Author: "Desiati, P" / Journal: physical review d - Searchworks@Jio Institute Digital Library Search Results

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42 results on '"Desiati, P"'

1. Characterization of the astrophysical diffuse neutrino flux using starting track events in IceCube

Author: Abbasi, R, Ackermann, M, Adams, J, Agarwalla, SK, Aguilar, JA, Ahlers, M, Alameddine, JM, Amin, NM, Andeen, K, Anton, G, Argüelles, C, Ashida, Y, Athanasiadou, S, Ausborm, L, Axani, SN, Bai, X, Balagopal, A, Baricevic, M, Barwick, SW, Bash, S, Basu, V, Bay, R, Beatty, JJ, Tjus, J Becker, Beise, J, Bellenghi, C, Benning, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Blaufuss, E, Blot, S, Bontempo, F, Book, JY, Meneguolo, C Boscolo, Böser, S, Botner, O, Böttcher, J, Braun, J, Brinson, B, Brostean-Kaiser, J, Brusa, L, Burley, RT, Busse, RS, Butterfield, D, Campana, MA, Caracas, I, Carloni, K, Carpio, J, Chattopadhyay, S, Chau, N, Chen, Z, Chirkin, D, Choi, S, Clark, BA, Coleman, A, Collin, GH, Connolly, A, Conrad, JM, Coppin, P, Corley, R, Correa, P, Cowen, DF, Dave, P, De Clercq, C, DeLaunay, JJ, Delgado, D, Deng, S, Deoskar, K, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, DeYoung, T, Diaz, A, Díaz-Vélez, JC, Dittmer, M, Domi, A, Draper, L, Dujmovic, H, DuVernois, MA, Ehrhardt, T, Eidenschink, L, Eimer, A, Eller, P, Ellinger, E, Mentawi, S El, Elsässer, D, Engel, R, Erpenbeck, H, Evans, J, Evenson, PA, Fan, KL, Fang, K, Farrag, K, Fazely, AR, Fedynitch, A, Feigl, N, and Fiedlschuster, S
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences
Abstract: A measurement of the diffuse astrophysical neutrino spectrum is presented using IceCube data collected from 2011-2022 (10.3 years). We developed novel detection techniques to search for events with a contained vertex and exiting track induced by muon neutrinos undergoing a charged-current interaction. Searching for these starting track events allows us to not only more effectively reject atmospheric muons but also atmospheric neutrino backgrounds in the southern sky, opening a new window to the sub-100 TeV astrophysical neutrino sky. The event selection is constructed using a dynamic starting track veto and machine learning algorithms. We use this data to measure the astrophysical diffuse flux as a single power law flux (SPL) with a best-fit spectral index of γ=2.58-0.09+0.10 and per-flavor normalization of φper-flavorAstro=1.68-0.22+0.19×10-18×GeV-1 cm-2 s-1 sr-1 (at 100 TeV). The sensitive energy range for this dataset is 3-550 TeV under the SPL assumption. This data was also used to measure the flux under a broken power law, however we did not find any evidence of a low energy cutoff.
Published: 2024

2. Search for neutrino lines from dark matter annihilation and decay with IceCube

Author: Abbasi, R, Ackermann, M, Adams, J, Agarwalla, SK, Aguilar, JA, Ahlers, M, Alameddine, JM, Amin, NM, Andeen, K, Anton, G, Argüelles, C, Ashida, Y, Athanasiadou, S, Axani, SN, Bai, X, Balagopal, A, Baricevic, M, Barwick, SW, Basu, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, Beise, J, Bellenghi, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bontempo, F, Book, JY, Meneguolo, C Boscolo, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Braun, J, Brinson, B, Brostean-Kaiser, J, Burley, RT, Busse, RS, Butterfield, D, Campana, MA, Carloni, K, Carnie-Bronca, EG, Chattopadhyay, S, Chau, N, Chen, C, Chen, Z, Chirkin, D, Choi, S, Clark, BA, Classen, L, Coleman, A, Collin, GH, Connolly, A, Conrad, JM, Coppin, P, Correa, P, Countryman, S, Cowen, DF, Dave, P, De Clercq, C, DeLaunay, JJ, López, D Delgado, Dembinski, H, Deoskar, K, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, DeYoung, T, Diaz, A, Díaz-Vélez, JC, Dittmer, M, Domi, A, Dujmovic, H, DuVernois, MA, Ehrhardt, T, Aisati, C El, Eller, P, Engel, R, Erpenbeck, H, Evans, J, Evenson, PA, Fan, KL, Fang, K, Fazely, AR, Fedynitch, A, Feigl, N, Fiedlschuster, S, Finley, C, Fischer, L, Fox, D, and Franckowiak, A
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences
Abstract: Dark matter particles in the Galactic Center and halo can annihilate or decay into a pair of neutrinos producing a monochromatic flux of neutrinos. The spectral feature of this signal is unique and it is not expected from any astrophysical production mechanism. Its observation would constitute a dark matter smoking gun signal. We performed the first dedicated search with a neutrino telescope for such signal, by looking at both the angular and energy information of the neutrino events. To this end, a total of five years of IceCube's DeepCore data has been used to test dark matter masses ranging from 10 GeV to 40 TeV. No significant neutrino excess was found and upper limits on the annihilation cross section, as well as lower limits on the dark matter lifetime, were set. The limits reached are of the order of 10-24 cm3/s for an annihilation and up to 1027 s for decaying dark matter. Using the same data sample we also derive limits for dark matter annihilation or decay into a pair of Standard Model charged particles.
Published: 2023

3. Search for GeV-scale dark matter annihilation in the Sun with IceCube DeepCore

Author: Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alameddine, JM, Alispach, C, Alves, AA, Amin, NM, Andeen, K, Anderson, T, Anton, G, Argüelles, C, Ashida, Y, Axani, S, Bai, X, Balagopal, A, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, Bellenghi, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Boddenberg, M, Bontempo, F, Borowka, J, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bradascio, F, Braun, J, Brinson, B, Bron, S, Brostean-Kaiser, J, Browne, S, Burgman, A, Burley, RT, Busse, RS, Campana, MA, Carnie-Bronca, EG, Chen, C, Chen, Z, Chirkin, D, Choi, K, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dappen, C, Dave, P, De Clercq, C, DeLaunay, JJ, López, D Delgado, Dembinski, H, Deoskar, K, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Diaz, A, Díaz-Vélez, JC, Dittmer, M, Dujmovic, H, Dunkman, M, DuVernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Erpenbeck, H, Evans, J, Evenson, PA, Fan, KL, Fazely, AR, Feigl, N, Fiedlschuster, S, Fienberg, AT, and Filimonov, K
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: The Sun provides an excellent target for studying spin-dependent dark matter-proton scattering due to its high matter density and abundant hydrogen content. Dark matter particles from the Galactic halo can elastically interact with Solar nuclei, resulting in their capture and thermalization in the Sun. The captured dark matter can annihilate into Standard Model particles including an observable flux of neutrinos. We present the results of a search for low-energy (
Published: 2022

4. All-flavor constraints on nonstandard neutrino interactions and generalized matter potential with three years of IceCube DeepCore data

Author: Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Alves, AA, Amin, NM, An, R, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Ashida, Y, Axani, S, Bai, X, V., A Balagopal, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, Bellenghi, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bontempo, F, Borowka, J, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Browne, S, Burgman, A, Busse, RS, Campana, MA, Chen, C, Chirkin, D, Choi, K, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Dharani, S, Diaz, A, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, DuVernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Erpenbeck, H, Evans, J, Evenson, PA, Fazely, AR, Fiedlschuster, S, Fienberg, AT, Filimonov, K, Finley, C, Fischer, L, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, and Fürst, P
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: We report constraints on nonstandard neutrino interactions (NSI) from the observation of atmospheric neutrinos with IceCube, limiting all individual coupling strengths from a single dataset. Furthermore, IceCube is the first experiment to constrain flavor-violating and nonuniversal couplings simultaneously. Hypothetical NSI are generically expected to arise due to the exchange of a new heavy mediator particle. Neutrinos propagating in matter scatter off fermions in the forward direction with negligible momentum transfer. Hence the study of the matter effect on neutrinos propagating in the Earth is sensitive to NSI independently of the energy scale of new physics. We present constraints on NSI obtained with an all-flavor event sample of atmospheric neutrinos based on three years of IceCube DeepCore data. The analysis uses neutrinos arriving from all directions, with reconstructed energies between 5.6 GeV and 100 GeV. We report constraints on the individual NSI coupling strengths considered singly, allowing for complex phases in the case of flavor-violating couplings. This demonstrates that IceCube is sensitive to the full NSI flavor structure at a level competitive with limits from the global analysis of all other experiments. In addition, we investigate a generalized matter potential, whose overall scale and flavor structure are also constrained.
Published: 2021

5. Measurement of the high-energy all-flavor neutrino-nucleon cross section with IceCube

Author: Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Alves, AA, Amin, NM, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Axani, S, Bai, X, V., A Balagopal, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, Bellenghi, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Busse, RS, Campana, MA, Chen, C, Chirkin, D, Choi, S, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Dharani, S, Diaz, A, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, DuVernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Evans, J, Evenson, PA, Fahey, S, Fazely, AR, Fiedlschuster, S, Fienberg, AT, Filimonov, K, Finley, C, Fischer, L, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, Fürst, P, Gaisser, TK, Gallagher, J, and Ganster, E
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: The flux of high-energy neutrinos passing through the Earth is attenuated due to their interactions with matter. The interaction rate is determined by the neutrino interaction cross section and affects the flux arriving at the IceCube Neutrino Observatory, a cubic-kilometer neutrino detector embedded in the Antarctic ice sheet. We present a measurement of the neutrino cross section between 60 TeV and 10 PeV using the high-energy starting event (HESE) sample from IceCube with 7.5 years of data. The result is binned in neutrino energy and obtained using both Bayesian and frequentist statistics. We find it compatible with predictions from the Standard Model. While the cross section is expected to be flavor independent above 1 TeV, additional constraints on the measurement are included through updated experimental particle identification (PID) classifiers, proxies for the three neutrino flavors. This is the first such measurement to use a ternary PID observable and the first to account for neutrinos from tau decay.
Published: 2021

6. IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data

Author: Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Alves, AA, Amin, NM, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Axani, S, Bai, X, V., A Balagopal, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, Bellenghi, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Busse, RS, Campana, MA, Chen, C, Chirkin, D, Choi, S, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Dharani, S, Diaz, A, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, DuVernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Evans, J, Evenson, PA, Fahey, S, Fazely, AR, Fiedlschuster, S, Fienberg, AT, Filimonov, K, Finley, C, Fischer, L, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, Fürst, P, Gaisser, TK, Gallagher, J, and Ganster, E
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: The IceCube Neutrino Observatory has established the existence of a high-energy all-sky neutrino flux of astrophysical origin. This discovery was made using events interacting within a fiducial region of the detector surrounded by an active veto and with reconstructed energy above 60 TeV, commonly known as the high-energy starting event sample (HESE). We revisit the analysis of the HESE sample with an additional 4.5 years of data, newer glacial ice models, and improved systematics treatment. This paper describes the sample in detail, reports on the latest astrophysical neutrino flux measurements, and presents a source search for astrophysical neutrinos. We give the compatibility of these observations with specific isotropic flux models proposed in the literature as well as generic power-law-like scenarios. Assuming νe:νμ:ντ=1:1:1, and an equal flux of neutrinos and antineutrinos, we find that the astrophysical neutrino spectrum is compatible with an unbroken power law, with a preferred spectral index of 2.87-0.19+0.20 for the 68% confidence interval.
Published: 2021

