stezelberger, T., Stokstad, R. G., Stoufer, M. C., Stoyanov, S., Strahler, E. A., Straszheim, T., Sulanke, K.-H., Sullivan, G. W., Sumner, T. J., Taboada, I., Tarasova, O., Tepe, A., Thollander, L., Tilav, S., Tluczykont, M., Toale, P. A., Turcan, D., van Eijndhoven, N., Vandenbroucke, J., Van Overloop, A., Viscomi, V., Voigt, B., Wagner, W., Walck, C., Waldmann, H., Walter, M., Wang, Y.-R., Wendt, C., Wiebusch, C. H., Wikstrom, G., Williams, D. R., Wischnewski, R., Wissing, H., Woschnagg, K., Xu, X. W., Yodh, G., Yoshida, S., Zornoza, J. D., and IceCube Collaboration

Subjects
Gamma rays: bursts, Normalization (statistics), Physics, Range (particle radiation), Muon, Astrophysics::High Energy Astrophysical Phenomena, Neutrinos, Telescopes, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Coincidence, Space and Planetary Science, Cascade, Astronomia, Diffuse flux, High Energy Physics::Experiment, Neutrino, Gamma-ray burst
Abstract

Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 seconds (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E^2 for the Waxman-Bahcall model at 1 PeV is 1.6 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 120 above the theoretical prediction). For this search 90% of the neutrinos would fall in the energy range 50 TeV to 7 PeV. The second analysis looked for neutrino-induced cascades in coincidence with 73 bursts detected by BATSE in the year 2000. The resulting upper limit on the diffuse flux normalization times E^2, also at 1 PeV, is 1.5 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 110 above the theoretical prediction) for the same energy range. The neutrino-induced cascade channel is complementary to the up-going muon channel. We comment on its advantages for searches of neutrinos from GRBs and its future use with IceCube., Comment: 38 pages. 16 postscript figures. Accepted for publication in the Astrophysical Journal

Published
2007
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2. Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data (vol 83, 092003, 2011)

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Brown, A.M., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Daughhetee, J., Davis, J.C., Clercq, C. De, Demirors, L., Denger, T., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Gora, D., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., and Lafebre, S.J.

Subjects
Aetiology, screening and detection [ONCOL 5], GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract

Contains fulltext : 97757.pdf (Publisher’s version ) (Open Access)

Published
2011

3. Constraints on high-energy neutrino emission from SN 2008D

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Davis, J.C., Clercq, C. De, Demirors, L., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Duvoort, M.R., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Helbing, K., Herquet, P., Hickford, S., Hill, G.C., Hoffman, K.D., Homeier, A., Hoshina, K., and Lafebre, S.J.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Experiment, Aetiology, screening and detection [ONCOL 5]
Abstract

Item does not contain fulltext SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and X-ray flashes and a physical connection is widely assumed. This connection could imply that some core collapse supernovae possess mildly relativistic jets in which high-energy neutrinos are produced through proton-proton collisions. The predicted neutrino spectra would be detectable by Cherenkov neutrino detectors like IceCube. A search for a neutrino signal in temporal and spatial correlation with the observed X-ray flash of SN 2008D was conducted using data taken in 2007-2008 with 22 strings of the IceCube detector. Events were selected based on a boosted decision tree classifier trained with simulated signal and experimental background data. The classifier was optimized to the position and a "soft jet" neutrino spectrum assumed for SN 2008D. Using three search windows placed around the X-ray peak, emission time scales from 100-10 000 s were probed. No events passing the cuts were observed in agreement with the signal expectation of 0.13 events. Upper limits on the muon neutrino flux from core collapse supernovae were derived for different emission time scales and the principal model parameters were constrained. While no meaningful limits can be given in the case of an isotropic neutrino emission, the parameter space for a jetted emission can be constrained. Future analyses with the full 86 string IceCube detector could detect up to similar to 100 events for a core-collapse supernova at 10 Mpc according to the soft jet model.

Published
2011

4. Search for a diffuse flux of astrophysical muon neutrinos with the IceCube 40-string detector

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Brown, A.M., Buitink, S., Caballero-Mora, K.S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Daughhetee, J., Davis, J.C., Clercq, C. De, Demirors, L., Denger, T., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Gora, D., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hajismail, A., Hallgren, A., Halzen, F., Han, K., Hanson, K., and Lafebre, S.J.

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment, Aetiology, screening and detection [ONCOL 5]
Abstract

Contains fulltext : 98335.pdf (Publisher’s version ) (Open Access) The IceCube Neutrino Observatory is a 1 km(3) detector currently taking data at the South Pole. One of the main strategies used to look for astrophysical neutrinos with IceCube is the search for a diffuse flux of high-energy neutrinos from unresolved sources. A hard energy spectrum of neutrinos from isotropically distributed astrophysical sources could manifest itself as a detectable signal that may be differentiated from the atmospheric neutrino background by spectral measurement. This analysis uses data from the IceCube detector collected in its half completed configuration which operated between April 2008 and May 2009 to search for a diffuse flux of astrophysical muon neutrinos. A total of 12 877 upward-going candidate neutrino events have been selected for this analysis. No evidence for a diffuse flux of astrophysical muon neutrinos was found in the data set leading to a 90% C. L. upper limit on the normalization of an E(-2) astrophysical nu(mu) flux of 8.9 x 10(-9) GeV cm(-2) s(-1) sr(-1). The analysis is sensitive in the energy range between 35 TeV and 7 PeV. The 12 877 candidate neutrino events are consistent with atmospheric muon neutrinos measured from 332 GeV to 84 TeV and no evidence for a prompt component to the atmospheric neutrino spectrum is found.

Published
2011

5. First search for atmospheric and extraterrestrial neutrino-induced cascades with the IceCube detector

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Brown, A.M., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Daughhetee, J., Davis, J.C., Clercq, C. De, Demirors, L., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., Herquet, P., Hickford, S., and Lafebre, S.J.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Experiment, Aetiology, screening and detection [ONCOL 5]
Abstract

Contains fulltext : 97922.pdf (Publisher’s version ) (Open Access) We report on the first search for atmospheric and for diffuse astrophysical neutrino-induced showers (cascades) in the IceCube detector using 257 days of data collected in the year 2007-2008 with 22 strings active. A total of 14 events with energies above 16 TeV remained after event selections in the diffuse analysis, with an expected total background contribution of 8.3 +/- 3.6. At 90% confidence we set an upper limit of E(2)Phi(90%CL) < 3.6 x 10(-7) GeV.cm(-2).s(-1).sr(-1) on the diffuse flux of neutrinos of all flavors in the energy range between 24 TeV and 6.6 PeV assuming that Phi proportional to E(-2) and the flavor composition of the nu(e):nu(mu):nu(tau) flux is 1:1:1 at the Earth. The atmospheric neutrino analysis was optimized for lower energies. A total of 12 events were observed with energies above 5 TeV. The observed number of events is consistent with the expected background, within the uncertainties.

