J. C. Davis - IceCube Collaboration

J. C. Davis
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J. C. Davis
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IceCube Collaboration
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High Energy Astrophysical Phenomena (16)
 
High Energy Physics - Experiment (10)
 
Physics - Optics (7)
 
High Energy Physics - Phenomenology (6)
 
Physics - Mesoscopic Systems and Quantum Hall Effect (6)
 
Physics - Instrumentation and Detectors (5)
 
Physics - Strongly Correlated Electrons (4)
 
Physics - Superconductivity (4)
 
Nuclear Experiment (4)
 
Physics - Other (3)
 
Computer Science - Artificial Intelligence (3)
 
Mathematics - Logic (3)
 
Physics - Atomic Physics (2)
 
Cosmology and Nongalactic Astrophysics (2)
 
Instrumentation and Methods for Astrophysics (2)
 
Astrophysics of Galaxies (1)
 
Physics - Soft Condensed Matter (1)
 
General Relativity and Quantum Cosmology (1)
 
High Energy Physics - Theory (1)
 
Mathematics - Numerical Analysis (1)
 
Statistics - Machine Learning (1)
 
Quantum Physics (1)
 
Physics - Physics and Society (1)
 
Statistics - Computation (1)
 
Quantitative Biology - Quantitative Methods (1)
 
Physics - Materials Science (1)
 
Solar and Stellar Astrophysics (1)
 
Computer Science - Cryptography and Security (1)

Publications Authored By J. C. Davis

We present a new inference method based on approximate Bayesian computation for estimating parameters governing an entire network based on link-traced samples of that network. To do this, we first take summary statistics from an observed link-traced network sample, such as a recruitment network of subjects in a hard-to-reach population. Then we assume prior distributions, such as multivariate uniform, for the distribution of some parameters governing the structure of the network and behaviour of its nodes. Read More

Managing patients with multimorbidity often results in polypharmacy: the prescription of multiple drugs. However, the long-term effects of specific combinations of drugs and diseases are typically unknown. In particular, drugs prescribed for one condition may result in adverse effects for the other. Read More

In this paper, we advocate the use of stratified logical theories for representing probabilistic models. We argue that such encodings can be more interpretable than those obtained in existing frameworks such as Markov logic networks. Among others, this allows for the use of domain experts to improve learned models by directly removing, adding, or modifying logical formulas. Read More

In an effort to characterize the fast neutron radiation background, 16 EJ-309 liquid scintillator cells were installed in the Radiological Multi-sensor Analysis Platform (RadMAP) to collect data in the San Francisco Bay Area. Each fast neutron event was associated with specific weather metrics (pressure, temperature, absolute humidity) and GPS coordinates. The expected exponential dependence of the fast neutron count rate on atmospheric pressure was demonstrated and event rates were subsequently adjusted given the measured pressure at the time of detection. Read More

2016Nov
Authors: IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, C. Argüelles, T. C. Arlen, J. Auffenberg, S. Axani, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. -H. Becker, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, S. Blot, D. J. Boersma, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, A. Burgman, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz-Vélez, V. di Lorenzo, H. Dujmovic, J. P. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C. -C. Fösig, A. Franckowiak, T. Fuchs, T. K. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, W. Giang, L. Gladstone, M. Glagla, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Góra, D. Grant, Z. Griffith, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, M. Jurkovic, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, A. Kheirandish, M. Kim, T. Kintscher, J. Kiryluk, T. Kittler, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, M. Kroll, G. Krückl, C. Krüger, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, S. Mancina, M. Mandelartz, R. Maruyama, K. Mase, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, M. Moulai, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, Ö. Penek, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, L. Sabbatini, S. E. Sanchez Herrera, A. Sandrock, J. Sandroos, S. Sarkar, K. Satalecka, M. Schimp, P. Schlunder, T. Schmidt, S. Schoenen, S. Schöneberg, A. Schönwald, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, A. Stasik, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, M. van Rossem, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, S. Wickmann, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, H. Wissing, M. Wolf, T. R. Wood, E. Woolsey, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll

The recent discovery of a diffuse cosmic neutrino flux extending up to PeV energies raises the question of which astrophysical sources generate this signal. One class of extragalactic sources which may produce such high-energy neutrinos are blazars. We present a likelihood analysis searching for cumulative neutrino emission from blazars in the 2nd Fermi-LAT AGN catalogue (2LAC) using an IceCube neutrino dataset 2009-12 which was optimised for the detection of individual sources. Read More

We discuss the influence on spin-fluctuation pairing theory of orbital selective strong correlation effects in Fe-based superconductors, particularly Fe chalcogenide systems. We propose that a key ingredient for an improved itinerant pairing theory is orbital selectivity, i.e. Read More

FeSe is the focus of intense research interest because of its unusual non-magnetic nematic state and because it forms the basis for achieving the highest critical temperatures of any iron-based superconductor. However, its Cooper pairing mechanism has not been determined because an accurate knowledge of the momentum-space structure of superconducting energy gaps ${\Delta}_i (\vec{k})$ on the different electron-bands $E_i (\vec{k})$ does not exist. Here we use Bogoliubov quasiparticle interference (BQPI) imaging to determine the coherent Fermi surface geometry of the {\alpha}- and {\epsilon}-bands surrounding the ${\Gamma}=(0,0)$ and $X=({\pi}/a,0)$ points of FeSe, and to measure their superconducting energy gaps ${\Delta}_{\alpha} (\vec{k})$ and ${\Delta}_{\epsilon} (\vec{k})$. Read More