7. Search for GeV neutrino emission during intense gamma-ray solar flares with the IceCube Neutrino Observatory

Author: Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Alves, AA, Amin, NM, An, R, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Axani, S, Bai, X, V., A Balagopal, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, Bellenghi, C, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Busse, RS, Campana, MA, Chen, C, Chirkin, D, Choi, S, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Dharani, S, Diaz, A, Vélez, JC Díaz, Dujmovic, H, Dunkman, M, DuVernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Evans, J, Evenson, PA, Fahey, S, Fazely, AR, Fiedlschuster, S, Fienberg, AT, Filimonov, K, Finley, C, Fischer, L, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, Fürst, P, Gaisser, TK, and Gallagher, J
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, astro-ph.HE, astro-ph.SR, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: Solar flares convert magnetic energy into thermal and nonthermal plasma energy, the latter implying particle acceleration of charged particles such as protons. Protons are injected out of the coronal acceleration region and can interact with dense plasma in the lower solar atmosphere, producing mesons that subsequently decay into gamma rays and neutrinos at O(MeV-GeV) energies. We present the results of the first search for GeV neutrinos emitted during solar flares carried out with the IceCube Neutrino Observatory. While the experiment was originally designed to detect neutrinos with energies between 10 GeV and a few PeV, a new approach allowing for a O(GeV) energy threshold will be presented. The resulting limits allow us to constrain some of the theoretical estimates of the expected neutrino flux.
Published: 2021

8. Measurements of the time-dependent cosmic-ray Sun shadow with seven years of IceCube data: Comparison with the Solar cycle and magnetic field models

Author: Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Amin, NM, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Bagherpour, H, Bai, X, Balagopal, AV, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Buscher, J, Busse, RS, Carver, T, Chen, C, Cheung, E, Chirkin, D, Choi, S, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desai, A, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Dharani, S, Diaz, A, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, DuVernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Evenson, PA, Fahey, S, Fazely, AR, Felde, J, Fichtner, H, Fienberg, AT, Filimonov, K, Finley, C, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, and Gaisser, TK
Subjects: Astronomical Sciences, Physical Sciences, astro-ph.HE, astro-ph.SR, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: Observations of the time-dependent cosmic-ray Sun shadow have been proven as a valuable diagnostic for the assessment of solar magnetic field models. In this paper, seven years of IceCube data are compared to solar activity and solar magnetic field models. A quantitative comparison of solar magnetic field models with IceCube data on the event rate level is performed for the first time. Additionally, a first energy-dependent analysis is presented and compared to recent predictions. We use seven years of IceCube data for the moon and the Sun and compare them to simulations on data rate level. The simulations are performed for the geometrical shadow hypothesis for the moon and the Sun and for a cosmic-ray propagation model governed by the solar magnetic field for the case of the Sun. We find that a linearly decreasing relationship between Sun shadow strength and solar activity is preferred over a constant relationship at the 6.4σ level. We test two commonly used models of the coronal magnetic field, both combined with a Parker spiral, by modeling cosmic-ray propagation in the solar magnetic field. Both models predict a weakening of the shadow in times of high solar activity as it is also visible in the data. We find tensions with the data on the order of 3σ for both models, assuming only statistical uncertainties. The magnetic field model CSSS fits the data slightly better than the PFSS model. This is generally consistent with what is found previously by the Tibet AS-γ Experiment; a deviation of the data from the two models is, however, not significant at this point. Regarding the energy dependence of the Sun shadow, we find indications that the shadowing effect increases with energy during times of high solar activity, in agreement with theoretical predictions.
Published: 2021

9. Searching for eV-scale sterile neutrinos with eight years of atmospheric neutrinos at the IceCube Neutrino Telescope

Author: Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Amin, NM, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Bagherpour, H, Bai, X, Balagopal V., A, Barbano, A, Barwick, SW, Bastian, B, Basu, V, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, KH, Becker Tjus, J, Benzvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Buscher, J, Busse, RS, Carver, T, Chen, C, Cheung, E, Chirkin, D, Choi, S, Clark, BA, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, De Clercq, C, Delaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desai, A, Desiati, P, De Vries, KD, De Wasseige, G, De With, M, Deyoung, T, Dharani, S, Diaz, A, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, Duvernois, MA, Dvorak, E, Ehrhardt, T, Eller, P, Engel, R, Evenson, PA, Fahey, S, Fazely, AR, Fedynitch, A, Felde, J, Fienberg, AT, Filimonov, K, Finley, C, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, and Gaisser, TK
Subjects: hep-ex, hep-ph
Abstract: We report in detail on searches for eV-scale sterile neutrinos, in the context of a 3+1 model, using eight years of data from the IceCube Neutrino Telescope. By analyzing the reconstructed energies and zenith angles of 305,735 atmospheric νμ and ν¯μ events we construct confidence intervals in two analysis spaces: sin2(2θ24) vs Δm412 under the conservative assumption θ34=0; and sin2(2θ24) vs sin2(2θ34) given sufficiently large Δm412 that fast oscillation features are unresolvable. Detailed discussions of the event selection, systematic uncertainties, and fitting procedures are presented. No strong evidence for sterile neutrinos is found, and the best-fit likelihood is consistent with the no sterile neutrino hypothesis with a p value of 8% in the first analysis space and 19% in the second.
Published: 2020

10. Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Alispach, C, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Arlen, TC, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Balagopal, A, Barbano, A, Bartos, I, Barwick, SW, Bastian, B, Baum, V, Baur, S, Bay, R, Beatty, JJ, Becker, KH, Becker Tjus, J, Benzvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Bohmer, M, Böser, S, Botner, O, Böttcher, J, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bron, S, Brostean-Kaiser, J, Burgman, A, Buscher, J, Busse, RS, Carver, T, Chen, C, Cheung, E, Chirkin, D, Choi, S, Clark, K, Classen, L, Coleman, A, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, De Clercq, C, Delaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desiati, P, De Vries, KD, De Wasseige, G, De With, M, Deyoung, T, Diaz, A, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, Duvernois, MA, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eller, P, Engel, R, Evans, JJ, Evenson, PA, Fahey, S, Farrag, K, Fazely, AR, Felde, J, Filimonov, K, Finley, C, Fox, D, Franckowiak, A, Friedman, E, Fritz, A, Gaisser, TK, and Gallagher, J
Subjects: hep-ex, physics.ins-det
Abstract: The ordering of the neutrino mass eigenstates is one of the fundamental open questions in neutrino physics. While current-generation neutrino oscillation experiments are able to produce moderate indications on this ordering, upcoming experiments of the next generation aim to provide conclusive evidence. In this paper we study the combined performance of the two future multi-purpose neutrino oscillation experiments JUNO and the IceCube Upgrade, which employ two very distinct and complementary routes toward the neutrino mass ordering. The approach pursued by the 20 kt medium-baseline reactor neutrino experiment JUNO consists of a careful investigation of the energy spectrum of oscillated νe produced by ten nuclear reactor cores. The IceCube Upgrade, on the other hand, which consists of seven additional densely instrumented strings deployed in the center of IceCube DeepCore, will observe large numbers of atmospheric neutrinos that have undergone oscillations affected by Earth matter. In a joint fit with both approaches, tension occurs between their preferred mass-squared differences Δm312=m32-m12 within the wrong mass ordering. In the case of JUNO and the IceCube Upgrade, this allows to exclude the wrong ordering at >5σ on a timescale of 3-7 years - even under circumstances that are unfavorable to the experiments' individual sensitivities. For PINGU, a 26-string detector array designed as a potential low-energy extension to IceCube, the inverted ordering could be excluded within 1.5 years (3 years for the normal ordering) in a joint analysis.
Published: 2020

11. Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCube

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Al Samarai, I, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Barbano, A, Barron, JP, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Börner, M, Bos, F, Böser, S, Botner, O, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Brenzke, M, Bretz, H-P, Bron, S, Brostean-Kaiser, J, Burgman, A, Busse, RS, Carver, T, Cheung, E, Chirkin, D, Clark, K, Classen, L, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, Day, M, de André, JPAM, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, di Lorenzo, V, Dujmovic, H, Dumm, JP, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Evenson, PA, Fahey, S, Fazely, AR, Felde, J, Filimonov, K, Finley, C, Franckowiak, A, Friedman, E, Fritz, A, Gaisser, TK, Gallagher, J, Ganster, E, Garrappa, S, Gerhardt, L, Ghorbani, K, Giang, W, and Glauch, T
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, hep-ex, astro-ph.HE, nucl-ex
Abstract: Inelasticity, the fraction of a neutrino's energy transferred to hadrons, is a quantity of interest in the study of astrophysical and atmospheric neutrino interactions at multi-TeV energies with IceCube. In this work, a sample of contained neutrino interactions in IceCube is obtained from five years of data and classified as 2650 tracks and 965 cascades. Tracks arise predominantly from charged-current νμ interactions, and we demonstrate that we can reconstruct their energy and inelasticity. The inelasticity distribution is found to be consistent with the calculation of Cooper-Sarkar et al. across the energy range from ∼1 to ∼100 TeV. Along with cascades from neutrinos of all flavors, we also perform a fit over the energy, zenith angle, and inelasticity distribution to characterize the flux of astrophysical and atmospheric neutrinos. The energy spectrum of diffuse astrophysical neutrinos is described well by a power law in both track and cascade samples, and a best-fit index γ=2.62±0.07 is found in the energy range from 3.5 TeV to 2.6 PeV. Limits are set on the astrophysical flavor composition and are compatible with a ratio of (13â¶13â¶13)âŠ•. Exploiting the distinct inelasticity distribution of νμ and ν̄μ interactions, the atmospheric νμ to ν̄μ flux ratio in the energy range from 770 GeV to 21 TeV is found to be 0.77-0.25+0.44 times the calculation by Honda et al. Lastly, the inelasticity distribution is also sensitive to neutrino charged-current charm production. The data are consistent with a leading-order calculation, with zero charm production excluded at 91% confidence level. Future analyses of inelasticity distributions may probe new physics that affects neutrino interactions both in and beyond the Standard Model.
Published: 2019

12. Measurement of atmospheric tau neutrino appearance with IceCube DeepCore

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Barbano, A, Barron, JP, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Becker, K-H, Tjus, J Becker, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Börner, M, Böser, S, Botner, O, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Bretz, H-P, Bron, S, Brostean-Kaiser, J, Burgman, A, Busse, RS, Carver, T, Chen, C, Cheung, E, Chirkin, D, Clark, K, Classen, L, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, de André, JPAM, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, Dujmovic, H, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eller, P, Evenson, PA, Fahey, S, Fazely, AR, Felde, J, Filimonov, K, Finley, C, Franckowiak, A, Friedman, E, Fritz, A, Gaisser, TK, Gallagher, J, Ganster, E, Garrappa, S, Gerhardt, L, Ghorbani, K, Giang, W, Glauch, T, Glüsenkamp, T, Goldschmidt, A, Gonzalez, JG, Grant, D, Griffith, Z, and Gündüz, M
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, hep-ex, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: We present a measurement of atmospheric tau neutrino appearance from oscillations with three years of data from the DeepCore subarray of the IceCube Neutrino Observatory. This analysis uses atmospheric neutrinos from the full sky with reconstructed energies between 5.6 and 56 GeV to search for a statistical excess of cascadelike neutrino events which are the signature of ντ interactions. For CC+NC (CC-only) interactions, we measure the tau neutrino normalization to be 0.73-0.24+0.30 (0.57-0.30+0.36) and exclude the absence of tau neutrino oscillations at a significance of 3.2σ (2.0σ) These results are consistent with, and of similar precision to, a confirmatory IceCube analysis also presented, as well as measurements performed by other experiments.
Published: 2019

13. Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Al Samarai, I, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Barbano, A, Barron, JP, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Börner, M, Bos, F, Böser, S, Botner, O, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Brenzke, M, Bretz, H-P, Bron, S, Brostean-Kaiser, J, Burgman, A, Busse, RS, Carver, T, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Collin, GH, Conrad, JM, Coppin, P, Correa, P, Cowen, DF, Cross, R, Dave, P, Day, M, de André, JPAM, De Clercq, C, DeLaunay, JJ, Dembinski, H, Deoskar, K, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, di Lorenzo, V, Dujmovic, H, Dumm, JP, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Evenson, PA, Fahey, S, Fazely, AR, Felde, J, Filimonov, K, Finley, C, Flis, S, Franckowiak, A, Friedman, E, Fritz, A, Gaisser, TK, Gallagher, J, Ganster, E, Gerhardt, L, Ghorbani, K, and Giang, W
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE, hep-ex, hep-ph
Abstract: We report a quasidifferential upper limit on the extremely-high-energy (EHE) neutrino flux above 5×106 GeV based on an analysis of nine years of IceCube data. The astrophysical neutrino flux measured by IceCube extends to PeV energies, and it is a background flux when searching for an independent signal flux at higher energies, such as the cosmogenic neutrino signal. We have developed a new method to place robust limits on the EHE neutrino flux in the presence of an astrophysical background, whose spectrum has yet to be understood with high precision at PeV energies. A distinct event with a deposited energy above 106 GeV was found in the new two-year sample, in addition to the one event previously found in the seven-year EHE neutrino search. These two events represent a neutrino flux that is incompatible with predictions for a cosmogenic neutrino flux and are considered to be an astrophysical background in the current study. The obtained limit is the most stringent to date in the energy range between 5×106 and 2×1010 GeV. This result constrains neutrino models predicting a three-flavor neutrino flux of Eν2φνe+νμ+ντ≃2×10-8 GeV/cm2 sec sr at 109 GeV. A significant part of the parameter space for EHE neutrino production scenarios assuming a proton-dominated composition of ultra-high-energy cosmic rays is disfavored independently of uncertain models of the extragalactic background light which previous IceCube constraints partially relied on.
Published: 2018

14. Search for nonstandard neutrino interactions with IceCube DeepCore

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Al Samarai, I, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Bagherpour, H, Bai, X, Barron, JP, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Brayeur, L, Brenzke, M, Bretz, H-P, Bron, S, Brostean-Kaiser, J, Burgman, A, Carver, T, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Coenders, S, Collin, GH, Conrad, JM, Cowen, DF, Cross, R, Day, M, de André, JPAM, De Clercq, C, DeLaunay, JJ, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, di Lorenzo, V, Dujmovic, H, Dumm, JP, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Evenson, PA, Fahey, S, Fazely, AR, Felde, J, Filimonov, K, Finley, C, Flis, S, Franckowiak, A, Friedman, E, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Ghorbani, K, Giang, W, Glauch, T, Glüsenkamp, T, and Goldschmidt, A
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, hep-ex, hep-ph
Abstract: As atmospheric neutrinos propagate through the Earth, vacuumlike oscillations are modified by Standard Model neutral- and charged-current interactions with electrons. Theories beyond the Standard Model introduce heavy, TeV-scale bosons that can produce nonstandard neutrino interactions. These additional interactions may modify the Standard Model matter effect producing a measurable deviation from the prediction for atmospheric neutrino oscillations. The result described in this paper constrains nonstandard interaction parameters, building upon a previous analysis of atmospheric muon-neutrino disappearance with three years of IceCube DeepCore data. The best fit for the muon to tau flavor changing term is ϵμτ=-0.0005, with a 90% C.L. allowed range of -0.0067
Published: 2018

15. Search for sterile neutrino mixing using three years of IceCube DeepCore data

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Samarai, I Al, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Archinger, M, Argüelles, C, Auffenberg, J, Axani, S, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berley, D, Bernardini, E, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Braun, J, Brayeur, L, Bretz, H-P, Bron, S, Burgman, A, Carver, T, Casier, M, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Coenders, S, Collin, GH, Conrad, JM, Cowen, DF, Cross, R, Day, M, de André, JPAM, De Clercq, C, del Pino Rosendo, E, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, di Lorenzo, V, Dujmovic, H, Dumm, JP, Dunkman, M, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Euler, S, Evenson, PA, Fahey, S, Fazely, AR, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Flis, S, Fösig, C-C, Franckowiak, A, Friedman, E, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Ghorbani, K, Giang, W, Gladstone, L, Glauch, T, Glüsenkamp, T, Goldschmidt, A, Gonzalez, JG, Grant, D, Griffith, Z, and Haack, C
Subjects: hep-ex, hep-ph, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: We present a search for a light sterile neutrino using three years of atmospheric neutrino data from the DeepCore detector in the energy range of approximately 10-60 GeV. DeepCore is the low-energy subarray of the IceCube Neutrino Observatory. The standard three-neutrino paradigm can be probed by adding an additional light (Δm412∼1 eV2) sterile neutrino. Sterile neutrinos do not interact through the standard weak interaction and, therefore, cannot be directly detected. However, their mixing with the three active neutrino states leaves an imprint on the standard atmospheric neutrino oscillations for energies below 100 GeV. A search for such mixing via muon neutrino disappearance is presented here. The data are found to be consistent with the standard three-neutrino hypothesis. Therefore, we derive limits on the mixing matrix elements at the level of |Uμ4|2
Published: 2017

16. Search for astrophysical tau neutrinos in three years of IceCube data

Author: Aartsen, MG, Abraham, K, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Ansseau, I, Archinger, M, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, Beiser, E, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Braun, J, Brayeur, L, Bretz, H-P, Buzinsky, N, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Coenders, S, Cowen, DF, Silva, AH Cruz, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, del Pino Rosendo, E, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, di Lorenzo, V, Dumm, JP, Dunkman, M, Eagan, R, Eberhardt, B, Ehrhardt, T, Eichmann, B, Euler, S, Evenson, PA, Fadiran, O, Fahey, S, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Fösig, C-C, Fuchs, T, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Ghorbani, K, Gier, D, Gladstone, L, Glagla, M, Glüsenkamp, T, Goldschmidt, A, and Golup, G
Subjects: astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract: The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7σ significance from an all-flavor search. The direct detection of tau neutrinos in this flux has yet to occur. Tau neutrinos become distinguishable from other flavors in IceCube at energies above a few hundred TeV, when the cascade from the tau neutrino charged current interaction becomes resolvable from the cascade from the tau lepton decay. This paper presents results from the first dedicated search for tau neutrinos with energies between 214 TeV and 72 PeV in the full IceCube detector. The analysis searches for IceCube optical sensors that observe two separate pulses in a single event - one from the tau neutrino interaction and a second from the tau decay. No candidate events were observed in three years of IceCube data. For the first time, a differential upper limit on astrophysical tau neutrinos is derived around the PeV energy region, which is nearly 3 orders of magnitude lower in energy than previous limits from dedicated tau neutrino searches.
Published: 2016

17. Measurement of the Atmospheric νe Spectrum with IceCube

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Archinger, M, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, Beiser, E, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Braun, J, Brayeur, L, Bretz, H-P, Brown, AM, Buzinsky, N, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Coenders, S, Cowen, DF, Silva, AH Cruz, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, Dumm, JP, Dunkman, M, Eagan, R, Eberhardt, B, Ehrhardt, T, Eichmann, B, Euler, S, Evenson, PA, Fadiran, O, Fahey, S, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Fuchs, T, Glagla, M, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Ghorbani, K, Gier, D, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, and Góra, D
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE
Abstract: We present a measurement of the atmospheric νe spectrum at energies between 0.1 and 100 TeV using data from the first year of the complete IceCube detector. Atmospheric νe originate mainly from the decays of kaons produced in cosmic-ray air showers. This analysis selects 1078 fully contained events in 332 days of live time, and then identifies those consistent with particle showers. A likelihood analysis with improved event selection extends our previous measurement of the conventional νe fluxes to higher energies. The data constrain the conventional νe flux to be 1.3-0.3+0.4 times a baseline prediction from a Honda's calculation, including the knee of the cosmic-ray spectrum. A fit to the kaon contribution (ξ) to the neutrino flux finds a kaon component that is ξ=1.3-0.4+0.5 times the baseline value. The fitted/measured prompt neutrino flux from charmed hadron decays strongly depends on the assumed astrophysical flux and shape. If the astrophysical component follows a power law, the result for the prompt flux is 0.0-0.0+3.0 times a calculated flux based on the work by Enberg, Reno, and Sarcevic.
Published: 2015

18. Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bos, F, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Brunner, J, Buzinsky, N, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Clevermann, F, Coenders, S, Cowen, DF, Silva, AH Cruz, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eichmann, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Frantzen, K, Fuchs, T, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Gier, D, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grant, D, Gretskov, P, Groh, JC, Groß, A, and Ha, C
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, hep-ex, physics.ins-det
Abstract: We present a measurement of neutrino oscillations via atmospheric muon neutrino disappearance with three years of data of the completed IceCube neutrino detector. DeepCore, a region of denser IceCube instrumentation, enables the detection and reconstruction of atmospheric muon neutrinos between 10 and 100 GeV, where a strong disappearance signal is expected. The IceCube detector volume surrounding DeepCore is used as a veto region to suppress the atmospheric muon background. Neutrino events are selected where the detected Cherenkov photons of the secondary particles minimally scatter, and the neutrino energy and arrival direction are reconstructed. Both variables are used to obtain the neutrino oscillation parameters from the data, with the best fit given by Δm322=2.72-0.20+0.19×10-3eV2 and sin2θ23=0.53-0.12+0.09 (normal mass ordering assumed). The results are compatible, and comparable in precision, to those of dedicated oscillation experiments.
Published: 2015

19. Atmospheric and astrophysical neutrinos above 1 TeV interacting in IceCube

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bos, F, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Buzinsky, N, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Clevermann, F, Coenders, S, Cowen, DF, Silva, AH Cruz, Danninger, M, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eichmann, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Frantzen, K, Fuchs, T, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Gier, D, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grant, D, Gretskov, P, Groh, JC, Groß, A, and Ha, C
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE
Abstract: The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV-PeV) neutrinos produced in distant astrophysical objects. A search for 100TeV neutrinos interacting inside the instrumented volume has recently provided evidence for an isotropic flux of such neutrinos. At lower energies, IceCube collects large numbers of neutrinos from the weak decays of mesons in cosmic-ray air showers. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1 TeV and 1 PeV in 641 days of data taken from 2010-2012, lowering the energy threshold for neutrinos from the southern sky below 10 TeV for the first time, far below the threshold of the previous high-energy analysis. Astrophysical neutrinos remain the dominant component in the southern sky down to a deposited energy of 10 TeV. From these data we derive new constraints on the diffuse astrophysical neutrino spectrum, Φν=2.06-0.3+0.4×10-18(Eν/105GeV)-2.46±0.12GeV-1cm-2sr-1s-1 for 25TeV
Published: 2015

20. Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

Author: Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bos, F, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Casey, J, Casier, M, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Clevermann, F, Coenders, S, Cowen, DF, Silva, AH Cruz, Danninger, M, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eichmann, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Frantzen, K, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Gier, D, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grandmont, DT, Grant, D, Gretskov, P, Groh, JC, Groß, A, Ha, C, Haack, C, Ismail, A Haj, and Hallen, P
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, astro-ph.HE
Abstract: We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of gravitational-wave emission energy of 10-2M c2 at ∼150Hz with ∼60ms duration, and high-energy neutrino emission of 1051erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6×10-2Mpc-3yr-1. We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.
Published: 2014

21. Observation of the cosmic-ray shadow of the Moon with IceCube

Author: Aartsen, MG, Abbasi, R, Abdou, Y, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Altmann, D, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Bechet, S, Tjus, J Becker, Becker, K-H, Bell, M, Benabderrahmane, ML, BenZvi, S, Berdermann, J, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Bertrand, D, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohaichuk, S, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Bruijn, R, Brunner, J, Carson, M, Casey, J, Casier, M, Chirkin, D, Christov, A, Christy, B, Clark, K, Clevermann, F, Coenders, S, Cohen, S, Cowen, DF, Silva, AH Cruz, Danninger, M, Daughhetee, J, Davis, JC, De Clercq, C, De Ridder, S, Desiati, P, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eisch, J, Ellsworth, RW, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Franke, R, Frantzen, K, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grandmont, DT, Grant, D, Groß, A, Ha, C, and Ismail, A Haj
Subjects: Particle and High Energy Physics, Physical Sciences, astro-ph.HE
Abstract: We report on the observation of a significant deficit of cosmic rays from the direction of the Moon with the IceCube detector. The study of this "Moon shadow" is used to characterize the angular resolution and absolute pointing capabilities of the detector. The detection is based on data taken in two periods before the completion of the detector: between April 2008 and May 2009, when IceCube operated in a partial configuration with 40 detector strings deployed in the South Pole ice, and between May 2009 and May 2010 when the detector operated with 59 strings. Using two independent analysis methods, the Moon shadow has been observed to high significance (>6σ) in both detector configurations. The observed location of the shadow center is within 0.2° of its expected position when geomagnetic deflection effects are taken into account. This measurement validates the directional reconstruction capabilities of IceCube. © 2014 American Physical Society.
Published: 2014

22. Search for neutrino-induced particle showers with IceCube-40

Author: Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Altmann, D, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Bruijn, R, Casey, J, Casier, M, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Clevermann, F, Coenders, S, Cohen, S, Cowen, DF, Silva, AH Cruz, Danninger, M, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eichmann, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Frantzen, K, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grandmont, DT, Grant, D, Gretskov, P, Groh, JC, Groß, A, Ha, C, Ismail, A Haj, Hallen, P, and Hallgren, A
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE
Abstract: We report on the search for neutrino-induced particle showers, so-called cascades, in the IceCube-40 detector. The data for this search were collected between April 2008 and May 2009 when the first 40 IceCube strings were deployed and operational. Three complementary searches were performed, each optimized for different energy regimes. The analysis with the lowest energy threshold (2 TeV) targeted atmospheric neutrinos. A total of 67 events were found, consistent with the expectation of 41 atmospheric muons and 30 atmospheric neutrino events. The two other analyses targeted a harder, astrophysical neutrino flux. The analysis with an intermediate threshold of 25 TeV leads to the observation of 14 cascadelike events, again consistent with the prediction of 3.0 atmospheric neutrino and 7.7 atmospheric muon events. We hence set an upper limit of E2Φlim≤7.46×10-8GeVsr-1s-1cm-2 (90% C.L.) on the diffuse flux from astrophysical neutrinos of all neutrino flavors, applicable to the energy range 25 TeV to 5 PeV, assuming an Eν-2 spectrum and a neutrino flavor ratio of 1 at the Earth. The third analysis utilized a larger and optimized sample of atmospheric muon background simulation, leading to a higher energy threshold of 100 TeV. Three events were found over a background prediction of 0.04 atmospheric muon events and 0.21 events from the flux of conventional and prompt atmospheric neutrinos. Including systematic errors this corresponds to a 2.7σ excess with respect to the background-only hypothesis. Our observation of neutrino event candidates above 100 TeV complements IceCube's recently observed evidence for high-energy astrophysical neutrinos. © 2014 American Physical Society.
Published: 2014

23. Search for a diffuse flux of astrophysical muon neutrinos with the IceCube 59-string configuration

Author: Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Altmann, D, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Bruijn, R, Casey, J, Casier, M, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Clevermann, F, Coenders, S, Cohen, S, Cowen, DF, Silva, AH Cruz, Danninger, M, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eichmann, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Frantzen, K, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grandmont, DT, Grant, D, Gretskov, P, Groh, JC, Groß, A, Ha, C, Ismail, A Haj, Hallen, P, and Hallgren, A
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE
Abstract: A search for high-energy neutrinos was performed using data collected by the IceCube Neutrino Observatory from May 2009 to May 2010, when the array was running in its 59-string configuration. The data sample was optimized to contain muon neutrino induced events with a background contamination of atmospheric muons of less than 1%. These data, which are dominated by atmospheric neutrinos, are analyzed with a global likelihood fit to search for possible contributions of prompt atmospheric and astrophysical neutrinos, neither of which have yet been identified. Such signals are expected to follow a harder energy spectrum than conventional atmospheric neutrinos. In addition, the zenith angle distribution differs for astrophysical and atmospheric signals. A global fit of the reconstructed energies and directions of observed events is performed, including possible neutrino flux contributions for an astrophysical signal and atmospheric backgrounds as well as systematic uncertainties of the experiment and theoretical predictions. The best fit yields an astrophysical signal flux for νμ+ν̄μ of E2·Φ(E)=0.25×10-8GeVcm-2s-1sr-1, and a zero prompt component. Although the sensitivity of this analysis for astrophysical neutrinos surpasses the Waxman and Bahcall upper bound, the experimental limit at 90% confidence level is a factor of 1.5 above at a flux of E2·Φ(E)=1.44×10-8GeVcm-2s-1sr-1. © 2014 American Physical Society.
Published: 2014

24. Probing the origin of cosmic rays with extremely high energy neutrinos using the IceCube Observatory

Author: Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Altmann, D, Arguelles, C, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Bruijn, R, Casey, J, Casier, M, Chirkin, D, Christov, A, Christy, B, Clark, K, Clevermann, F, Coenders, S, Cohen, S, Cowen, DF, Silva, AH Cruz, Danninger, M, Daughhetee, J, Davis, JC, Day, M, De Clercq, C, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Frantzen, K, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grandmont, DT, Grant, D, Gretskov, P, Groh, JC, Groß, A, Ha, C, Ismail, A Haj, Hallen, P, Hallgren, A, Halzen, F, Hanson, K, Heereman, D, and Heinen, D
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, astro-ph.HE, astro-ph.CO, hep-ex, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract: We have searched for extremely high energy neutrinos using data taken with the IceCube detector between May 2010 and May 2012. Two neutrino-induced particle shower events with energies around 1 PeV were observed, as reported previously. In this work, we investigate whether these events could originate from cosmogenic neutrinos produced in the interactions of ultrahigh energy cosmic rays with ambient photons while propagating through intergalactic space. Exploiting IceCube's large exposure for extremely high energy neutrinos and the lack of observed events above 100 PeV, we can rule out the corresponding models at more than 90% confidence level. The model-independent quasidifferential 90% C.L. upper limit, which amounts to E2e+ν+ν=1.2×10-7 GeV cm-2 s-1 sr-1 at 1 EeV, provides the most stringent constraint in the energy range from 10 PeV to 10 EeV. Our observation disfavors strong cosmological evolution of the highest energy cosmic-ray sources such as the Fanaroff-Riley type II class of radio galaxies. © 2013 American Physical Society.
Published: 2013

25. Measurement of the high-energy all-flavor neutrino-nucleon cross section with IceCube

Author: IceCube Collaboration, Abbasi, R., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alispach, C., Alves, A. A., Amin, N. M., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Axani, S., Bai, X., Balagopal V., A., Barbano, A., Barwick, S. W., Bastian, B., Basu, V., Baum, V., Baur, S., Bay, R., Beatty, J. J., Becker, K.-H., Becker Tjus, J., Bellenghi, C., BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Busse, R. S., Campana, M. A., Chen, C., Chirkin, D., Choi, S., Clark, B. A., Clark, K., Classen, L., Coleman, A., Collin, G. H., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., De Clercq, C., DeLaunay, J. J., Dembinski, H., Deoskar, K., De Ridder, S., Desai, A., Desiati, P., Vries, K. D. de, Wasseige, G. de, With, M. de, DeYoung, T., Dharani, S., Diaz, A., Díaz-Vélez, J. C., Dujmovic, H., Dunkman, M., DuVernois, M. A., Dvorak, E., Ehrhardt, T., Eller, P., Engel, R., Evans, J., Evenson, P. A., Fahey, S., Fazely, A. R., Fiedlschuster, S., Fienberg, A. T., Filimonov, K., Finley, C., Fischer, L., Fox, D., Franckowiak, A., Friedman, E., Fritz, A., Fürst, P., Gaisser, T. K., Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Ghadimi, A., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Goswami, S., Grant, D., Grégoire, T., Griffith, Z., Griswold, S., Gündüz, M., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Ha Minh, M., Hanson, K., Hardin, J., Haungs, A., Hauser, S., Hebecker, D., Helbing, K., Henningsen, F., Hickford, S., Hignight, J., Hill, C., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Huber, T., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jones, B. J. P., Joppe, R., Kang, D., Kang, W., Kang, X., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Katz, U., Kauer, M., Kellermann, M., Kelley, J. L., Kheirandish, A., Kim, J., Kin, K., Kintscher, T., Kiryluk, J., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Koundal, P., Kovacevich, M., Kowalski, M., Krings, K., Krückl, G., Kulacz, N., Kurahashi, N., Kyriacou, A., Lagunas Gualda, C., Lanfranchi, J. L., Larson, M. J., Lauber, F., Lazar, J. P., Leonard, K., Leszczyńska, A., Li, Y., Liu, Q. R., Lohfink, E., Lozano Mariscal, C. J., Lu, L., Lucarelli, F., Ludwig, A., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Mahn, K. B. M., Makino, Y., Mallik, P., Mancina, S., Mariş, I. C., Maruyama, R., Mase, K., McNally, F., Meagher, K., Medina, A., Meier, M., Meighen-Berger, S., Merz, J., Micallef, J., Mockler, D., Momenté, G., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Naab, R., Nagai, R., Naumann, U., Necker, J., Neer, G., Nguyễn, L. V., Niederhausen, H., Nisa, M. U., Nowicki, S. C., Nygren, D. R., Obertacke Pollmann, A., Oehler, M., Olivas, A., O’Sullivan, E., Pandya, H., Pankova, D. V., Park, N., Parker, G. K., Paudel, E. N., Peiffer, P., Pérez de los Heros, C., Philippen, S., Pieloth, D., Pieper, S., Pizzuto, A., Plum, M., Popovych, Y., Porcelli, A., Prado Rodriguez, M., Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Rawlins, K., Rea, I. C., Rehman, A., Reimann, R., Renschler, M., Renzi, G., Resconi, E., Reusch, S., Rhode, W., Richman, M., Riedel, B., Robertson, S., Roellinghoff, G., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk Cantu, D., Safa, I., Sanchez Herrera, S. E., Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Scharf, M., Schaufel, M., Schieler, H., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shefali, S., Silva, M., Smithers, B., Snihur, R., Soedingrekso, J., Soldin, D., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Strotjohann, N. L., Stuttard, T., Sullivan, G. W., Taboada, I., Tenholt, F., Ter-Antonyan, S., Tilav, S., Tischbein, F., Tollefson, K., Tomankova, L., Tönnis, C., Toscano, S., Tosi, D., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Twagirayezu, J. P., Ty, B., Unger, E., Unland Elorrieta, M. A., Usner, M., Vandenbroucke, J., Eijk, D. van, Eijndhoven, N. van, Vannerom, D., Santen, J. van, Verpoest, S., Vraeghe, M., Walck, C., Wallace, A., Wandkowsky, N., Watson, T. B., Weaver, C., Weindl, A., Weiss, M. J., Weldert, J., Wendt, C., Werthebach, J., Weyrauch, M., Whelan, B. J., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wolf, M., Wood, T. R., Woschnagg, K., Wrede, G., Wulff, J., Xu, X. W., Xu, Y., Yanez, J. P., Yoshida, S., Yuan, T., Zhang, Z., Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, and Elementary Particle Physics
Subjects: Physics::Instrumentation and Detectors, ice, interaction [neutrino nucleon], 01 natural sciences, Particle identification, IceCube, High Energy Physics - Experiment, Subatomär fysik, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), Astronomi, astrofysik och kosmologi, Subatomic Physics, Astronomy, Astrophysics and Cosmology, detector [neutrino], astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, hep-ph, Observable, ddc, observatory, High Energy Physics - Phenomenology, Neutrino detector, statistics, decay [tau], Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Nucleon, data analysis method, Particle physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, ACCELERATION, Bayesian [statistical analysis], IceCube Neutrino Observatory, Standard Model, cross section [neutrino nucleon], 0103 physical sciences, ddc:530, GLASHOW RESONANCE, 010306 general physics, hep-ex, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, flavor [neutrino], flux [neutrino], frequentist [statistical analysis], Physics and Astronomy, energy [neutrino], High Energy Physics::Experiment, Event (particle physics), experimental results
Abstract: The flux of high-energy neutrinos passing through the Earth is attenuated due to their interactions with matter. The interaction rate is modulated by the neutrino interaction cross section and affects the flux arriving at the IceCube Neutrino Observatory, a cubic-kilometer neutrino detector embedded in the Antarctic ice sheet. We present a measurement of the neutrino cross section between 60 TeV and 10 PeV using the high-energy starting events (HESE) sample from IceCube with 7.5 years of data. The result is binned in neutrino energy and obtained using both Bayesian and frequentist statistics. We find it compatible with predictions from the Standard Model. Flavor information is explicitly included through updated morphology classifiers, proxies for the the three neutrino flavors. This is the first such measurement to use the three morphologies as observables and the first to account for neutrinos from tau decay., Comment: 10 pages, 7 figures, 2 tables. This article is supported by a long-form paper that discusses in high-energy starting event selection titled: "The IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data"
Published: 2021
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26. Search for neutrino-induced cascades with the AMANDA detector