Published
2011

6. Search for dark matter from the Galactic halo with the IceCube Neutrino Telescope

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Brown, A.M., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Daughhetee, J., Davis, J.C., Clercq, C. De, Demirors, L., Denger, T., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., Herquet, P., and Lafebre, S.J.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Experiment, Astrophysics::Cosmology and Extragalactic Astrophysics, Aetiology, screening and detection [ONCOL 5], Astrophysics::Galaxy Astrophysics
Abstract

Contains fulltext : 96327.pdf (Author’s version preprint ) (Open Access) Contains fulltext : 96327-1.pdf (Publisher’s version ) (Open Access) Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihilation cross section of h similar or equal to 10(-22) cm(3) s(-1) for weakly interacting massive particle masses above 1 TeV, assuming a monochromatic neutrino line spectrum.

Published
2011

7. Erratum: Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data (Physical Review D (2011) 83 (092003))

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J. A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Bay, R., Bazo Alba, J. L., Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K. -H., Benabderrahmane, M. L., Benzvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Brown, A. M., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D. F., D'Agostino, M. V., Danninger, M., Daughhetee, J., Davis, J. C., De Clercq, C., Demirors, L., Denger, T., Depaepe, O., Descamps, F., Desiati, P., De Vries-Uiterweerd, G., Deyoung, T., Diaz-Velez, J. C., Dierckxsens, M., Dreyer, J., Dumm, J. P., Ehrlich, R., Eisch, J., Ellsworth, R. W., Engdegard, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Foerster, M. M., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J. A., Gora, D., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., Herquet, P., Hickford, S., Hill, G. C., Hoffman, K. D., Homeier, A., Hoshina, K., Hubert, D., Huelsnitz, W., Hulss, J. -P., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Joseph, J. M., Kampert, K. -H., Kappes, A., Karg, T., Karle, A., Kelley, J. L., Kenny, P., Kiryluk, J., Kislat, F., Klein, S. R., Kohne, J. -H., Kohnen, G., Kolanoski, H., Kopke, L., Kopper, S., Koskinen, D. J., Kowalski, M., Kowarik, T., Krasberg, M., Krings, T., Kroll, G., Kuwabara, T., Labare, M., Lafebre, S., Laihem, K., Landsman, H., Larson, M. J., Lauer, R., Lunemann, J., Madsen, J., Majumdar, P., Marotta, A., Maruyama, R., Mase, K., Matis, H. S., Meagher, K., Merck, M., Meszaros, P., Meures, T., Middell, E., Milke, N., Miller, J., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Nam, J. W., Naumann, U., Niessen, P., Nygren, D. R., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Ono, M., Panknin, S., Paul, L., Perez De Los Heros, C., Petrovic, J., Piegsa, A., Pieloth, D., Porrata, R., Posselt, J., Price, P. B., Przybylski, G. T., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Rodrigues, J. P., Roth, P., Rothmaier, F., Rott, C., Ruhe, T., Rutledge, D., Ruzybayev, B., Ryckbosch, D., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Schmidt, T., Schonwald, A., Schukraft, A., Schultes, A., Schulz, O., Schunck, M., Seckel, D., Semburg, B., Seo, S. H., Sestayo, Y., Seunarine, S., Silvestri, A., Slipak, A., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stephens, G., Stezelberger, T., Stokstad, R. G., Stossl, A., Stoyanov, S., Strahler, E. A., Straszheim, T., Stur, M., Sullivan, G. W., Swillens, Q., Taavola, H., Taboada, I., Tamburro, A., Tepe, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Tosi, D., Turcan, D., Van Eijndhoven, N., Vandenbroucke, J., Van Overloop, A., Van Santen, J., Vehring, M., Voge, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Weaver, C., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wischnewski, R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., X. W., Xu, Yodh, G., Yoshida, S., and Zarzhitsky, P.

Published
2011

8. Search for relativistic magnetic monopoles with the AMANDA-II neutrino telescope: The IceCube Collaboration

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J. A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Bay, R., Bazo Alba, J. L., Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K. -H., Benabderrahmane, M. L., Benzvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bissok, M., Blaufuss, E., Boersma, D. J., Bohm, C., Boser, S., Botner, O., Bradley, L., Braun, J., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D. F., D'Agostino, M. V., Danninger, M., Davis, J. C., de Clercq, C., Demirors, L., Depaepe, O., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., Deyoung, T., Diaz-Velez, J. C., Dierckxsens, M., Dreyer, J., Dumm, J. P., Duvoort, M. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Engdegard, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Feusels, T., Filimonov, K., Finley, C., Foerster, M. M., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J. A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Helbing, K., Herquet, P., Hickford, S., Hill, G. C., Hoffman, K. D., Homeier, A., Hoshina, K., Hubert, D., Huelsnitz, W., Hulss, J. -P., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Joseph, J. M., Kampert, K. -H., Karg, T., Karle, A., Kelley, J. L., Kemming, N., Kenny, P., Kiryluk, J., Kislat, F., Klein, S. R., Knops, S., Kohne, J. -H., Kohnen, G., Kolanoski, H., Kopke, L., Koskinen, D. J., Kowalski, M., Kowarik, T., Krasberg, M., Krings, T., Kroll, G., Kuehn, K., Kuwabara, T., Labare, M., Lafebre, S., Laihem, K., Landsman, H., Lauer, R., Lehmann, R., Lennarz, D., Lunemann, J., Madsen, J., Majumdar, P., Marotta, A., Maruyama, R., Mase, K., Matis, H. S., Matusik, M., Meagher, K., Merck, M., Meszaros, P., Meures, T., Middell, E., Milke, N., Miller, J., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Nam, J. W., Naumann, U., Niessen, P., Nygren, D. R., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Ono, M., Panknin, S., Paul, L., Perez de los Heros, C., Petrovic, J., Piegsa, A., Pieloth, D., Porrata, R., Posselt, J., Price, P. B., Prikockis, M., Przybylski, G. T., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Rodrigues, J. P., Roth, P., Rothmaier, F., Rott, C., Roucelle, C., Ruhe, T., Rutledge, D., Ruzybayev, B., Ryckbosch, D., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Schlenstedt, S., Schmidt, T., Schukraft, A., Schultes, A., Schulz, O., Schunck, M., Seckel, D., Semburg, B., Seo, S. H., Sestayo, Y., Seunarine, S., Silvestri, A., Slipak, A., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stephens, G., Stezelberger, T., Stokstad, R. G., Stoyanov, S., Strahler, E. A., Straszheim, T., Sullivan, G. W., Swillens, Q., Taavola, H., Taboada, I., Tamburro, A., Tarasova, O., Tepe, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Tosi, D., Turcan, D., van Eijndhoven, N., Vandenbroucke, J., van Overloop, A., van Santen, J., Voge, M., Voigt, B., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Weaver, C., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Wikstrom, G., Williams, D. R., Wischnewski, R., Wissing, H., Wolf, M., Woschnagg, K., Xu, C., X. W., Xu, Yodh, G., Yoshida, S., and Zarzhitsky, P.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Lattice
Abstract