The EXO-200 Collaboration is searching for neutrinoless double beta decay using a liquid xenon (LXe) time projection chamber. This measurement relies on modeling the transport of charge deposits produced by interactions in the LXe to allow discrimination between signal and background events. Here we present measurements of the transverse diffusion constant and drift velocity of electrons at drift fields between 20~V/cm and 615~V/cm using EXO-200 data. Read More

The quantum mechanical propagator of a massive particle in a linear gravitational potential derived already in 1927 by Earle H. Kennard \cite{Kennard,Kennard2} contains a phase that scales with the third power of the time $T$ during which the particle experiences the corresponding force. Since in conventional atom interferometers the internal atomic states are all exposed to the same acceleration $a$, this $T^3$-phase cancels out and the interferometer phase scales as $T^2$. Read More

Theories based upon strong real space (r-space) electron electron interactions have long predicted that unidirectional charge density modulations (CDM) with four unit cell (4$a_0$) periodicity should occur in the hole doped cuprate Mott insulator (MI). Experimentally, however, increasing the hole density p is reported to cause the conventionally defined wavevector $Q_A$ of the CDM to evolve continuously as if driven primarily by momentum space (k-space) effects. Here we introduce phase resolved electronic structure visualization for determination of the cuprate CDM wavevector. Read More

While a vast amount of theoretical and experimental approaches can be used to study the band structure of simple solids, the investigation of the electronic properties of high-temperature superconductors and other strongly correlated systems is far less simple. Limitations to both theory and experiments arise from e.g. Read More

Micro and nanomechanical resonators with ultra-low dissipation have great potential as useful quantum resources. The superfluid micromechanical resonators presented here possess several advantageous characteristics: straightforward thermalization, dissipationless flow, and in situ tunability. We identify and quantitatively model the various dissipation mechanisms in two resonators, one fabricated from borosilicate glass and one from single crystal quartz. Read More

Heteronuclear multi-quantum spectroscopy is a powerful part of the NMR toolbox, commonly used to identify specific sequences of atoms in complex pulse sequences designed to determine the structure of complex molecules, including proteins. Optical coherent multidimensional spectroscopy (CMDS) is analogous to multidimensional NMR and many of the techniques of NMR have been adapted for application in the optical regime. This has been highly successful, with CMDS being used to understand energy transfer in photosynthesis and many body effects in semiconductor nanostructures amongst many other scientific breakthroughs. Read More

Biological datasets amenable to applied machine learning are more available today than ever before, yet they lack adequate representation in the Data-for-Good community. Here we present a work in progress case study performing analysis on antimicrobial resistance (AMR) using standard ensemble machine learning techniques and note the successes and pitfalls such work entails. Broadly, applied machine learning (AML) techniques are well suited to AMR, with classification accuracies ranging from mid-90% to low- 80% depending on sample size. Read More

Mechanical transduction of torque has been key to probing a number of physical phenomena, such as gravity, the angular momentum of light, the Casimir effect, magnetism, and quantum oscillations. Following similar trends as mass and force sensing, mechanical torque sensitivity can be dramatically improved by scaling down the physical dimensions, and therefore moment of inertia, of a torsional spring. Yet now, through precision nanofabrication and sub-wavelength cavity optomechanics, we have reached a point where geometric optimization can only provide marginal improvements to torque sensitivity. Read More

We quantify the amount of data needed in order to measure the size and position of the $^8$B neutrino production region within the solar core, for experiments looking at elastic scattering between electrons and solar neutrinos. The directions of the electrons immediately after scattering are strongly correlated with the incident directions of the neutrinos, however this is degraded significantly by the subsequent scattering of these electrons in the detector medium. We generate distributions of such electrons for different neutrino production profiles, and use a maximum likelihood analysis to make projections for future experimental sensitivity. Read More

2016Jun
Authors: IceCube collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, T. C. Arlen, J. Auffenberg, S. Axani, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. -H. Becker, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, S. Blot, D. J. Boersma, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, A. Burgman, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz-Vélez, V. di Lorenzo, H. Dujmovic, J. P. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C. -C. Fösig, A. Franckowiak, T. Fuchs, T. K. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, W. Giang, L. Gladstone, M. Glagla, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Góra, D. Grant, Z. Griffith, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, M. Jurkovic, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, A. Kheirandish, M. Kim, T. Kintscher, J. Kiryluk, T. Kittler, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, M. Kroll, G. Krückl, C. Krüger, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, S. Mancina, M. Mandelartz, R. Maruyama, K. Mase, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, M. Moulai, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, Ö. Penek, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, L. Sabbatini, S. E. Sanchez Herrera, A. Sandrock, J. Sandroos, S. Sarkar, K. Satalecka, M. Schimp, P. Schlunder, T. Schmidt, S. Schoenen, S. Schöneberg, A. Schönwald, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, A. Stasik, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, F. Tenholt, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, M. van Rossem, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, S. Wickmann, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, H. Wissing, M. Wolf, T. R. Wood, E. Woolsey, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll

We present the first IceCube search for a signal of dark matter annihilations in the Milky Way using all-flavour neutrino-induced particle cascades. The analysis focuses on the DeepCore sub-detector of IceCube, and uses the surrounding IceCube strings as a veto region in order to select starting events in the DeepCore volume. We use 329 live-days of data from IceCube operating in its 86-string configuration during 2011-2012. Read More

This thesis consists of two parts: the construction of a jointly universal family of graphs, and then an exploration of set-theoretic geology. Firstly we shall construct a model in which $2^{\aleph_{\omega_1}}=2^{\aleph_{\omega_1+1}}=\aleph_{\omega_1+3}$ but there is a jointly universal family of size $\aleph_{\omega_1+2}$ of graphs on $\aleph_{\omega_1+1}$. We take a supercompact cardinal $\kappa$ and will use Radin forcing with interleaved collapses to change $\kappa$ into $\aleph_{\omega_1}$. Read More

Dark excitons are of fundamental importance in a broad range of contexts, but are difficult to study using conventional optical spectroscopy due to their weak interaction with light. We show how coherent multidimensional spectroscopy can reveal and characterize dark states. Using this approach, we identify different types of dark excitons in InGaAs/GaAs quantum wells and determine details regarding lifetimes, homogeneous and inhomogeneous linewidths, broadening mechanisms and coupling strengths. Read More

The energy resolution of the EXO-200 detector is limited by electronics noise in the measurement of the scintillation response. Here we present a new technique to extract optimal scintillation energy measurements for signals split across multiple channels in the presence of correlated noise. The implementation of these techniques improves the energy resolution of the detector at the neutrinoless double beta decay Q-value from $\left[1. Read More

Starting from a supercompact cardinal we build a model in which $2^{\aleph_{\omega_1}}=2^{\aleph_{\omega_1+1}}=\aleph_{\omega_1+3}$ but there is a jointly universal family of size $\aleph_{\omega_1+2}$ of graphs on $\aleph_{\omega_1+1}$. The same technique will work for any uncountable cardinal in place of $\omega_1$. Read More

This paper provides an accessible introduction to some of the work of Woodin on suitable extender models. We define the HOD conjecture, prove it is equivalent to a formulation in terms of weak extender models for supercompactness, and give some of its consequences. Read More

2016Apr
Authors: IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, T. C. Arlen, J. Auffenberg, S. Axani, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. -H. Becker, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, S. Blot, D. J. Boersma, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, A. Burgman, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz-Vélez, V. di Lorenzo, H. Dujmovic, J. P. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C. -C. Fösig, T. Fuchs, T. K. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, L. Gladstone, M. Glagla, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Góra, D. Grant, Z. Griffith, C. Ha, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, M. Jurkovic, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, A. Kheirandish, M. Kim, T. Kintscher, J. Kiryluk, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, M. Kroll, G. Krückl, C. Krüger, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, S. Mancina, M. Mandelartz, R. Maruyama, K. Mase, H. S. Matis, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, M. Moulai, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, Ö. Penek, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, L. Sabbatini, A. Sandrock, J. Sandroos, S. Sarkar, K. Satalecka, M. Schimp, P. Schlunder, T. Schmidt, S. Schoenen, S. Schöneberg, A. Schönwald, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, A. Stasik, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, M. van Rossem, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, N. Whitehorn, S. Wickmann, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll

Observation of a point source of astrophysical neutrinos would be a "smoking gun" signature of a cosmic-ray accelerator. While IceCube has recently discovered a diffuse flux of astrophysical neutrinos, no localized point source has been observed. Previous IceCube searches for point sources in the southern sky were restricted by either an energy threshold above a few hundred TeV or poor neutrino angular resolution. Read More

A supernova event in our own galaxy will result in a large number of neutrinos detected on Earth within the time-frame of a few seconds. These neutrinos will have been produced thermally with, in principle, three distinct temperatures for the electron, anti-electron and remaining heavy flavours respectively. We revisit the possibility that new MeV-mass particles $\chi$ are also produced thermally during the event, which scatter with the neutrinos and alter their temperatures. Read More

We introduce a setting for learning possibilistic logic theories from defaults of the form "if alpha then typically beta". We first analyse this problem from the point of view of machine learning theory, determining the VC dimension of possibilistic stratifications as well as the complexity of the associated learning problems, after which we present a heuristic learning algorithm that can easily scale to thousands of defaults. An important property of our approach is that it is inherently able to handle noisy and conflicting sets of defaults. Read More

This paper proposes a method to completely hide the functionality of a digital standard cell. This is accomplished by a differential threshold logic gate (TLG). A TLG with $n$ inputs implements a subset of Boolean functions of $n$ variables that are linear threshold functions. Read More

2016Mar
Authors: IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, T. C. Arlen, J. Auffenberg, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. -H. Becker, E. Beiser, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz-Vélez, V. di Lorenzo, H. Dujmovic, J. P. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C. -C. Fösig, T. Fuchs, T. K. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, D. Gier, L. Gladstone, M. Glagla, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Góra, D. Grant, Z. Griffith, C. Ha, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, M. Jurkovic, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, A. Kheirandish, M. Kim, T. Kintscher, J. Kiryluk, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, G. Kroll, M. Kroll, G. Krückl, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, M. Mandelartz, R. Maruyama, K. Mase, H. S. Matis, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, L. Paul, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, S. Richter, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, L. Sabbatini, H. -G. Sander, A. Sandrock, J. Sandroos, S. Sarkar, K. Schatto, M. Schimp, P. Schlunder, T. Schmidt, S. Schoenen, S. Schöneberg, A. Schönwald, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, A. Stasik, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll

The IceCube Neutrino Observatory has accumulated a total of 318 billion cosmic-ray induced muon events between May 2009 and May 2015. This data set was used for a detailed analysis of the cosmic-ray arrival direction anisotropy in the TeV to PeV energy range. The observed global anisotropy features large regions of relative excess and deficit, with amplitudes on the order of $10^{-3}$ up to about 100 TeV. Read More

2016Feb
Authors: S. Adrián-Martínez1, A. Albert2, M. André3, G. Anton4, M. Ardid5, J. -J. Aubert6, T. Avgitas7, B. Baret8, J. Barrios-Martí9, S. Basa10, V. Bertin11, S. Biagi12, R. Bormuth13, M. C. Bouwhuis14, R. Bruijn15, J. Brunner16, J. Busto17, A. Capone18, L. Caramete19, J. Carr20, S. Celli21, T. Chiarusi22, M. Circella23, A. Coleiro24, R. Coniglione25, H. Costantini26, P. Coyle27, A. Creusot28, A. Deschamps29, G. De Bonis30, C. Distefano31, C. Donzaud32, D. Dornic33, D. Drouhin34, T. Eberl35, I. El Bojaddaini36, D. Elsässer37, A. Enzenhöfer38, K. Fehn39, I. Felis40, L. A. Fusco41, S. Galatà42, P. Gay43, S. Geißelsöder44, K. Geyer45, V. Giordano46, V. Giordano47, A. Gleixner48, H. Glotin49, R. Gracia-Ruiz50, K. Graf51, S. Hallmann52, H. van Haren53, A. J. Heijboer54, Y. Hello55, J. J. Hernández-Rey56, J. Hößl57, J. Hofestädt58, C. Hugon59, G. Illuminati60, C. W James61, M. de Jong62, M. Jongen63, M. Kadler64, O. Kalekin65, U. Katz66, D. Kießling67, A. Kouchner68, M. Kreter69, I. Kreykenbohm70, V. Kulikovskiy71, C. Lachaud72, R. Lahmann73, D. Lefèvre74, E. Leonora75, S. Loucatos76, M. Marcelin77, A. Margiotta78, A. Marinelli79, J. A. Martínez-Mora80, A. Mathieu81, K. Melis82, T. Michael83, P. Migliozzi84, A. Moussa85, C. Mueller86, E. Nezri87, G. E. Păvălaş88, C. Pellegrino89, C. Perrina90, P. Piattelli91, V. Popa92, T. Pradier93, C. Racca94, G. Riccobene95, K. Roensch96, M. Saldaña97, D. F. E. Samtleben98, M. Sanguineti99, P. Sapienza100, J. Schnabel101, F. Schüssler102, T. Seitz103, C. Sieger104, M. Spurio105, Th. Stolarczyk106, A. Sánchez-Losa107, M. Taiuti108, A. Trovato109, M. Tselengidou110, D. Turpin111, C. T\112, B. Vallage113, C. Vallée114, V. Van Elewyck115, D. Vivolo116, S. Wagner117, J. Wilms118, J. D. Zornoza119, J. Zúñiga120, . M. G. Aartsen121, K. Abraham122, M. Ackermann123, J. Adams124, J. A. Aguilar125, M. Ahlers126, M. Ahrens127, D. Altmann128, T. Anderson129, I. Ansseau130, G. Anton131, M. Archinger132, C. Arguelles133, T. C. Arlen134, J. Auffenberg135, X. Bai136, S. W. Barwick137, V. Baum138, R. Bay139, J. J. Beatty140, J. Becker Tjus141, K. -H. Becker142, E. Beiser143, S. BenZvi144, P. Berghaus145, D. Berley146, E. Bernardini147, A. Bernhard148, D. Z. Besson149, G. Binder150, D. Bindig151, M. Bissok152, E. Blaufuss153, J. Blumenthal154, D. J. Boersma155, C. Bohm156, M. Börner157, F. Bos158, D. Bose159, S. Böser160, O. Botner161, J. Braun162, L. Brayeur163, H. -P. Bretz164, N. Buzinsky165, J. Casey166, M. Casier167, E. Cheung168, D. Chirkin169, A. Christov170, K. Clark171, L. Classen172, S. Coenders173, G. H. Collin174, J. M. Conrad175, D. F. Cowen176, A. H. Cruz Silva177, J. Daughhetee178, J. C. Davis179, M. Day180, J. P. A. M. de André181, C. De Clercq182, E. del Pino Rosendo183, H. Dembinski184, S. De Ridder185, P. Desiati186, K. D. de Vries187, G. de Wasseige188, M. de With189, T. DeYoung190, J. C. Díaz-Vélez191, V. di Lorenzo192, H. Dujmovic193, J. P. Dumm194, M. Dunkman195, B. Eberhardt196, T. Ehrhardt197, B. Eichmann198, S. Euler199, P. A. Evenson200, S. Fahey201, A. R. Fazely202, J. Feintzeig203, J. Felde204, K. Filimonov205, C. Finley206, S. Flis207, C. -C. Fösig208, T. Fuchs209, T. K. Gaisser210, R. Gaior211, J. Gallagher212, L. Gerhardt213, K. Ghorbani214, D. Gier215, L. Gladstone216, M. Glagla217, T. Glüsenkamp218, A. Goldschmidt219, G. Golup220, J. G. Gonzalez221, D. Góra222, D. Grant223, Z. Griffith224, C. Ha225, C. Haack226, A. Haj