Author: Ahrens, J., Bai, X., Böser, S., Stokstad, R. G., Sulanke, K.-H., Taboada, I., Thollander, L., Tilav, S., Vander Donckt, M., Wagner, W., Walck, C., Weinheimer, C., Wiebusch, C. H., Booth, J., Widemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., AMANDA Collaboration, Botner, O., Bouchta, A., Bouhali, O., Boyce, M. M., Burgess, T., Carius, S., Chen, A., Chirkin, D., Barouch, G., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Davour, A., De Clercq, C., DeYoung, T., Desiati, P., Dewulf, J.-P., Doksus, P., Barwick, S. W., Ekström, P., Feser, T., Frère, J.-M., Gaisser, T. K., Gaug, M., Geenen, H., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Bay, R. C., Hardtke, R., Hauschildt, T., Hellwig, M., Hill, G. C., Hulth, P. O., Hultqvist, K., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Becka, T., Koci, B., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Lowder, D. M., Madsen, J., Becker, K.-H., Marciniewski, P., Matis, H. S., McParland, C. P., Messarius, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Bertrand, D., Niessen, P., Nygren, D. R., Ogelman, H., Olbrechts, Ph., Pérez de los Heros, C., Pohl, A. C., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Binon, F., Reed, C., Resconi, E., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H.-G., Schinarakis, K., Biron, A., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., and Steffen, P.
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), High Energy Physics::Phenomenology, Detector, FOS: Physical sciences, Observable, Astrophysics, equipment and supplies, Particle detector, Particle identification, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Neutrino detector, ddc:530, High Energy Physics::Experiment, Neutrino, Electron neutrino, Lepton
Abstract: We report on a search for electromagnetic and/or hadronic showers (cascades) induced by a diffuse flux of neutrinos with energies between 5 TeV and 300 TeV from extraterrestrial sources. Cascades may be produced by matter interactions of all flavors of neutrinos, and contained cascades have better energy resolution and afford better background rejection than through-going \nu_\mu-induced muons. Data taken in 1997 with the AMANDA detector were searched for events with a high-energy cascade-like signature. The observed events are consistent with expected backgrounds from atmospheric neutrinos and catastrophic energy losses from atmospheric muons. Effective volumes for all flavors of neutrinos, which allow the calculation of limits for any neutrino flux model, are presented. The limit on cascades from a diffuse flux of \nu_e+\nu_\mu+\nu_\tau+\bar{\nu}_e+\bar{\nu}_\mu+\bar{\nu}_\tau is E^2 d\Phi/dE < 9.8 x 10^{-6} GeV/(cm^2 s sr), assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of \nu_e+\bar{\nu}_e is E^ d\Phi/dE < 6.5 x 10{-6} GeV/(cm^2 s sr), independent of the assumed neutrino flavor flux ratio., Comment: 11 pages, 8 figures, 2 tables Submitted to Physical Review D
Published: 2003
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27. IceCube search for dark matter annihilation in nearby galaxies and galaxy clusters

Author: Aartsen, M. G., primary, Abbasi, R., additional, Abdou, Y., additional, Ackermann, M., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Altmann, D., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Baum, V., additional, Bay, R., additional, Beatty, J. J., additional, Bechet, S., additional, Becker Tjus, J., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bernhard, A., additional, Bertrand, D., additional, Besson, D. Z., additional, Binder, G., additional, Bindig, D., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohaichuk, S., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Brayeur, L., additional, Bretz, H.-P., additional, Brown, A. M., additional, Bruijn, R., additional, Brunner, J., additional, Carson, M., additional, Casey, J., additional, Casier, M., additional, Chirkin, D., additional, Christov, A., additional, Christy, B., additional, Clark, K., additional, Clevermann, F., additional, Coenders, S., additional, Cohen, S., additional, Cowen, D. F., additional, Cruz Silva, A. H., additional, Danninger, M., additional, Daughhetee, J., additional, Davis, J. C., additional, Day, M., additional, De Clercq, C., additional, De Ridder, S., additional, Desiati, P., additional, de Vries, K. D., additional, de With, M., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dunkman, M., additional, Eagan, R., additional, Eberhardt, B., additional, Eisch, J., additional, Ellsworth, R. W., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feintzeig, J., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Fischer-Wasels, T., additional, Flis, S., additional, Franckowiak, A., additional, Frantzen, K., additional, Fuchs, T., additional, Gaisser, T. K., additional, Gallagher, J., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Golup, G., additional, Gonzalez, J. G., additional, Goodman, J. A., additional, Góra, D., additional, Grandmont, D. T., additional, Grant, D., additional, Groß, A., additional, Ha, C., additional, Haj Ismail, A., additional, Hallen, P., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Heereman, D., additional, Heinen, D., additional, Helbing, K., additional, Hellauer, R., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Hoffmann, R., additional, Homeier, A., additional, Hoshina, K., additional, Huelsnitz, W., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobi, E., additional, Jacobsen, J., additional, Jagielski, K., additional, Japaridze, G. S., additional, Jero, K., additional, Jlelati, O., additional, Kaminsky, B., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kiryluk, J., additional, Kläs, J., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kopper, C., additional, Kopper, S., additional, Koskinen, D. J., additional, Kowalski, M., additional, Krasberg, M., additional, Krings, K., additional, Kroll, G., additional, Kunnen, J., additional, Kurahashi, N., additional, Kuwabara, T., additional, Labare, M., additional, Landsman, H., additional, Larson, M. J., additional, Lesiak-Bzdak, M., additional, Leuermann, M., additional, Leute, J., additional, Lünemann, J., additional, Macías, O., additional, Madsen, J., additional, Maggi, G., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McNally, F., additional, Meagher, K., additional, Merck, M., additional, Meures, T., additional, Miarecki, S., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Mohrmann, L., additional, Montaruli, T., additional, Morse, R., additional, Nahnhauer, R., additional, Naumann, U., additional, Niederhausen, H., additional, Nowicki, S. C., additional, Nygren, D. R., additional, Obertacke, A., additional, Odrowski, S., additional, Olivas, A., additional, Omairat, A., additional, O’Murchadha, A., additional, Paul, L., additional, Pepper, J. A., additional, Pérez de los Heros, C., additional, Pfendner, C., additional, Pieloth, D., additional, Pinat, E., additional, Posselt, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rädel, L., additional, Rameez, M., additional, Rawlins, K., additional, Redl, P., additional, Reimann, R., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Richman, M., additional, Riedel, B., additional, Rodrigues, J. P., additional, Rott, C., additional, Ruhe, T., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Saba, S. M., additional, Salameh, T., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Scheriau, F., additional, Schmidt, T., additional, Schmitz, M., additional, Schoenen, S., additional, Schöneberg, S., additional, Schönwald, A., additional, Schukraft, A., additional, Schulte, L., additional, Schulz, O., additional, Seckel, D., additional, Sestayo, Y., additional, Seunarine, S., additional, Shanidze, R., additional, Sheremata, C., additional, Smith, M. W. E., additional, Soldin, D., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stasik, A., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stößl, A., additional, Strahler, E. A., additional, Ström, R., additional, Sullivan, G. W., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tešić, G., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Unger, E., additional, Usner, M., additional, Vallecorsa, S., additional, van Eijndhoven, N., additional, Van Overloop, A., additional, van Santen, J., additional, Vehring, M., additional, Voge, M., additional, Vraeghe, M., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Weaver, Ch., additional, Wellons, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Williams, D. R., additional, Wissing, H., additional, Wolf, M., additional, Wood, T. R., additional, Woschnagg, K., additional, Xu, D. L., additional, Xu, X. W., additional, Yanez, J. P., additional, Yodh, G., additional, Yoshida, S., additional, Zarzhitsky, P., additional, Ziemann, J., additional, Zierke, S., additional, and Zoll, M., additional
Published: 2013
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28. Measurement of the cosmic ray energy spectrum with IceTop-73