We present the search for Cherenkov signatures from relativistic magnetic monopoles in data taken with the AMANDA-II detector, a neutrino telescope deployed in the Antarctic ice cap at the Geographic South Pole. The non-observation of a monopole signal in data collected during the year 2000 improves present experimental limits on the flux of relativistic magnetic monopoles: Our flux limit varies between 3.8 × 10-17 cm-2 s-1 sr-1 (for monopoles moving at the vacuum speed of light) and 8.8 × 10-16 cm-2 s-1 sr-1 (for monopoles moving at a speed β=v/c=0.76, just above the Cherenkov threshold in ice). These limits apply to monopoles that are energetic enough to penetrate the Earth and enter the detector from below the horizon. The limit obtained for monopoles reaching the detector from above the horizon is less stringent by roughly an order of magnitude, due to the much larger background from down-going atmospheric muons. This looser limit is however valid for a larger class of magnetic monopoles, since the monopoles are not required to pass through the Earth. © 2010 The Author(s).

Published
2010

9. Erratum: Search for high-energy Muon neutrinos from the 'naked-eye' GRB080319b with the icecube neutrino telescope (The Astrophysical Journal (2009) 701 (1721))

Author

Abbasi, R., Abdou, Y., Ackermann, M., Adams, J., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Bay, R., Alba, J. L. B., Beattie, K., Bechet, S., Becker, J. K., Becker, K. -H., Benabderrahmane, M. L., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bissok, M., Blaufuss, E., Boersma, D. J., Bohm, C., Bolmont, J., Boser, S., Botner, O., Bradley, L., Braun, J., Breder, D., Burgess, T., Castermans, T., Chirkin, D., Christy, B., Clem, J., Cohen, S., Cowen, D. F., D'Agostino, M. V., Danninger, M., Day, C. T., De Clercq, C., Demirors, L., Depaepe, O., Descamps, F., Desiati, P., De Vries-Uiterweerd, G., Deyoung, T., Diaz-Velez, J. C., Dreyer, J., Dumm, J. P., Duvoort, M. R., Edwards, W. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Engdegrd, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Feusels, T., Filimonov, K., Finley, C., Foerster, M. M., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Ganugapati, R., Gerhardt, L., Gladstone, L., Goldschmidt, A., Goodman, J. A., Gozzini, R., Grant, D., Griesel, T., Gro, A., Grullon, S., Gunasingha, R. M., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Hasegawa, Y., Heise, J., Helbing, K., Herquet, P., Hickford, S., Hill, G. C., Hoffman, K. D., Hoshina, K., Hubert, D., Huelsnitz, W., Hul, J. -P., Hulth, P. O., Hultqvist, K., Hussain, S., Imlay, R. L., Inaba, M., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Joseph, J. M., Kampert, K. -H., Kappes, A., Karg, T., Karle, A., Kelley, J. L., Kenny, P., Kiryluk, J., Kislat, F., Klein, S. R., Klepser, S., Knops, S., Kohnen, G., Kolanoski, H., Kopke, L., Kowalski, M., Kowarik, T., Krasberg, M., Kuehn, K., Kuwabara, T., Labare, M., Laihem, K., Landsman, H., Lauer, R., Leich, H., Lennarz, D., Lucke, A., Lundberg, J., Lunemann, J., Madsen, J., Majumdar, P., Maruyama, R., Mase, K., Matis, H. S., Mcparland, C. P., Meagher, K., Merck, M., Meszros, P., Middell, E., Milke, N., Miyamoto, H., Mohr, A., Montaruli, T., Morse, R., Movit, S. M., Munich, K., Nahnhauer, R., Nam, J. W., Nieen, P., Nygren, D. R., Odrowski, S., Olivas, A., Olivo, M., Ono, M., Panknin, S., Patton, S., Heros, C. P. D. L., Petrovic, J., Piegsa, A., Pieloth, D., Pohl, A. C., Porrata, R., Potthoff, N., Price, P. B., Prikockis, M., Przybylski, G. T., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Rodrigues, J. P., Roth, P., Rothmaier, F., Rott, C., Roucelle, C., Rutledge, D., Ryckbosch, D., Sander, H. -G., Sarkar, S., Satalecka, K., Schlenstedt, S., Schmidt, T., Schneider, D., Schukraft, A., Schulz, O., Schunck, M., Seckel, D., Semburg, B., Seo, S. H., Sestayo, Y., Seunarine, S., Silvestri, A., Slipak, A., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stephens, G., Stezelberger, T., Stokstad, R. G., Stoufer, M. C., Stoyanov, S., Strahler, E. A., Straszheim, T., Sulanke, K. -H., Sullivan, G. W., Swillens, Q., Taboada, I., Tarasova, O., Tepe, A., Ter-Antonyan, S., Terranova, C., Tilav, S., Tluczykont, M., Toale, P. A., Tosi, D., Turan, D., Van Eijndhoven, N., Vandenbroucke, J., Van Overloop, A., Voigt, B., Walck, C., Waldenmaier, T., Walter, M., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebusch, C. H., Wiedemann, A., Wikstrom, G., Williams, D. R., Wischnewski, R., Wissing, H., Woschnagg, K., X. W., Xu, Yodh, G., and Yoshida, S.

Published
2010

10. Production of the omega meson in the pd --> 3He omega reaction at 1450 MeV and 1360 MeV

Author

Schonning, K., Bargholtz, Chr., Bashkanov, M., Berlowski, M., Bogoslawsky, D., Calen, H., Clement, H., Demirors, L., Ekstrom, C., Fransson, K., Geren, L., Gustafsson, L., Hoistad, B., Ivanov, G., Jacewicz, M., Jiganov, E., Johansson, T., Keleta, S., Khakimova, O., Khemchandani, K. P., Kren, F., Kullander, S., Kupsc, A., Kuzmin, A., Lindberg, K., Marciniewski, P., Morosov, B., Oelert, W., Pauly, C., Petren, H., Petukhov, Y., Povtorejko, A., Ruber, R. J. M. Y., Scobel, W., Shafigullin, R., Shwartz, B., Skorodko, T., Sopov, V., Stepaniak, J., Tegner, P. -E., Engblom, P. Thorngren, Tikhomirov, V., Turowiecki, A., Wagner, G. J., Wilkin, C., Wolke, M., Zabierowski, J., Zartova, I., and Zlomanczuk, J.