Ismail227, A. Hallgren228, F. Halzen229, E. Hansen230, B. Hansmann231, T. Hansmann232, K. Hanson233, D. Hebecker234, D. Heereman235, K. Helbing236, R. Hellauer237, S. Hickford238, J. Hignight239, G. C. Hill240, K. D. Hoffman241, R. Hoffmann242, K. Holzapfel243, A. Homeier244, K. Hoshina245, F. Huang246, M. Huber247, W. Huelsnitz248, P. O. Hulth249, K. Hultqvist250, S. In251, A. Ishihara252, E. Jacobi253, G. S. Japaridze254, M. Jeong255, K. Jero256, B. J. P. Jones257, M. Jurkovic258, A. Kappes259, T. Karg260, A. Karle261, U. Katz262, M. Kauer263, A. Keivani264, J. L. Kelley265, J. Kemp266, A. Kheirandish267, M. Kim268, T. Kintscher269, J. Kiryluk270, S. R. Klein271, G. Kohnen272, R. Koirala273, H. Kolanoski274, R. Konietz275, L. Köpke276, C. Kopper277, S. Kopper278, D. J. Koskinen279, M. Kowalski280, K. Krings281, G. Kroll282, M. Kroll283, G. Krückl284, J. Kunnen285, S. Kunwar286, N. Kurahashi287, T. Kuwabara288, M. Labare289, J. L. Lanfranchi290, M. J. Larson291, D. Lennarz292, M. Lesiak-Bzdak293, M. Leuermann294, J. Leuner295, L. Lu296, J. Lünemann297, J. Madsen298, G. Maggi299, K. B. M. Mahn300, M. Mandelartz301, R. Maruyama302, K. Mase303, H. S. Matis304, R. Maunu305, F. McNally306, K. Meagher307, M. Medici308, M. Meier309, A. Meli310, T. Menne311, G. Merino312, T. Meures313, S. Miarecki314, E. Middell315, L. Mohrmann316, T. Montaruli317, R. Morse318, R. Nahnhauer319, U. Naumann320, G. Neer321, H. Niederhausen322, S. C. Nowicki323, D. R. Nygren324, A. Obertacke Pollmann325, A. Olivas326, A. Omairat327, A. O'Murchadha328, T. Palczewski329, H. Pandya330, D. V. Pankova331, L. Paul332, J. A. Pepper333, C. Pérez de los Heros334, C. Pfendner335, D. Pieloth336, E. Pinat337, J. Posselt338, P. B. Price339, G. T. Przybylski340, M. Quinnan341, C. Raab342, L. Rädel343, M. Rameez344, K. Rawlins345, R. Reimann346, M. Relich347, E. Resconi348, W. Rhode349, M. Richman350, S. Richter351, B. Riedel352, S. Robertson353, M. Rongen354, C. Rott355, T. Ruhe356, D. Ryckbosch357, L. Sabbatini358, H. -G. Sander359, A. Sandrock360, J. Sandroos361, S. Sarkar362, K. Schatto363, M. Schimp364, P. Schlunder365, T. Schmidt366, S. Schoenen367, S. Schöneberg368, A. Schönwald369, L. Schumacher370, D. Seckel371, S. Seunarine372, D. Soldin373, M. Song374, G. M. Spiczak375, C. Spiering376, M. Stahlberg377, M. Stamatikos378, T. Stanev379, A. Stasik380, A. Steuer381, T. Stezelberger382, R. G. Stokstad383, A. Stößl384, R. Ström385, N. L. Strotjohann386, G. W. Sullivan387, M. Sutherland388, H. Taavola389, I. Taboada390, J. Tatar391, S. Ter-Antonyan392, A. Terliuk393, G. Tešić394, S. Tilav395, P. A. Toale396, M. N. Tobin397, S. Toscano398, D. Tosi399, M. Tselengidou400, A. Turcati401, E. Unger402, M. Usner403, S. Vallecorsa404, J. Vandenbroucke405, N. van Eijndhoven406, S. Vanheule407, J. van Santen408, J. Veenkamp409, M. Vehring410, M. Voge411, M. Vraeghe412, C. Walck413, A. Wallace414, M. Wallraff415, N. Wandkowsky416, Ch. Weaver417, C. Wendt418, S. Westerhoff419, B. J. Whelan420, K. Wiebe421, C. H. Wiebusch422, L. Wille423, D. R. Williams424, L. Wills425, H. Wissing426, M. Wolf427, T. R. Wood428, K. Woschnagg429, D. L. Xu430, X. W. Xu431, Y. Xu432, J. P. Yanez433, G. Yodh434, S. Yoshida435, M. Zoll436, . B. P. Abbott437, R. Abbott438, T. D. Abbott439, M. R. Abernathy440, F. Acernese441, K. Ackley442, C. Adams443, T. Adams444, P. Addesso445, R. X. Adhikari446, V. B. Adya447, C. Affeldt448, M. Agathos449, K. Agatsuma450, N. Aggarwal451, O. D. Aguiar452, L. Aiello453, A. Ain454, P. Ajith455, B. Allen456, A. Allocca457, P. A. Altin458, S. B. Anderson459, W. G. Anderson460, K. Arai461, M. C. Araya462, C. C. Arceneaux463, J. S. Areeda464, N. Arnaud465, K. G. Arun466, S. Ascenzi467, G. Ashton468, M. Ast469, S. M. Aston470, P. Astone471, P. Aufmuth472, C. Aulbert473, S. Babak474, P. Bacon475, M. K. M. Bader476, P. T. Baker477, F. Baldaccini478, G. Ballardin479, S. W. Ballmer480, J. C. Barayoga481, S. E. Barclay482, B. C. Barish483, D. Barker484, F. Barone485, B. Barr486, L. Barsotti487, M. Barsuglia488, D. Barta489, J. Bartlett490, I. Bartos491, R. Bassiri492, A. Basti493, J. C. Batch494, C. Baune495, V. Bavigadda496, M. Bazzan497, B. Behnke498, M. Bejger499, A. S. Bell500, C. J. Bell501, B. K. Berger502, J. Bergman503, G. Bergmann504, C. P. L. Berry505, D. Bersanetti506, A. Bertolini507, J. Betzwieser508, S. Bhagwat509, R. Bhandare510, I. A. Bilenko511, G. Billingsley512, J. Birch513, R. Birney514, S. Biscans515, A. Bisht516, M. Bitossi517, C. Biwer518, M. A. Bizouard519, J. K. Blackburn520, C. D. Blair521, D. G. Blair522, R. M. Blair523, S. Bloemen524, O. Bock525, T. P. Bodiya526, M. Boer527, G. Bogaert528, C. Bogan529, A. Bohe530, P. Bojtos531, C. Bond532, F. Bondu533, R. Bonnand534, B. A. Boom535, R. Bork536, V. Boschi537, S. Bose538, Y. Bouffanais539, A. Bozzi540, C. Bradaschia541, P. R. Brady542, V. B. Braginsky543, M. Branchesi544, J. E. Brau545, T. Briant546, A. Brillet547, M. Brinkmann548, V. Brisson549, P. Brockill550, A. F. Brooks551, D. D. Brown552, N. M. Brown553, C. C. Buchanan554, A. Buikema555, T. Bulik556, H. J. Bulten557, A. Buonanno558, D. Buskulic559, C. Buy560, R. L. Byer561, L. Cadonati562, G. Cagnoli563, C. Cahillane564, J. Calderón Bustillo565, T. Callister566, E. Calloni567, J. B. Camp568, K. C. Cannon569, J. Cao570, C. D. Capano571, E. Capocasa572, F. Carbognani573, S. Caride574, J. Casanueva Diaz575, C. Casentini576, S. Caudill577, M. Cavaglià578, F. Cavalier579, R. Cavalieri580, G. Cella581, C. B. Cepeda582, L. Cerboni Baiardi583, G. Cerretani584, E. Cesarini585, R. Chakraborty586, T. Chalermsongsak587, S. J. Chamberlin588, M. Chan589, S. Chao590, P. Charlton591, E. Chassande-Mottin592, H. Y. Chen593, Y. Chen594, C. Cheng595, A. Chincarini596, A. Chiummo597, H. S. Cho598, M. Cho599, J. H. Chow600, N. Christensen601, Q. Chu602, S. Chua603, S. Chung604, G. Ciani605, F. Clara606, J. A. Clark607, F. Cleva608, E. Coccia609, P. -F. Cohadon610, A. Colla611, C. G. Collette612, L. Cominsky613, M. Constancio Jr.614, A. Conte615, L. Conti616, D. Cook617, T. R. Corbitt618, N. Cornish619, A. Corsi620, S. Cortese621, C. A. Costa622, M. W. Coughlin623, S. B. Coughlin624, J. -P. Coulon625, S. T. Countryman626, P. Couvares627, E. E. Cowan628, D. M. Coward629, M. J. Cowart630, D. C. Coyne631, R. Coyne632, K. Craig633, J. D. E. Creighton634, J. Cripe635, S. G. Crowder636, A. Cumming637, L. Cunningham638, E. Cuoco639, T. Dal Canton640, S. L. Danilishin641, S. D'Antonio642, K. Danzmann643, N. S. Darman644, V. Dattilo645, I. Dave646, H. P. Daveloza647, M. Davier648, G. S. Davies649, E. J. Daw650, R. Day651, D. DeBra652, G. Debreczeni653, J. Degallaix654, M. De Laurentis655, S. Deléglise656, W. Del Pozzo657, T. Denker658, H. Dereli659, V. Dergachev660, R. T. DeRosa661, R. De Rosa662, R. DeSalvo663, S. Dhurandhar664, M. C. Díaz665, L. Di Fiore666, M. Di Giovanni667, A. Di Lieto668, S. Di Pace669, I. Di Palma670, A. Di