Author: Aartsen, M. G., primary, Abbasi, R., additional, Abdou, Y., additional, Ackermann, M., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Altmann, D., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Baum, V., additional, Bay, R., additional, Beatty, J. J., additional, Bechet, S., additional, Becker Tjus, J., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bernhard, A., additional, Bertrand, D., additional, Besson, D. Z., additional, Binder, G., additional, Bindig, D., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohaichuk, S., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Brayeur, L., additional, Bretz, H.-P., additional, Brown, A. M., additional, Bruijn, R., additional, Brunner, J., additional, Carson, M., additional, Casey, J., additional, Casier, M., additional, Chirkin, D., additional, Christov, A., additional, Christy, B., additional, Clark, K., additional, Clevermann, F., additional, Coenders, S., additional, Cohen, S., additional, Cowen, D. F., additional, Cruz Silva, A. H., additional, Danninger, M., additional, Daughhetee, J., additional, Davis, J. C., additional, De Clercq, C., additional, De Ridder, S., additional, Desiati, P., additional, de Vries, K. D., additional, de With, M., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dunkman, M., additional, Eagan, R., additional, Eberhardt, B., additional, Eisch, J., additional, Ellsworth, R. W., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feintzeig, J., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Fischer-Wasels, T., additional, Flis, S., additional, Franckowiak, A., additional, Frantzen, K., additional, Fuchs, T., additional, Gaisser, T. K., additional, Gallagher, J., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Golup, G., additional, Gonzalez, J. G., additional, Goodman, J. A., additional, Góra, D., additional, Grandmont, D. T., additional, Grant, D., additional, Groß, A., additional, Ha, C., additional, Haj Ismail, A., additional, Hallen, P., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Heereman, D., additional, Heinen, D., additional, Helbing, K., additional, Hellauer, R., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Hoffmann, R., additional, Homeier, A., additional, Hoshina, K., additional, Huelsnitz, W., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobi, E., additional, Jacobsen, J., additional, Jagielski, K., additional, Japaridze, G. S., additional, Jero, K., additional, Jlelati, O., additional, Kaminsky, B., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kiryluk, J., additional, Kläs, J., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kopper, C., additional, Kopper, S., additional, Koskinen, D. J., additional, Kowalski, M., additional, Krasberg, M., additional, Krings, K., additional, Kroll, G., additional, Kunnen, J., additional, Kurahashi, N., additional, Kuwabara, T., additional, Labare, M., additional, Landsman, H., additional, Larson, M. J., additional, Lesiak-Bzdak, M., additional, Leuermann, M., additional, Leute, J., additional, Lünemann, J., additional, Macíias, O., additional, Madsen, J., additional, Maggi, G., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McNally, F., additional, Meagher, K., additional, Merck, M., additional, Meures, T., additional, Miarecki, S., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Mohrmann, L., additional, Montaruli, T., additional, Morse, R., additional, Nahnhauer, R., additional, Naumann, U., additional, Niederhausen, H., additional, Nowicki, S. C., additional, Nygren, D. R., additional, Obertacke, A., additional, Odrowski, S., additional, Olivas, A., additional, Omairat, A., additional, O’Murchadha, A., additional, Paul, L., additional, Pepper, J. A., additional, Pérez de los Heros, C., additional, Pfendner, C., additional, Pieloth, D., additional, Pinat, E., additional, Posselt, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rädel, L., additional, Rameez, M., additional, Rawlins, K., additional, Redl, P., additional, Reimann, R., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Richman, M., additional, Riedel, B., additional, Rodrigues, J. P., additional, Rott, C., additional, Ruhe, T., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Saba, S. M., additional, Salameh, T., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Scheriau, F., additional, Schmidt, T., additional, Schmitz, M., additional, Schoenen, S., additional, Schöneberg, S., additional, Schönwald, A., additional, Schukraft, A., additional, Schulte, L., additional, Schulz, O., additional, Seckel, D., additional, Sestayo, Y., additional, Seunarine, S., additional, Shanidze, R., additional, Sheremata, C., additional, Smith, M. W. E., additional, Soldin, D., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stasik, A., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stößl, A., additional, Strahler, E. A., additional, Ström, R., additional, Sullivan, G. W., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tešić, G., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Unger, E., additional, Usner, M., additional, Vallecorsa, S., additional, van Eijndhoven, N., additional, Van Overloop, A., additional, van Santen, J., additional, Vehring, M., additional, Voge, M., additional, Vraeghe, M., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Weaver, Ch., additional, Wellons, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Williams, D. R., additional, Wissing, H., additional, Wolf, M., additional, Wood, T. R., additional, Woschnagg, K., additional, Xu, C., additional, Xu, D. L., additional, Xu, X. W., additional, Yanez, J. P., additional, Yodh, G., additional, Yoshida, S., additional, Zarzhitsky, P., additional, Ziemann, J., additional, Zierke, S., additional, and Zoll, M., additional
Published: 2013
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29. Erratum: Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data [Phys. Rev. D83, 092003 (2011)]

Author: Abbasi, R., primary, Abdou, Y., additional, Abu-Zayyad, T., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bindig, D., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Braun, J., additional, Brown, A. M., additional, Buitink, S., additional, Carson, M., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Clevermann, F., additional, Cohen, S., additional, Colnard, C., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Daughhetee, J., additional, Davis, J. C., additional, De Clercq, C., additional, Demirörs, L., additional, Denger, T., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dierckxsens, M., additional, Dreyer, J., additional, Dumm, J. P., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Fischer-Wasels, T., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Geisler, M., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gora, D., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Heinen, D., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Homeier, A., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kopper, S., additional, Koskinen, D. J., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Krings, T., additional, Kroll, G., additional, Kuwabara, T., additional, Labare, M., additional, Lafebre, S., additional, Laihem, K., additional, Landsman, H., additional, Larson, M. J., additional, Lauer, R., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Marotta, A., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Nahnhauer, R., additional, Nam, J. W., additional, Naumann, U., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, O’Murchadha, A., additional, Ono, M., additional, Panknin, S., additional, Paul, L., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Porrata, R., additional, Posselt, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Ruhe, T., additional, Rutledge, D., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Schmidt, T., additional, Schönwald, A., additional, Schukraft, A., additional, Schultes, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stössl, A., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Stür, M., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, van Santen, J., additional, Vehring, M., additional, Voge, M., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Walter, M., additional, Weaver, Ch., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Wolf, M., additional, Wood, T. R., additional, Woschnagg, K., additional, Xu, C., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zarzhitsky, P., additional
Published: 2011
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30. First search for atmospheric and extraterrestrial neutrino-induced cascades with the IceCube detector

Author: Abbasi, R., primary, Abdou, Y., additional, Abu-Zayyad, T., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bindig, D., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Braun, J., additional, Brown, A. M., additional, Buitink, S., additional, Carson, M., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Clevermann, F., additional, Cohen, S., additional, Colnard, C., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Daughhetee, J., additional, Davis, J. C., additional, De Clercq, C., additional, Demirörs, L., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dierckxsens, M., additional, Dreyer, J., additional, Dumm, J. P., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Fischer-Wasels, T., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Geisler, M., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Heinen, D., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Homeier, A., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kemming, N., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kopper, S., additional, Koskinen, D. J., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Krings, T., additional, Kroll, G., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Lafebre, S., additional, Laihem, K., additional, Landsman, H., additional, Larson, M. J., additional, Lauer, R., additional, Lehmann, R., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Marotta, A., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Nahnhauer, R., additional, Nam, J. W., additional, Naumann, U., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, O’Murchadha, A., additional, Ono, M., additional, Panknin, S., additional, Paul, L., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Porrata, R., additional, Posselt, J., additional, Price, P. B., additional, Prikockis, M., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Ruhe, T., additional, Rutledge, D., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Schmidt, T., additional, Schoenwald, A., additional, Schukraft, A., additional, Schultes, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, van Santen, J., additional, Vehring, M., additional, Voge, M., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Walter, M., additional, Weaver, Ch., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Wolf, M., additional, Woschnagg, K., additional, Xu, C., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zarzhitsky, P., additional
Published: 2011
Full Text: View/download PDF

31. Search for a Lorentz-violating sidereal signal with atmospheric neutrinos in IceCube

Author: Abbasi, R., primary, Abdou, Y., additional, Abu-Zayyad, T., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Braun, J., additional, Buitink, S., additional, Carson, M., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Clevermann, F., additional, Cohen, S., additional, Colnard, C., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Davis, J. C., additional, De Clercq, C., additional, Demirörs, L., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dierckxsens, M., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Geisler, M., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Homeier, A., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kemming, N., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Koskinen, D. J., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Krings, T., additional, Kroll, G., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Lafebre, S., additional, Laihem, K., additional, Landsman, H., additional, Larson, M. J., additional, Lauer, R., additional, Lehmann, R., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Marotta, A., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, Matusik, M., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Nahnhauer, R., additional, Nam, J. W., additional, Naumann, U., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, O’Murchadha, A., additional, Ono, M., additional, Panknin, S., additional, Paul, L., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Porrata, R., additional, Posselt, J., additional, Price, P. B., additional, Prikockis, M., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Ruhe, T., additional, Rutledge, D., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schukraft, A., additional, Schultes, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Singh, K., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, van Santen, J., additional, Voge, M., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Walter, M., additional, Weaver, Ch., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Wolf, M., additional, Woschnagg, K., additional, Xu, C., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zarzhitsky, P., additional
Published: 2010
Full Text: View/download PDF

32. First search for extremely high energy cosmogenic neutrinos with the IceCube Neutrino Observatory

Author: Abbasi, R., primary, Abdou, Y., additional, Abu-Zayyad, T., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bissok, M., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Böser, S., additional, Botner, O., additional, Bradley, L., additional, Braun, J., additional, Buitink, S., additional, Carson, M., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Clevermann, F., additional, Cohen, S., additional, Colnard, C., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Davis, J. C., additional, De Clercq, C., additional, Demirörs, L., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Geisler, M., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Homeier, A., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Imlay, R. L., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kemming, N., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Knops, S., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Koskinen, D. J., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Krings, T., additional, Kroll, G., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Lafebre, S., additional, Laihem, K., additional, Landsman, H., additional, Lauer, R., additional, Lehmann, R., additional, Lennarz, D., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, Matusik, M., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Nahnhauer, R., additional, Nam, J. W., additional, Naumann, U., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, Ono, M., additional, Panknin, S., additional, Paul, L., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Porrata, R., additional, Posselt, J., additional, Price, P. B., additional, Prikockis, M., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Roucelle, C., additional, Ruhe, T., additional, Rutledge, D., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Schatto, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Schukraft, A., additional, Schultes, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taboada, I., additional, Tamburro, A., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tilav, S., additional, Toale, P. A., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, van Santen, J., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Walter, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, C., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zarzhitsky, P., additional
Published: 2010
Full Text: View/download PDF

33. Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector

Author: Abbasi, R., primary, Abdou, Y., additional, Abu-Zayyad, T., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bissok, M., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Botner, O., additional, Bradley, L., additional, Braun, J., additional, Breder, D., additional, Carson, M., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cohen, S., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Gerhardt, L., additional, Gladstone, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hasegawa, Y., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Homeier, A., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Imlay, R. L., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kemming, N., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Knops, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Koskinen, D. J., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Krings, T., additional, Kroll, G., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Lafebre, S., additional, Laihem, K., additional, Landsman, H., additional, Lauer, R., additional, Lehmann, R., additional, Lennarz, D., additional, Lucke, A., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McParland, C. P., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Middell, E., additional, Milke, N., additional, Miyamoto, H., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, Ono, M., additional, Panknin, S., additional, Patton, S., additional, Paul, L., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Potthoff, N., additional, Price, P. B., additional, Prikockis, M., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Roucelle, C., additional, Rutledge, D., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Schatto, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Schukraft, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taboada, I., additional, Tamburro, A., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Terranova, C., additional, Tilav, S., additional, Toale, P. A., additional, Tooker, J., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, van Santen, J., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Walter, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Wiedemann, A., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, C., additional, Xu, X. W., additional, Yodh, G., additional, and Yoshida, S., additional
Published: 2010
Full Text: View/download PDF

34. Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II

Author: Abbasi, R., primary, Abdou, Y., additional, Ackermann, M., additional, Adams, J., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bissok, M., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Böser, S., additional, Botner, O., additional, Bradley, L., additional, Braun, J., additional, Breder, D., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cohen, S., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Diaz-Velez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Gerhardt, L., additional, Gladstone, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hasegawa, Y., additional, Heise, J., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Imlay, R. L., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Klepser, S., additional, Knops, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Laihem, K., additional, Landsman, H., additional, Lauer, R., additional, Leich, H., additional, Lennarz, D., additional, Lucke, A., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McParland, C. P., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Middell, E., additional, Milke, N., additional, Miyamoto, H., additional, Mohr, A., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, Ono, M., additional, Panknin, S., additional, Patton, S., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Potthoff, N., additional, Price, P. B., additional, Prikockis, M., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Roucelle, C., additional, Rutledge, D., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Satalecka, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Schukraft, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taboada, I., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Terranova, C., additional, Tilav, S., additional, Tluczykont, M., additional, Toale, P. A., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Walter, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebusch, C. H., additional, Wiedemann, A., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, X. W., additional, Yodh, G., additional, and Yoshida, S., additional
Published: 2009
Full Text: View/download PDF

35. Search for point sources of high energy neutrinos with final data from AMANDA-II

Author: Abbasi, R., primary, Ackermann, M., additional, Adams, J., additional, Ahlers, M., additional, Ahrens, J., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Baret, B., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Becka, T., additional, Becker, J. K., additional, Becker, K.-H., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Böser, S., additional, Botner, O., additional, Braun, J., additional, Breder, D., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Davour, A., additional, Day, C. T., additional, Depaepe, O., additional, De Clercq, C., additional, Demirörs, L., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Diaz-Velez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Gerhardt, L., additional, Gladstone, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hardtke, R., additional, Hasegawa, Y., additional, Heise, J., additional, Helbing, K., additional, Hellwig, M., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hodges, J., additional, Hoffman, K. D., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hughey, B., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hundertmark, S., additional, Hussain, S., additional, Imlay, R. L., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kawai, H., additional, Kelley, J. L., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Klepser, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Laihem, K., additional, Landsman, H., additional, Lauer, R., additional, Leich, H., additional, Leier, D., additional, Lewis, C., additional, Lucke, A., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McParland, C. P., additional, Meagher, K., additional, Meli, A., additional, Merck, M., additional, Messarius, T., additional, Mészáros, P., additional, Miyamoto, H., additional, Mohr, A., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, Ono, M., additional, Panknin, S., additional, Patton, S., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Potthoff, N., additional, Pretz, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Razzaque, S., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Robbins, W. J., additional, Rodriguez, J., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Roucelle, C., additional, Rutledge, D., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Satalecka, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Schultz, O., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Smith, A. J., additional, Song, C., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taboada, I., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tilav, S., additional, Tluczykont, M., additional, Toale, P. A., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, Viscomi, V., additional, Vogt, C., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Walter, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebusch, C. H., additional, Wiedemann, C., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, X. W., additional, Yodh, G., additional, and Yoshida, S., additional
Published: 2009
Full Text: View/download PDF

36. Erratum: Multiyear search for a diffuse flux of muon neutrinos with AMANDA-II [Phys. Rev. D76, 042008 (2007)]

Author: Achterberg, A., primary, Ackermann, M., additional, Adams, J., additional, Ahrens, J., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baret, B., additional, Barwick, S. W., additional, Bay, R., additional, Beattie, K., additional, Becka, T., additional, Becker, J. K., additional, Becker, K.-H., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Böser, S., additional, Botner, O., additional, Bouchta, A., additional, Braun, J., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Davour, A., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Descamps, F., additional, Desiati, P., additional, DeYoung, T., additional, Diaz-Velez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Geenen, H., additional, Gerhardt, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hardtke, D., additional, Hardtke, R., additional, Hart, J. E., additional, Hasegawa, Y., additional, Hauschildt, T., additional, Hays, D., additional, Heise, J., additional, Helbing, K., additional, Hellwig, M., additional, Herquet, P., additional, Hill, G. C., additional, Hodges, J., additional, Hoffman, K. D., additional, Hommez, B., additional, Hoshina, K., additional, Hubert, D., additional, Hughey, B., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hundertmark, S., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Jones, A., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kawai, H., additional, Kelley, J. L., additional, Kislat, F., additional, Kitamura, N., additional, Klein, S. R., additional, Klepser, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Kuehn, K., additional, Labare, M., additional, Landsman, H., additional, Lauer, R., additional, Leich, H., additional, Leier, D., additional, Liubarsky, I., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McCauley, T., additional, McParland, C. P., additional, Meli, A., additional, Messarius, T., additional, Mészáros, P., additional, Miyamoto, H., additional, Mokhtarani, A., additional, Montaruli, T., additional, Morey, A., additional, Morse, R., additional, Movit, S. M., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Ögelman, H., additional, Olivas, A., additional, Patton, S., additional, Peña-Garay, C., additional, Pérez de los Heros, C., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Pretz, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Razzaque, S., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Robbins, S., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Rutledge, D., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Satalecka, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Smith, A. J., additional, Solarz, M., additional, Song, C., additional, Sopher, J. E., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Sumner, T. J., additional, Taboada, I., additional, Tarasova, O., additional, Tepe, A., additional, Thollander, L., additional, Tilav, S., additional, Tluczykont, M., additional, Toale, P. A., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, Viscomi, V., additional, Voigt, B., additional, Wagner, W., additional, Walck, C., additional, Waldmann, H., additional, Walter, M., additional, Wang, Y.-R., additional, Wendt, C., additional, Wiebusch, C. H., additional, Wiedemann, C., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zornoza, J. D., additional
Published: 2008
Full Text: View/download PDF

37. Multiyear search for a diffuse flux of muon neutrinos with AMANDA-II

Author: Achterberg, A., primary, Ackermann, M., additional, Adams, J., additional, Ahrens, J., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baret, B., additional, Barwick, S. W., additional, Bay, R., additional, Beattie, K., additional, Becka, T., additional, Becker, J. K., additional, Becker, K.-H., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Böser, S., additional, Botner, O., additional, Bouchta, A., additional, Braun, J., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Davour, A., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Descamps, F., additional, Desiati, P., additional, DeYoung, T., additional, Diaz-Velez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Geenen, H., additional, Gerhardt, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hardtke, D., additional, Hardtke, R., additional, Hart, J. E., additional, Hasegawa, Y., additional, Hauschildt, T., additional, Hays, D., additional, Heise, J., additional, Helbing, K., additional, Hellwig, M., additional, Herquet, P., additional, Hill, G. C., additional, Hodges, J., additional, Hoffman, K. D., additional, Hommez, B., additional, Hoshina, K., additional, Hubert, D., additional, Hughey, B., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hundertmark, S., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Jones, A., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kawai, H., additional, Kelley, J. L., additional, Kislat, F., additional, Kitamura, N., additional, Klein, S. R., additional, Klepser, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Kuehn, K., additional, Labare, M., additional, Landsman, H., additional, Lauer, R., additional, Leich, H., additional, Leier, D., additional, Liubarsky, I., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McCauley, T., additional, McParland, C. P., additional, Meli, A., additional, Messarius, T., additional, Mészáros, P., additional, Miyamoto, H., additional, Mokhtarani, A., additional, Montaruli, T., additional, Morey, A., additional, Morse, R., additional, Movit, S. M., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Ögelman, H., additional, Olivas, A., additional, Patton, S., additional, Peña-Garay, C., additional, Pérez de los Heros, C., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Pretz, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Razzaque, S., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Robbins, S., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Rutledge, D., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Satalecka, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Smith, A. J., additional, Solarz, M., additional, Song, C., additional, Sopher, J. E., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Sumner, T. J., additional, Taboada, I., additional, Tarasova, O., additional, Tepe, A., additional, Thollander, L., additional, Tilav, S., additional, Tluczykont, M., additional, Toale, P. A., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, Viscomi, V., additional, Voigt, B., additional, Wagner, W., additional, Walck, C., additional, Waldmann, H., additional, Walter, M., additional, Wang, Y.-R., additional, Wendt, C., additional, Wiebusch, C. H., additional, Wiedemann, C., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zornoza, J. D., additional
Published: 2007
Full Text: View/download PDF

38. Detection of atmospheric muon neutrinos with the IceCube 9-string detector

Author: Achterberg, A., primary, Ackermann, M., additional, Adams, J., additional, Ahrens, J., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baret, B., additional, Barwick, S. W., additional, Bay, R., additional, Beattie, K., additional, Becka, T., additional, Becker, J. K., additional, Becker, K.-H., additional, Beimforde, M., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Böser, S., additional, Botner, O., additional, Bouchta, A., additional, Braun, J., additional, Burgess, C., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Davour, A., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Descamps, F., additional, Desiati, P., additional, DeYoung, T., additional, Diaz-Velez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Geenen, H., additional, Gerhardt, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Griesel, T., additional, Grullon, S., additional, Groß, A., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hardtke, D., additional, Hardtke, R., additional, Hart, J. E., additional, Hasegawa, Y., additional, Hauschildt, T., additional, Hays, D., additional, Heise, J., additional, Helbing, K., additional, Hellwig, M., additional, Herquet, P., additional, Hill, G. C., additional, Hodges, J., additional, Hoffman, K. D., additional, Hommez, B., additional, Hoshina, K., additional, Hubert, D., additional, Hughey, B., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hundertmark, S., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Jones, A., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kawai, H., additional, Kelley, J. L., additional, Kislat, F., additional, Kitamura, N., additional, Klein, S. R., additional, Klepser, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Kuehn, K., additional, Labare, M., additional, Landsman, H., additional, Lauer, R., additional, Leich, H., additional, Leier, D., additional, Liubarsky, I., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McCauley, T., additional, McParland, C. P., additional, Meagher, K., additional, Meli, A., additional, Messarius, T., additional, Mészáros, P., additional, Miyamoto, H., additional, Mokhtarani, A., additional, Montaruli, T., additional, Morey, A., additional, Morse, R., additional, Movit, S. M., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Olivas, A., additional, Patton, S., additional, Peña-Garay, C., additional, de los Heros, C. Pérez, additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Pretz, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Razzaque, S., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Robbins, S., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Rutledge, D., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Satalecka, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Smith, A. J., additional, Song, C., additional, Sopher, J. E., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Sumner, T. J., additional, Taboada, I., additional, Tarasova, O., additional, Tepe, A., additional, Thollander, L., additional, Tilav, S., additional, Tluczykont, M., additional, Toale, P. A., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, de Vries-Uiterweerd, G., additional, Viscomi, V., additional, Voigt, B., additional, Wagner, W., additional, Walck, C., additional, Waldmann, H., additional, Walter, M., additional, Wang, Y.-R., additional, Wendt, C., additional, Wiebusch, C. H., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zornoza, J. D., additional
Published: 2007
Full Text: View/download PDF