Subjects
Nuclear Theory, Nuclear Experiment
Abstract

The production of $\omega$ mesons in the $pd \to{}^3$He$ \omega$ reaction has been studied at two energies near the kinematic threshold, $T_p=1450$ MeV and $T_p=1360$ MeV. The differential cross section was measured as a function of the $\omega$ cm angle at both energies over the whole angular range. Whereas the results at 1360 MeV are consistent with isotropy, strong rises are observed near both the forward and backward directions at 1450 MeV. Calculations made using a two-step model with an intermediate pion fail to reproduce the shapes of the measured angular distributions and also underestimate the total cross sections., Comment: 10 pages, 13 figures

Published
2009

11. Production of the omega meson in the pd -> He-3 omega reaction at 1450 MeV and 1360 MeV

Author

Schonning, K., Bargholtz, C., Bashkanov, M., Berlowski, M., Bogoslawsky, D., Calen, H., Clement, H., Demirors, L., Ekstrom, C., Fransson, K., Geren, L., Gustafsson, L., Hoistad, B., Ivanov, G., Jacewicz, M., Jiganov, E., Johansson, T., Keleta, S., Khakimova, O., Khemchandani, Kanchan P., Kren, F., Kullander, S., Kupsc, A., Kuzmin, A., Lindberg, K., Marciniewski, P., Morosov, B., Oelert, W., Pauly, C., Petren, H., Petukhov, Y., Povtorejko, A., Ruber, Rjmy, Scobel, W., Shafigullin, R., Shwartz, B., Skorodko, T., Sopov, V., Stepaniak, J., Tegner, P. E., Engblom, P. T., Tikhomirov, V., Turowiecki, A., Wagner, G. J., Wilkin, C., Wolke, M., Zabierowski, J., Zartova, I., and Zlomanczuk, J.

Subjects
Nuclear Theory, Nuclear Experiment
Abstract

The production of omega mesons in the pd -> He-3 omega reaction has been studied at two energies near the kinematic threshold, T-p = 1450 MeV and T-p = 1360 MeV. The differential cross section was measured as a function of the omega c.m. angle at both energies over the whole angular range. Whereas the results at 1360 MeV are consistent with isotropy, strong rises are observed near both the forward and backward directions at 1450 MeV. Calculations made using a two-step model with an intermediate pion fail to reproduce the shapes of the measured angular distributions and also underestimate the total cross sections., We wish to thank the personnel at the The Svedberg Laboratory for their support during the course of the experiment. We are grateful to Y. le Bornec for providing us with information regarding Ref. [5] and also V. Shklyar for supplying the t-matrix element of the Giessen model described in Ref. [31]. This work was supported by the European Community under the “Structuring the Research Area” Specific Program Research Infrastructures Action (Hadron Physics, contract no. RII-cT-204-506078) by the Swedish Research Council, and BMBF (06TU201). K.P.K. wishes to thank the Fundacao para a Ciˆencia e a Tecnologia of the Minist´erio da Ciˆencia, Tecnologia e Ensino Superior of Portugal for financial support under Contract No. SFRH/BPD/40309/2007.

Published
2009

12. Exclusive measurement of two-pion production in the dd --> 4Hepipi reaction

Author

Keleta, S., Bargholtz, Chr., Bashkanov, M., Berlowski, M., Bogoslawsky, D., Calen, H., Clement, H., Demirors, L., Ekstrom, C., Fransson, K., Geren, L., Gustafsson, L., Hoistad, B., Ivanov, G., Jacewicz, M., Jiganov, E., Johansson, T., Khakimova, O., Kren, F., Kullander, S., Kupsc, A., Kuzmin, A., Lindberg, K., Marciniewski, P., Morosov, B., Oelert, W., Pauly, C., Petren, H., Petukhov, Y., Povtorejko, A., Pricking, A., Ruber, R. J. M. Y., Schonning, K., Scobel, W., Shafigullin, R., Shwartz, B., Skorodko, T., Sopov, V., Stepaniak, J., Tegner, P. -E., Engblom, P. Thorngren, Tikhomirov, V., Turowiecki, A., Wagner, G. J., Wilkin, C., Wolke, M., Zabierowski, J., Zartova, I., and Zlomanczuk, J.

Subjects
FOS: Physical sciences, Nuclear Experiment (nucl-ex), Nuclear Experiment
Abstract

The results from the first kinematically complete measurement of the dd --> 4Hepipi reaction are reported. The aim was to investigate a long standing puzzle regarding the origin of the peculiar pipi-invariant mass distributions appearing in double pion production in light ion collisions, the so-called ABC effect. The measurements were performed at the incident deuteron energies of 712 MeV and 1029 MeV, with the WASA detector assembly at CELSIUS in Uppsala, Sweden. We report the observation of a characteristic enhancement at low pipi-invariant mass at 712 MeV, the lowest energy yet. At the higher energy, in addition to confirming previous experimental observations, our results reveal a strong angular dependence of the pions in the overall centre of mass system. The results are qualitatively reproduced by a theoretical model, according to which the ABC effect is described as resulting from a kinematical enhancement in the production of the pion pairs from two parallel and independent NN--> dpi sub-processes., 20 pages including 18 figures

Published
2009
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13. Production of the omega meson in the pd --> 3He omega reaction at 1450 MeV and 1360 MeV

Author

Schonning, K., Bargholtz, Chr., Bashkanov, M., Berlowski, M., Bogoslawsky, D., Calen, H., Clement, H., Demirors, L., Ekstrom, C., Fransson, K., Geren, L., Gustafsson, L., Hoistad, B., Ivanov, G., Jacewicz, M., Jiganov, E., Johansson, T., Keleta, S., Khakimova, O., Khemchandani, K. P., Kren, F., Kullander, S., Kupsc, A., Kuzmin, A., Lindberg, K., Marciniewski, P., Morosov, B., Oelert, W., Pauly, C., Petren, H., Petukhov, Y., Povtorejko, A., Ruber, R. J. M. Y., Scobel, W., Shafigullin, R., Shwartz, B., Skorodko, T., Sopov, V., Stepaniak, J., Tegner, P. -E., Engblom, P. Thorngren, Tikhomirov, V., Turowiecki, A., Wagner, G. J., Wilkin, C., Wolke, M., Zabierowski, J., Zartova, I., and Zlomanczuk, J.