Virgilio671, G. Dojcinoski672, V. Dolique673, F. Donovan674, K. L. Dooley675, S. Doravari676, R. Douglas677, T. P. Downes678, M. Drago679, R. W. P. Drever680, J. C. Driggers681, Z. Du682, M. Ducrot683, S. E. Dwyer684, T. B. Edo685, M. C. Edwards686, A. Effler687, H. -B. Eggenstein688, P. Ehrens689, J. Eichholz690, S. S. Eikenberry691, W. Engels692, R. C. Essick693, T. Etzel694, M. Evans695, T. M. Evans696, R. Everett697, M. Factourovich698, V. Fafone699, H. Fair700, S. Fairhurst701, X. Fan702, Q. Fang703, S. Farinon704, B. Farr705, W. M. Farr706, M. Favata707, M. Fays708, H. Fehrmann709, M. M. Fejer710, I. Ferrante711, E. C. Ferreira712, F. Ferrini713, F. Fidecaro714, I. Fiori715, D. Fiorucci716, R. P. Fisher717, R. Flaminio718, M. Fletcher719, J. -D. Fournier720, S. Franco721, S. Frasca722, F. Frasconi723, Z. Frei724, A. Freise725, R. Frey726, V. Frey727, T. T. Fricke728, P. Fritschel729, V. V. Frolov730, P. Fulda731, M. Fyffe732, H. A. G. Gabbard733, J. R. Gair734, L. Gammaitoni735, S. G. Gaonkar736, F. Garufi737, A. Gatto738, G. Gaur739, N. Gehrels740, G. Gemme741, B. Gendre742, E. Genin743, A. Gennai744, J. George745, L. Gergely746, V. Germain747, Archisman Ghosh748, S. Ghosh749, J. A. Giaime750, K. D. Giardina751, A. Giazotto752, K. Gill753, A. Glaefke754, E. Goetz755, R. Goetz756, L. Gondan757, G. González758, J. M. Gonzalez Castro759, A. Gopakumar760, N. A. Gordon761, M. L. Gorodetsky762, S. E. Gossan763, M. Gosselin764, R. Gouaty765, C. Graef766, P. B. Graff767, M. Granata768, A. Grant769, S. Gras770, C. Gray771, G. Greco772, A. C. Green773, P. 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Isogai840, B. R. Iyer841, K. Izumi842, T. Jacqmin843, H. Jang844, K. Jani845, P. Jaranowski846, S. Jawahar847, F. Jiménez-Forteza848, W. W. Johnson849, D. I. Jones850, R. Jones851, R. J. G. Jonker852, L. Ju853, Haris K854, C. V. Kalaghatgi855, V. Kalogera856, S. Kandhasamy857, G. Kang858, J. B. Kanner859, S. Karki860, M. Kasprzack861, E. Katsavounidis862, W. Katzman863, S. Kaufer864, T. Kaur865, K. Kawabe866, F. Kawazoe867, F. Kéfélian868, M. S. Kehl869, D. Keitel870, D. B. Kelley871, W. Kells872, R. Kennedy873, J. S. Key874, A. Khalaidovski875, F. Y. Khalili876, I. Khan877, S. Khan878, Z. Khan879, E. A. Khazanov880, N. Kijbunchoo881, C. Kim882, J. Kim883, K. Kim884, Nam-Gyu Kim885, Namjun Kim886, Y. -M. Kim887, E. J. King888, P. J. King889, D. L. Kinzel890, J. S. Kissel891, L. Kleybolte892, S. Klimenko893, S. M. Koehlenbeck894, K. Kokeyama895, S. Koley896, V. Kondrashov897, A. Kontos898, M. Korobko899, W. Z. Korth900, I. Kowalska901, D. B. Kozak902, V. Kringel903, B. Krishnan904, A. 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Markosyan970, E. Maros971, F. Martelli972, L. Martellini973, I. W. Martin974, R. M. Martin975, D. V. Martynov976, J. N. Marx977, K. Mason978, A. Masserot979, T. J. Massinger980, M. Masso-Reid981, F. Matichard982, L. Matone983, N. Mavalvala984, N. Mazumder985, G. Mazzolo986, R. McCarthy987, D. E. McClelland988, S. McCormick989, S. C. McGuire990, G. McIntyre991, J. McIver992, D. J. McManus993, S. T. McWilliams994, D. Meacher995, G. D. Meadors996, J. Meidam997, A. Melatos998, G. Mendell999, D. Mendoza-Gandara1000, R. A. Mercer1001, E. Merilh1002, M. Merzougui1003, S. Meshkov1004, C. Messenger1005, C. Messick1006, P. M. Meyers1007, F. Mezzani1008, H. Miao1009, C. Michel1010, H. Middleton1011, E. E. Mikhailov1012, L. Milano1013, J. Miller1014, M. Millhouse1015, Y. Minenkov1016, J. Ming1017, S. Mirshekari1018, C. Mishra1019, S. Mitra1020, V. P. Mitrofanov1021, G. Mitselmakher1022, R. Mittleman1023, A. Moggi1024, M. Mohan1025, S. R. P. Mohapatra1026, M. Montani1027, B. C. Moore1028, C. J. 