39. Five years of searches for point sources of astrophysical neutrinos with the AMANDA-II neutrino telescope

Author: Achterberg, A., primary, Ackermann, M., additional, Adams, J., additional, Ahrens, J., additional, Andeen, K., additional, Atlee, D. W., additional, Bahcall, J. N., additional, Bai, X., additional, Baret, B., additional, Barwick, S. W., additional, Bay, R., additional, Beattie, K., additional, Becka, T., additional, Becker, J. K., additional, Becker, K.-H., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Böser, S., additional, Botner, O., additional, Bouchta, A., additional, Braun, J., additional, Burgess, C., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Davour, A., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Descamps, F., additional, Desiati, P., additional, DeYoung, T., additional, Diaz-Velez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Feser, T., additional, Filimonov, K., additional, Fox, B. D., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Geenen, H., additional, Gerhardt, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Grullon, S., additional, Groß, A., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hardtke, D., additional, Hardtke, R., additional, Harenberg, T., additional, Hart, J. E., additional, Hauschildt, T., additional, Hays, D., additional, Heise, J., additional, Helbing, K., additional, Hellwig, M., additional, Herquet, P., additional, Hill, G. C., additional, Hodges, J., additional, Hoffman, K. D., additional, Hommez, B., additional, Hoshina, K., additional, Hubert, D., additional, Hughey, B., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hundertmark, S., additional, Hülß, J.-P., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Jones, A., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Karle, A., additional, Kawai, H., additional, Kelley, J. L., additional, Kestel, M., additional, Kitamura, N., additional, Klein, S. R., additional, Klepser, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Kowalski, M., additional, Köpke, L., additional, Krasberg, M., additional, Kuehn, K., additional, Landsman, H., additional, Leich, H., additional, Leier, D., additional, Leuthold, M., additional, Liubarsky, I., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Mase, K., additional, Matis, H. S., additional, McCauley, T., additional, McParland, C. P., additional, Meli, A., additional, Messarius, T., additional, Mészáros, P., additional, Miyamoto, H., additional, Mokhtarani, A., additional, Montaruli, T., additional, Morey, A., additional, Morse, R., additional, Movit, S. M., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Ögelman, H., additional, Olivas, A., additional, Patton, S., additional, Peña-Garay, C., additional, Pérez de los Heros, C., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Pretz, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Razzaque, S., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Robbins, S., additional, Roth, P., additional, Rott, C., additional, Rutledge, D., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Seckel, D., additional, Seo, S. H., additional, Seunarine, S., additional, Silvestri, A., additional, Smith, A. J., additional, Solarz, M., additional, Song, C., additional, Sopher, J. E., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Steffen, P., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Sumner, T. J., additional, Taboada, I., additional, Tarasova, O., additional, Tepe, A., additional, Thollander, L., additional, Tilav, S., additional, Tluczykont, M., additional, Toale, P. A., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, Voigt, B., additional, Wagner, W., additional, Walck, C., additional, Waldmann, H., additional, Walter, M., additional, Wang, Y.-R., additional, Wendt, C., additional, Wiebusch, C. H., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, X. W., additional, Yodh, G., additional, Yoshida, S., additional, and Zornoza, J. D., additional
Published: 2007
Full Text: View/download PDF

40. Search for extraterrestrial point sources of high energy neutrinos with AMANDA-II using data collected in 2000–2002

Author: Ackermann, M., primary, Ahrens, J., additional, Bai, X., additional, Bay, R., additional, Bartelt, M., additional, Barwick, S. W., additional, Becka, T., additional, Becker, K. H., additional, Becker, J. K., additional, Bernardini, E., additional, Bertrand, D., additional, Boersma, D. J., additional, Böser, S., additional, Botner, O., additional, Bouchta, A., additional, Bouhali, O., additional, Braun, J., additional, Burgess, C., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Collin, B., additional, Conrad, J., additional, Cooley, J., additional, Cowen, D. F., additional, Davour, A., additional, De Clercq, C., additional, DeYoung, T., additional, Desiati, P., additional, Ekström, P., additional, Feser, T., additional, Gaisser, T. K., additional, Ganugapati, R., additional, Geenen, H., additional, Gerhardt, L., additional, Goldschmidt, A., additional, Groß, A., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Hardtke, D., additional, Hardtke, R., additional, Harenberg, T., additional, Hauschildt, T., additional, Helbing, K., additional, Hellwig, M., additional, Herquet, P., additional, Hill, G. C., additional, Hodges, J., additional, Hubert, D., additional, Hughey, B., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hundertmark, S., additional, Jacobsen, J., additional, Kampert, K. H., additional, Karle, A., additional, Kelley, J. L., additional, Kestel, M., additional, Kohnen, G., additional, Köpke, L., additional, Kowalski, M., additional, Krasberg, M., additional, Kuehn, K., additional, Leich, H., additional, Leuthold, M., additional, Liubarsky, I., additional, Lundberg, J., additional, Madsen, J., additional, Marciniewski, P., additional, Matis, H. S., additional, McParland, C. P., additional, Messarius, T., additional, Minaeva, Y., additional, Miočinović, P., additional, Morse, R., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Neunhöffer, T., additional, Niessen, P., additional, Nygren, D. R., additional, Ögelman, H., additional, Olbrechts, Ph., additional, Pérez de los Heros, C., additional, Pohl, A. C., additional, Porrata, R., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Richter, S., additional, Rodríguez Martino, J., additional, Sander, H. G., additional, Schinarakis, K., additional, Schlenstedt, S., additional, Schneider, D., additional, Schwarz, R., additional, Silvestri, A., additional, Solarz, M., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Steele, D., additional, Steffen, P., additional, Stokstad, R. G., additional, Sulanke, K. H., additional, Taboada, I., additional, Tarasova, O., additional, Thollander, L., additional, Tilav, S., additional, Wagner, W., additional, Walck, C., additional, Walter, M., additional, Wang, Y. R., additional, Wendt, C., additional, Wiebusch, C. H., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, and Yodh, G., additional
Published: 2005
Full Text: View/download PDF

41. Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector

Author: Ahrens, J., primary, Andrés, E., additional, Bai, X., additional, Barouch, G., additional, Barwick, S. W., additional, Bay, R. C., additional, Becka, T., additional, Becker, K.-H., additional, Bertrand, D., additional, Biron, A., additional, Botner, O., additional, Bouchta, A., additional, Carius, S., additional, Chen, A., additional, Chirkin, D., additional, Conrad, J., additional, Cooley, J., additional, Costa, C. G. S., additional, Cowen, D. F., additional, Dalberg, E., additional, De Clercq, C., additional, DeYoung, T., additional, Desiati, P., additional, Dewulf, J.-P., additional, Doksus, P., additional, Edsjö, J., additional, Ekström, P., additional, Feser, T., additional, Gaisser, T. K., additional, Gaug, M., additional, Gerhardt, L., additional, Goldschmidt, A., additional, Goobar, A., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Hardtke, R., additional, Hauschildt, T., additional, Hellwig, M., additional, Hill, G. C., additional, Hulth, P. O., additional, Hundertmark, S., additional, Jacobsen, J., additional, Karle, A., additional, Kim, J., additional, Koci, B., additional, Köpke, L., additional, Kowalski, M., additional, Lamoureux, J. I., additional, Leich, H., additional, Leuthold, M., additional, Lindahl, P., additional, Loaiza, P., additional, Lowder, D. M., additional, Ludvig, J., additional, Madsen, J., additional, Marciniewski, P., additional, Matis, H. S., additional, McParland, C. P., additional, Miller, T. C., additional, Minaeva, Y., additional, Miočinović, P., additional, Mock, P. C., additional, Morse, R., additional, Neunhöffer, T., additional, Niessen, P., additional, Nygren, D. R., additional, Ogelman, H., additional, Olbrechts, Ph., additional, Pérez de los Heros, C., additional, Pohl, A., additional, Porrata, R., additional, Price, P. B., additional, Przybylski, G.T., additional, Rawlins, K., additional, Rhode, W., additional, Ribordy, M., additional, Richter, S., additional, Rodríguez Martino, J., additional, Romenesko, P., additional, Ross, D., additional, Sander, H.-G., additional, Schmidt, T., additional, Schneider, D., additional, Schneider, E., additional, Schwarz, R., additional, Silvestri, A., additional, Solarz, M., additional, Spiczak, G. M., additional, Spiering, C., additional, Steele, D., additional, Steffen, P., additional, Stokstad, R. G., additional, Streicher, O., additional, Sudhoff, P., additional, Sulanke, K. H., additional, Taboada, I., additional, Thollander, L., additional, Thon, T., additional, Tilav, S., additional, Vander Donckt, M., additional, Walck, C., additional, Weinheimer, C., additional, Wiebusch, C. H., additional, Wiedemann, C., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Wu, W., additional, Yodh, G., additional, and Young, S., additional
Published: 2002
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42. Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array

Author: Ahrens, J., primary, Andrés, E., additional, Bai, X., additional, Barouch, G., additional, Barwick, S. W., additional, Bay, R. C., additional, Becka, T., additional, Becker, K.-H., additional, Bertrand, D., additional, Binon, F., additional, Biron, A., additional, Booth, J., additional, Botner, O., additional, Bouchta, A., additional, Bouhali, O., additional, Boyce, M. M., additional, Carius, S., additional, Chen, A., additional, Chirkin, D., additional, Conrad, J., additional, Cooley, J., additional, Costa, C. G. S., additional, Cowen, D. F., additional, Dalberg, E., additional, De Clercq, C., additional, DeYoung, T., additional, Desiati, P., additional, Dewulf, J.-P., additional, Doksus, P., additional, Edsjö, J., additional, Ekström, P., additional, Feser, T., additional, Frère, J.-M., additional, Gaisser, T. K., additional, Gaug, M., additional, Goldschmidt, A., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Hardtke, R., additional, Hauschildt, T., additional, Hellwig, M., additional, Heukenkamp, H., additional, Hill, G. C., additional, Hulth, P. O., additional, Hundertmark, S., additional, Jacobsen, J., additional, Karle, A., additional, Kim, J., additional, Koci, B., additional, Köpke, L., additional, Kowalski, M., additional, Lamoureux, J. I., additional, Leich, H., additional, Leuthold, M., additional, Lindahl, P., additional, Liubarsky, I., additional, Loaiza, P., additional, Lowder, D. M., additional, Madsen, J., additional, Marciniewski, P., additional, Matis, H. S., additional, McParland, C. P., additional, Miller, T. C., additional, Minaeva, Y., additional, Miočinović, P., additional, Mock, P. C., additional, Morse, R., additional, Neunhöffer, T., additional, Niessen, P., additional, Nygren, D. R., additional, Ögelman, H., additional, Olbrechts, Ph., additional, Pérez de los Heros, C., additional, Pohl, A. C., additional, Porrata, R., additional, Price, P. B., additional, Przybylski, G. T., additional, Rawlins, K., additional, Reed, C., additional, Rhode, W., additional, Ribordy, M., additional, Richter, S., additional, Rodríguez Martino, J., additional, Romenesko, P., additional, Ross, D., additional, Sander, H.-G., additional, Schmidt, T., additional, Schneider, D., additional, Schwarz, R., additional, Silvestri, A., additional, Solarz, M., additional, Spiczak, G. M., additional, Spiering, C., additional, Starinsky, N., additional, Steele, D., additional, Steffen, P., additional, Stokstad, R. G., additional, Streicher, O., additional, Sudhoff, P., additional, Sulanke, K.-H., additional, Taboada, I., additional, Thollander, L., additional, Thon, T., additional, Tilav, S., additional, Vander Donckt, M., additional, Walck, C., additional, Weinheimer, C., additional, Wiebusch, C. H., additional, Wiedeman, C., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Wu, W., additional, Yodh, G., additional, and Young, S., additional
Published: 2002
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