Subjects
Nuclear Theory, FOS: Physical sciences, Nuclear Experiment (nucl-ex), Nuclear Experiment
Abstract

The production of $��$ mesons in the $pd \to{}^3$He$ ��$ reaction has been studied at two energies near the kinematic threshold, $T_p=1450$ MeV and $T_p=1360$ MeV. The differential cross section was measured as a function of the $��$ cm angle at both energies over the whole angular range. Whereas the results at 1360 MeV are consistent with isotropy, strong rises are observed near both the forward and backward directions at 1450 MeV. Calculations made using a two-step model with an intermediate pion fail to reproduce the shapes of the measured angular distributions and also underestimate the total cross sections., 10 pages, 13 figures

Published
2009
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14. Polarisation of the omega meson in the pd-->3He+omega reaction at 1360 and 1450 MeV

Author

Schonning, K., Bargholtz, Chr., Bashkanov, M., Berlowski, M., Bogoslawsky, D., Calen, H., Clement, H., Demirors, L., Ekstrom, C., Fransson, K., Geren, L., Gustafsson, L., Hoistad, B., Ivanov, G., Jacewicz, M., Jiganov, E., Johansson, T., Keleta, S., Khakimova, O., Koch, I., Kren, F., Kullander, S., Kupsc, A., Kuzmin, A., Lindberg, K., Marciniewski, P., Morosov, B., Oelert, W., Pauly, C., Pettersson, H., Petukhov, Y., Povtorejko, A., Ruber, R. J. M. Y., Scobel, W., Shafigullin, R., Shwartz, B., Skorodko, T., Sopov, V., Stepaniak, J., Tegner, P. -E., Engblom, P. Thorngren, Tikhomirov, V., Turowiecki, A., Wagner, G. J., Wilkin, C., Wolke, M., Zabierowski, J., Zartova, I., and Zlomanczuk, J.

Subjects
High Energy Physics::Phenomenology, Nuclear Theory, High Energy Physics::Experiment, Nuclear Experiment
Abstract

The tensor polarisation of omega mesons produced in the pd-->3He+omega reaction has been studied at two energies near threshold. The 3He nuclei were detected in coincidence with the pi0pi+pi- or pi0gamma decay products of the omega. In contrast to the case of phi meson production, the omega mesons are found to be unpolarised. This brings into question the applicability of the Okubo-Zweig-Iizuka rule when comparing the production of vector mesons in low energy hadronic reactions., Comment: 11 pages, 4 figures

Published
2008

15. Polarisation of the omega meson in the pd-->3He+omega reaction at 1360 and 1450 MeV

Author

Schonning, K., Bargholtz, Chr., Bashkanov, M., Berlowski, M., Bogoslawsky, D., Calen, H., Clement, H., Demirors, L., Ekstrom, C., Fransson, K., Geren, L., Gustafsson, L., Hoistad, B., Ivanov, G., Jacewicz, M., Jiganov, E., Johansson, T., Keleta, S., Khakimova, O., Koch, I., Kren, F., Kullander, S., Kupsc, A., Kuzmin, A., Lindberg, K., Marciniewski, P., Morosov, B., Oelert, W., Pauly, C., Pettersson, H., Petukhov, Y., Povtorejko, A., Ruber, R. J. M. Y., Scobel, W., Shafigullin, R., Shwartz, B., Skorodko, T., Sopov, V., Stepaniak, J., Tegner, P. -E., Engblom, P. Thorngren, Tikhomirov, V., Turowiecki, A., Wagner, G. J., Wilkin, C., Wolke, M., Zabierowski, J., Zartova, I., and Zlomanczuk, J.

Subjects
High Energy Physics::Phenomenology, Nuclear Theory, FOS: Physical sciences, High Energy Physics::Experiment, Nuclear Experiment (nucl-ex), Nuclear Experiment
Abstract

The tensor polarisation of omega mesons produced in the pd-->3He+omega reaction has been studied at two energies near threshold. The 3He nuclei were detected in coincidence with the pi0pi+pi- or pi0gamma decay products of the omega. In contrast to the case of phi meson production, the omega mesons are found to be unpolarised. This brings into question the applicability of the Okubo-Zweig-Iizuka rule when comparing the production of vector mesons in low energy hadronic reactions., 11 pages, 4 figures

Published
2008
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16. Multiyear search for a diffuse flux of muon neutrinos with AMANDA-II (Physical Review D. Particles, Fields, Gravitation and Cosmology (2007) 76, (042008))

Author

Achterberg, A., Ackermann, M., Adams, J., Ahrens, J., Andeen, K., Auffenberg, J., Bai, X., Baret, B., Barwick, S. W., Bay, R., Beattie, K., Becka, T., Becker, J. K., Becker, K. -H., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Blaufuss, E., Boersma, D. J., Bohm, C., Bolmont, J., Boser, S., Botner, O., Bouchta, A., Braun, J., Burgess, T., Castermans, T., Chirkin, D., Christy, B., Clem, J., Cowen, D. F., D'Agostino, M. V., Davour, A., Day, C. T., De Clercq, C., Demirors, L., Descamps, F., Desiati, P., Deyoung, T., Diaz-Velez, J. C., Dreyer, J., Dumm, J. P., Duvoort, M. R., Edwards, W. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Evenson, P. A., Fadiran, O., Fazely, A. R., Filimonov, K., Finley, C., Foerster, M. M., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Ganugapati, R., Geenen, H., Gerhardt, L., Goldschmidt, A., Goodman, J. A., Gozzini, R., Griesel, T., Gross, A., Grullon, S., Gunasingha, R. M., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Hardtke, D., Hardtke, R., Hart, J. E., Hasegawa, Y., Hauschildt, T., Hays, D., Heise, J., Helbing, K., Hellwig, M., Herquet, P., Hill, G. C., Hodges, J., Hoffman, K. D., Hommez, B., Hoshina, K., Hubert, D., Hughey, B., Hulss, J. -P., Hulth, P. O., Hultqvist, K., Hundertmark, S., Inaba, M., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Jones, A., Joseph, J. M., Kampert, K. -H., Kappes, A., Karg, T., Karle, A., Kawai, H., Kelley, J. L., Kislat, F., Kitamura, N., Klein, S. R., Klepser, S., Kohnen, G., Kolanoski, H., Kopke, L., Kowalski, M., Kowarik, T., Krasberg, M., Kuehn, K., Labare, M., Landsman, H., Lauer, R., Leich, H., Leier, D., Liubarsky, I., Lundberg, J., Lunemann, J., Madsen, J., Maruyama, R., Mase, K., Matis, H. S., Mccauley, T., Mcparland, C. P., Meli, A., Messarius, T., Meszaros, P., Miyamoto, H., Mokhtarani, A., Montaruli, T., Morey, A., Morse, R., Movit, S. M., Munich, K., Nahnhauer, R., Nam, J. W., Niessen, P., Nygren, D. R., Ogelman, H., Olivas, A., Patton, S., Pena-Garay, C., Perez De Los Heros, C., Piegsa, A., Pieloth, D., Pohl, A. C., Porrata, R., Pretz, J., Price, P. B., Przybylski, G. T., Rawlins, K., Razzaque, S., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Robbins, S., Roth, P., Rothmaier, F., Rott, C., Rutledge, D., Ryckbosch, D., Sander, H. -G., Sarkar, S., Satalecka, K., Schlenstedt, S., Schmidt, T., Schneider, D., Seckel, D., Semburg, B., Seo, S. H., Sestayo, Y., Seunarine, S., Silvestri, A., Smith, A. J., Solarz, M., Song, C., Sopher, J. E., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stezelberger, T., Stokstad, R. G., Stoufer, M. C., Stoyanov, S., Strahler, E. A., Straszheim, T., Sulanke, K. -H., Sullivan, G. W., Sumner, T. J., Taboada, I., Tarasova, O., Tepe, A., Thollander, L., Tilav, S., Tluczykont, M., Toale, P. A., Tosi, D., Turcan, D., Van Eijndhoven, N., Vandenbroucke, J., Van Overloop, A., Viscomi, V., Voigt, B., Wagner, W., Walck, C., Waldmann, H., Walter, M., Wang, Y. -R., Wendt, C., Wiebusch, C. H., Wiedemann, C., Wikstrom, G., Williams, D. R., Wischnewski, R., Wissing, H., Woschnagg, K., X. W., Xu, Yodh, G., Yoshida, S., and Zornoza, J. D.

Published
2008

17. Anisotropy in the pion angular distribution of the reaction pp -> pp pi0 at 400 MeV

Author

Engblom, P. Thorngren, Keleta, S. Negasi, Cappellaro, F., Hoistad, B., Jacewicz, M., Johansson, T., Koch, I., Kullander, S., Pettersson, H., Schonning, K., Zlomanczuk, J., Calen, H., Fransson, K., Kupsc, A., Marciniewski, P., Wolke, M., Pauly, C., Demirors, L., Scobel, W., Stepaniak, J., Zabierowski, J., Bashkanov, M., Clement, H., Khakimova, O., Kren, F., and Skorodko, T.

Subjects
FOS: Physical sciences, High Energy Physics::Experiment, Nuclear Experiment (nucl-ex), Nuclear Experiment
Abstract

The reaction pp -> pp pi0 was studied with the WASA detector at the CELSIUS storage ring. The center of mass angular distribution of the pi0 was obtained by detection of the gamma decay products together with the two outgoing protons, and found to be anisotropic with a negative second derivative slope, in agreement with the theoretical predictions from a microscopic calculation., Revtex 4 style, 5 pages 7 figures, PACS numbers:13.60.Le, 13.75.Cs, 21.45.+v, 25.10.+s

Published
2006
Full Text
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18. Constraints on high-energy neutrino emission from SN 2008D

Author

IceCube Collaboration, Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J. A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Bay, R., Alba, J. L. Bazo, Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K. -H., Benabderrahmane, M. L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D. F., D'Agostino, M. V., Danninger, M., Davis, J. C., De Clercq, C., Demirors, L., Depaepe, O., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., DeYoung, T., D\?iaz-Velez, J. C., Dierckxsens, M., Dreyer, J., Dumm, J. P., Duvoort, M. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Foerster, M. M., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Geisler, M., 9, L. Gerhardt, Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J. A., Grant, D., Griesel, T., Groß, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Helbing, K., Herquet, P., Hickford, S., Hill, G. C., Hoffman, K. D., Homeier, A., Hoshina, K., Hubert, D., Huelsnitz, W., Hülß, J. -P., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Joseph, J. M., Kampert, K. -H., Kappes, A., Karg, T., Karle, A., Kelley, J. L., Kemming, N., Kenny, P., Kiryluk, J., Kislat, F., Klein, S. R., Kohne, J. -H., Kohnen, G., Kolanoski, H., Köpke, L., Koskinen, D. J., Kowalski, M., Kowarik, T., Krasberg, M., Krings, T., Kroll, G., Kuehn, K., Kuwabara, T., Labare, M., Lafebre, S., Laihem, K., Landsman, H., Larson, M. J., Lauer, R., Lehmann, R., Lunemann, J., Madsen, J., Majumdar, P., Marotta, A., Maruyama, R., Mase, K., Matis, H. S., Matusik, M., Meagher, K., Merck, M., Mészaros, P., Meures, T., Middell, E., Milke, N., Miller, J., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Nam, J. W., Naumann, U., Nießen, P., Nygren, D. R., Odrowski, S., Olivas, A., Olivo, M., O'Murchadha, A., Ono, M., Panknin, S., Paul18, L., Heros, C. Perez de los, Petrovic, J., Piegsa, A., Pieloth, D., Porrata, R., Posselt, J., Price, P. B., Prikockis, M., Przybylski, G. T., Rawlins, K., Redl, P., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Rodrigues, J. P., Roth, P., Rothmaier, F., Rott, C., Ruhe, T., Rutledge, D., Ruzybayev, B., Ryckbosch, D., Sander, H. -G., Santander, M., Sarkar, S., Schatto, K., Schlenstedt, S., Schmidt, T., Schukraft, A., Schultes, A., Schulz, O., Schunck, M., Seckel, D., Semburg, B., Seo, S. H., Sestayo, Y., Seunarine, S., Silvestri, A., Singh, K., Slipak, A., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stephens, G., Stezelberger, T., Stokstad, R. G., Stoyanov, S., 20, E. A. Strahler, Straszheim16, T., Sullivan16, G. W., Swillens, Q., Taavola, H., Taboada, I., Tamburro, A., Tarasova, O., Tepe, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Tosi, D., Turcan, D., van Eijndhoven, N., Vandenbroucke, J., Van Overloop, A., van Santen, J., Voge, M., Voigt, B., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Weaver, Ch., Wendt1, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Wikstrom, G., Williams, D. R., Wischnewski, R., Wissing, H., Wolf, M., Woschnagg, K., Xu, C., Xu, X. W., Yodh, G., Yoshida, S., and Zarzhitsky, P.

Subjects
TELESCOPE, supernovae, Supernova, MUON NEUTRINOS, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, SN 2008D, Astrophysics, 01 natural sciences, Spectral line, Transient 080109, GAMMA-RAY BURST, individual: SN 2008D [supernovae], Astrophysical jet, ICECUBE DETECTOR, 0103 physical sciences, Muon neutrino, individual, 010306 general physics, Telescope, 010303 astronomy & astrophysics, SUPERNOVA, Cherenkov radiation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Icecube Detector, Muon Neutrinos, supernovae: individual: SN 2008D, neutrinos, Astronomy and Astrophysics, Science General, Type II supernova, Gamma-Ray Burst, MODEL, Neutrino detector, Jet, JET, astroparticle physics, 13. Climate action, Space and Planetary Science, ddc:520, High Energy Physics::Experiment, TRANSIENT 080109, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Model
Abstract

SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and X-ray flashes and a physical connection is widely assumed. This connection could imply that some core collapse supernovae possess mildly relativistic jets in which high-energy neutrinos are produced through proton-proton collisions. The predicted neutrino spectra would be detectable by Cherenkov neutrino detectors like IceCube. A search for a neutrino signal in temporal and spatial correlation with the observed X-ray flash of SN 2008D was conducted using data taken in 2007-2008 with 22 strings of the IceCube detector. Events were selected based on a boosted decision tree classifier trained with simulated signal and experimental background data. The classifier was optimized to the position and a "soft jet" neutrino spectrum assumed for SN 2008D. Using three search windows placed around the X-ray peak, emission time scales from 100 - 10000 s were probed. No events passing the cuts were observed in agreement with the signal expectation of 0.13 events. Upper limits on the muon neutrino flux from core collapse supernovae were derived for different emission time scales and the principal model parameters were constrained., 8 pages

Published
2011
Full Text
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19. Measurement of the atmospheric neutrino energy spectrum from 100 GeV to 400 TeV with IceCube

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Davis, J.C., Clercq, C. De, Demirors, L., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Duvoort, M.R., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Helbing, K., Herquet, P., Hickford, S., Hill, G.C., Hoffman, K.D., Homeier, A., Hoshina, K., and Lafebre, S.J.

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Physics::Accelerator Physics, High Energy Physics::Experiment, Aetiology, screening and detection [ONCOL 5]
Abstract

Contains fulltext : 98086.pdf (Publisher’s version ) (Open Access) A measurement of the atmospheric muon neutrino energy spectrum from 100 GeV to 400 TeV was performed using a data sample of about 18 000 up-going atmospheric muon neutrino events in IceCube. Boosted decision trees were used for event selection to reject misreconstructed atmospheric muons and obtain a sample of up-going muon neutrino events. Background contamination in the final event sample is less than 1%. This is the first measurement of atmospheric neutrinos up to 400 TeV, and is fundamental to understanding the impact of this neutrino background on astrophysical neutrino observations with IceCube. The measured spectrum is consistent with predictions for the atmospheric nu(mu) + (nu) over bar (mu) flux.

Published
2011

20. Limits on Neutrino Emission from Gamma-Ray Bursts with the 40 String IceCube Detector

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Brown, A.M., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Daughhetee, J., Davis, J.C., Clercq, C. De, Demirors, L., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., Herquet, P., Hickford, S., and Lafebre, S.J.

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, High Energy Physics::Experiment, Aetiology, screening and detection [ONCOL 5]
Abstract

Contains fulltext : 98055.pdf (Publisher’s version ) (Open Access) IceCube has become the first neutrino telescope with a sensitivity below the TeV neutrino flux predicted from gamma-ray bursts if gamma-ray bursts are responsible for the observed cosmic-ray flux above 10(18) eV. Two separate analyses using the half-complete IceCube detector, one a dedicated search for neutrinos from p gamma interactions in the prompt phase of the gamma-ray burst fireball and the other a generic search for any neutrino emission from these sources over a wide range of energies and emission times, produced no evidence for neutrino emission, excluding prevailing models at 90% confidence.

Published
2011

21. Contributions to 2nd TeV Particle Astrophysics Conference (TeV PA II). Madison, Wisconsin 28-31 Aug 2006

Author

Achterberg, A., Ackermann, M., Adams, J., Ahrens, J., Andeen, K., Atlee, D. W., Bahcall, J. N., Bai, X., Baret, B., Barwick, S. W., Bay, R., Beattie, K., Becka, T., Becker, J. K., Becker, K. H., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Blaufuss, E., Boersma, D. J., Bohm, C., Bolmont, J., Boeser, Sebastian, Botner, O., Bouchta, A., Braun, J., Burgess, C., Burgess, T., Castermans, T., Chirkin, D., Christy, B., Clem, J., Cowen, D. F., D Agostino, M. V., Davour, A., Day, C. T., Clercq, C., Demirors, L., Descamps, F., Desiati, P., Deyoung, T., Diaz-Velez, J. C., Dreyer, J., Dumm, J. P., Duvoort, M. R., Edwards, W. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Evenson, Paul A., Fadiran, O., Fazely, A. R., Feser, T., Filimonov, K., Fox, B. D., Gaisser, T. K., Gallagher, J., Ganugapati, R., Geenen, Heiko, Gerhardt, L., Goldschmidt, A., Goodman, J. A., Gozzini, R., Grullon, S., Gross, A., Gunasingha, R. M., Gurtner, M., Hallgren, A., Halzen, F., Han, K., Hanson, K., Hardtke, D., Hardtke, R., Harenberg, T., Hart, J. E., Hauschildt, T., Hays, D., Heise, J., Helbing, K., Hellwig, M., Herquet, P., Hill, G. C., Hodges, J., Hoffman, Kara Dion, Hommez, B., Hoshina, K., Hubert, D., Hughey, B., Hulth, P. O., Hultqvist, K., Hundertmark, S., Hulss, J. P., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Jones, A., Joseph, J. M., Kampert, K. H., Karle, A., Kawai, H., Kelley, J. L., Kestel, M., Kitamura, N., Klein, S. R., Klepser, S., Kohnen, G., Kolanoski, H., Kopke, L., Krasberg, M., Kuehn, K., Landsman, H., Leich, H., Leier, D., Leuthold, M., Liubarsky, I., Lundberg, J., Lunemann, J., Madsen, J., Mase, K., Matis, H. S., Thomas McCauley, Mcparland, C. P., Meli, A., Messarius, T., Meszaros, P., Miyamoto, H., Mokhtarani, A., Montaruli, T., Morey, A., Morse, R., Movit, S. M., Munich, K., Nahnhauer, R., Nam, J. W., Niessen, P., Nygren, D. R., Ogelman, H., Olivas, A., Patton, S., Pena-Garay, C., Perez Los Heros, C., Piegsa, A., Pieloth, D., Pohl, A. C., Porrata, R., Pretz, J., Price, P. B., Przybylski, G. T., Rawlins, K., Razzaque, S., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Robbins, S., Roth, P., Rott, C., Rutledge, D., Ryckbosch, D., Sander, H. G., Sarkar, Subir, Schlenstedt, S., Schmidt, T., Schneider, D., Seckel, D., Seo, S. H., Seunarine, S., Silvestri, A., Smith, A. J., Solarz, M., Song, C., Sopher, J. E., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Steffen, P., Stezelberger, T., Stokstad, R. G., Stoufer, M. C., Stoyanov, S., Strahler, E. A., Straszheim, T., Sulanke, K. H., Sullivan, G. W., Sumner, T. J., Taboada, I., Tarasova, O., Tepe, A., Thollander, L., Tilav, S., Tluczykont, M., Toale, P. A., Turcan, D., Eijndhoven, N., Vandenbroucke, J., Overloop, A., Voigt, B., Wagner, W., Walck, C., Waldmann, H., Walter, M., Wang, Y. R., Wendt, C., Wiebusch, C. H., Wikstrom, G., Williams, D. R., Wischnewski, R., Wissing, H., Woschnagg, K., Xu, X. W., Yodh, G., Yoshida, S., and Zornoza, J. D.

22. The IceCube Neutrino Observatory II: All Sky Searches: Atmospheric, Diffuse and EHE

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Allen, M. M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Bay, R., Bazo Alba, J. L., Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K. H., Benabderrahmane, M. L., Benzvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bose, D., Boser, S., Botner, O., Brown, A. M., Buitink, S., Caballero-Mora, K. S., Carson, M., Chirkin, D., Christy, B., Clevermann, F., Cohen, S., Colnard, C., Cowen, D. F., Cruz Silva, A. H., D Agostino, M. V., Danninger, M., Daughhetee, J., Davis, J. C., Clercq, C., Degner, T., Demirors, L., Descamps, F., Desiati, P., Vries-Uiterweerd, G., Deyoung, T., Diaz-Velez, J. C., Dierckxsens, M., Dreyer, J., Dumm, J. P., Dunkman, M., Eisch, J., Ellsworth, R. W., Engdegard, O., Euler, Sebastian, Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, Laura, Glusenkamp, T., Goldschmidt, A., Goodman, J. A., Gora, D., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Homeier, A., Hoshina, K., Huelsnitz, W., Hulss, J. P., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Johansson, H., Kampert, K. H., Kappes, A., Karg, T., Karle, A., Kenny, P., Kiryluk, J., Kislat, F., Klein, S. R., Kohne, J. H., Kohnen, G., Kolanoski, H., Kopke, L., Kopper, S., Koskinen, D. Jason, Kowalski, M., Kowarik, T., Krasberg, M., Krings, T., Kroll, G., Kurahashi, N., Kuwabara, T., Labare, M., Laihem, K., Landsman, H., Larson, M. J., Lauer, R., Lunemann, J., Madsen, J., Marotta, A., Maruyama, R., Mase, K., Matis, H. S., Meagher, K., Merck, M., Meszaros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Nam, J. W., Naumann, U., Nygren, D. R., Odrowski, S., Olivas, A., Olivo, M., O Murchadha, A., Panknin, S., Paul, L., Perez Los Heros, C., Petrovic, J., Piegsa, A., Pieloth, D., Porrata, R., Posselt, J., Price, P. B., Przybylski, G. T., Rawlins, K., Redl, P., Resconi, E., Rhode, Wolfgang, Ribordy, M., Richman, M., Rodrigues, J. P., Rothmaier, F., Rott, C., Ruhe, T., Rutledge, D., Ruzybayev, B., Ryckbosch, D., Sander, H. G., Santander, M., Sarkar, S., Schatto, K., Schmidt, T., Schonwald, A., Schukraft, A., Schultes, A., Schulz, O., Schunck, M., Seckel, D., Semburg, B., Seo, S. H., Sestayo, Y., Seunarine, S., Silvestri, A., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stezelberger, T., Stokstad, R. G., Stossl, A., Strahler, E. A., Strom, R., Stuer, M., Sullivan, G. W., Swillens, Q., Taavola, H., Taboada, I., Tamburro, A., Tepe, A., Samvel Ter-Antonyan, Tilav, S., Toale, P. A., Toscano, S., Tosi, D., Eijndhoven, N., Vandenbroucke, J., Overloop, A., Santen, J., Vehring, M., Voge, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Weaver, C., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wischnewski, R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., and Zoll, M.

23. The IceCube Neutrino Observatory I: Point Source Searches

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Allen, M. M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Bay, R., Bazo Alba, J. L., Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K. H., Benabderrahmane, M. L., Benzvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bose, D., Boser, S., Botner, O., Brown, A. M., Buitink, S., Caballero-Mora, K. S., Carson, M., Chirkin, D., Christy, B., Clevermann, F., Cohen, S., Colnard, C., Cowen, D. F., Cruz Silva, A. H., D Agostino, M. V., Danninger, M., Daughhetee, J., Davis, J. C., Clercq, C., Degner, T., Demirors, L., Descamps, F., Desiati, P., Vries-Uiterweerd, G., Deyoung, T., Diaz-Velez, J. C., Dierckxsens, M., Dreyer, J., Dumm, J. P., Dunkman, M., Eisch, J., Ellsworth, R. W., Engdegard, O., Euler, Sebastian, Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gladstone, Laura, Glusenkamp, T., Goldschmidt, A., Goodman, J. A., Gora, D., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Ismail, A. Haj, Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., Hellauer, R., Hickford, S., Hill, G. C., Hoffman, K. D., Homeier, A., Hoshina, K., Huelsnitz, W., Hulss, J. P., Hulth, P. O., Hultqvist, K., Hussain, S., Ishihara, A., Jacobi, E., Jacobsen, J., Japaridze, G. S., Johansson, H., Kampert, K. H., Kappes, A., Karg, T., Karle, A., Kenny, P., Kiryluk, J., Kislat, F., Klein, S. R., Kohne, J. H., Kohnen, G., Kolanoski, H., Kopke, L., Kopper, S., Koskinen, D. Jason, Kowalski, M., Kowarik, T., Krasberg, M., Krings, T., Kroll, G., Kurahashi, N., Kuwabara, T., Labare, M., Laihem, K., Landsman, H., Larson, M. J., Lauer, R., Lunemann, J., Madsen, J., Marotta, A., Maruyama, R., Mase, K., Matis, H. S., Meagher, K., Merck, M., Meszaros, P., Meures, T., Miarecki, S., Middell, E., Milke, N., Miller, J., Montaruli, T., Morse, R., Movit, S. M., Nahnhauer, R., Nam, J. W., Naumann, U., Nygren, D. R., Odrowski, S., Olivas, A., Olivo, M., O Murchadha, A., Panknin, S., Paul, L., Perez Los Heros, C., Petrovic, J., Piegsa, A., Pieloth, D., Porrata, R., Posselt, J., Price, P. B., Przybylski, G. T., Rawlins, K., Redl, P., Resconi, E., Rhode, Wolfgang, Ribordy, M., Richman, M., Rodrigues, J. P., Rothmaier, F., Rott, C., Ruhe, T., Rutledge, D., Ruzybayev, B., Ryckbosch, D., Sander, H. G., Santander, M., Subir Sarkar, Schatto, K., Schmidt, T., Schonwald, A., Schukraft, A., Schultes, A., Schulz, O., Schunck, M., Seckel, D., Semburg, B., Seo, S. H., Sestayo, Y., Seunarine, S., Silvestri, A., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stezelberger, T., Stokstad, R. G., Stossl, A., Strahler, E. A., Strom, R., Stuer, M., Sullivan, G. W., Swillens, Q., Taavola, H., Taboada, I., Tamburro, A., Tepe, A., Ter-Antonyan, S., Tilav, S., Toale, P. A., Toscano, S., Tosi, D., Eijndhoven, N., Vandenbroucke, J., Overloop, A., Santen, J., Vehring, M., Voge, M., Walck, C., Waldenmaier, T., Wallraff, M., Walter, M., Weaver, C., Wendt, C., Westerhoff, S., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wischnewski, R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, C., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., and Zoll, M.

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