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Rakhmanov1148, P. Rapagnani1149, V. Raymond1150, M. Razzano1151, V. Re1152, J. Read1153, C. M. Reed1154, T. Regimbau1155, L. Rei1156, S. Reid1157, D. H. Reitze1158, H. Rew1159, S. D. Reyes1160, F. Ricci1161, K. Riles1162, N. A. Robertson1163, R. Robie1164, F. Robinet1165, A. Rocchi1166, L. Rolland1167, J. G. Rollins1168, V. J. Roma1169, J. D. Romano1170, R. Romano1171, G. Romanov1172, J. H. Romie1173, D. Rosińska1174, S. Rowan1175, A. Rüdiger1176, P. Ruggi1177, K. Ryan1178, S. Sachdev1179, T. Sadecki1180, L. Sadeghian1181, L. Salconi1182, M. Saleem1183, F. Salemi1184, A. Samajdar1185, L. Sammut1186, E. J. Sanchez1187, V. Sandberg1188, B. Sandeen1189, J. R. Sanders1190, B. Sassolas1191, B. S. Sathyaprakash1192, P. R. Saulson1193, O. Sauter1194, R. L. Savage1195, A. Sawadsky1196, P. Schale1197, R. Schilling1198, J. Schmidt1199, P. Schmidt1200, R. Schnabel1201, R. M. S. Schofield1202, A. Schönbeck1203, E. Schreiber1204, D. Schuette1205, B. F. Schutz1206, J. Scott1207, S. M. Scott1208, D. Sellers1209, A. S. Sengupta1210, D. Sentenac1211, V. Sequino1212, A. Sergeev1213, G. Serna1214, Y. Setyawati1215, A. Sevigny1216, D. A. Shaddock1217, S. Shah1218, M. S. Shahriar1219, M. Shaltev1220, Z. Shao1221, B. Shapiro1222, P. Shawhan1223, A. Sheperd1224, D. H. Shoemaker1225, D. M. Shoemaker1226, K. Siellez1227, X. Siemens1228, D. Sigg1229, A. D. Silva1230, D. Simakov1231, A. Singer1232, L. P. Singer1233, A. Singh1234, R. Singh1235, A. Singhal1236, A. M. Sintes1237, B. J. J. Slagmolen1238, J. R. Smith1239, N. D. Smith1240, R. J. E. Smith1241, E. J. Son1242, B. Sorazu1243, F. Sorrentino1244, T. Souradeep1245, A. K. Srivastava1246, A. Staley1247, M. Steinke1248, J. Steinlechner1249, S. Steinlechner1250, D. Steinmeyer1251, B. C. Stephens1252, R. Stone1253, K. A. Strain1254, N. Straniero1255, G. Stratta1256, N. A. Strauss1257, S. Strigin1258, R. Sturani1259, A. L. Stuver1260, T. Z. Summerscales1261, L. Sun1262, P. J. Sutton1263, B. L. Swinkels1264, M. J. Szczepańczyk1265, M. Tacca1266, D. Talukder1267, D. B. Tanner1268, M. Tápai1269, S. P. Tarabrin1270, A. Taracchini1271, R. Taylor1272, T. Theeg1273, M. P. Thirugnanasambandam1274, E. G. Thomas1275, M. Thomas1276, P. Thomas1277, K. A. Thorne1278, K. S. Thorne1279, E. Thrane1280, S. Tiwari1281, V. Tiwari1282, K. V. Tokmakov1283, C. Tomlinson1284, M. Tonelli1285, C. V. Torres1286, C. I. Torrie1287, D. Töyrä1288, F. Travasso1289, G. Traylor1290, D. Trifirò1291, M. C. Tringali1292, L. Trozzo1293, M. Tse1294, M. Turconi1295, D. Tuyenbayev1296, D. Ugolini1297, C. S. Unnikrishnan1298, A. L. Urban1299, S. A. Usman1300, H. Vahlbruch1301, G. Vajente1302, G. Valdes1303, N. van Bakel1304, M. van Beuzekom1305, J. F. J. van den Brand1306, C. Van Den Broeck1307, D. C. Vander-Hyde1308, L. van der Schaaf1309, J. V. van Heijningen1310, A. A. van Veggel1311, M. Vardaro1312, S. Vass1313, M. Vasúth1314, R. Vaulin1315, A. Vecchio1316, G. Vedovato1317, J. Veitch1318, P. J. Veitch1319, K. Venkateswara1320, D. Verkindt1321, F. 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Zhang1386, M. Zhang1387, Y. Zhang1388, C. Zhao1389, M. Zhou1390, Z. Zhou1391, X. J. Zhu1392, M. E. Zucker1393, S. E. Zuraw1394, J. Zweizig1395
Affiliations: 1ANTARES Collaboration, 2ANTARES Collaboration, 3ANTARES Collaboration, 4ANTARES Collaboration, 5ANTARES Collaboration, 6ANTARES Collaboration, 7ANTARES Collaboration, 8ANTARES Collaboration, 9ANTARES Collaboration, 10ANTARES Collaboration, 11ANTARES Collaboration, 12ANTARES Collaboration, 13ANTARES Collaboration, 14ANTARES Collaboration, 15ANTARES Collaboration, 16ANTARES Collaboration, 17ANTARES Collaboration, 18ANTARES Collaboration, 19ANTARES Collaboration, 20ANTARES Collaboration, 21ANTARES Collaboration, 22ANTARES Collaboration, 23ANTARES Collaboration, 24ANTARES Collaboration, 25ANTARES Collaboration, 26ANTARES Collaboration, 27ANTARES Collaboration, 28ANTARES Collaboration, 29ANTARES Collaboration, 30ANTARES Collaboration, 31ANTARES Collaboration, 32ANTARES Collaboration, 33ANTARES Collaboration, 34ANTARES Collaboration, 35ANTARES Collaboration, 36ANTARES Collaboration, 37ANTARES Collaboration, 38ANTARES Collaboration, 39ANTARES Collaboration, 40ANTARES Collaboration, 41ANTARES Collaboration, 42ANTARES Collaboration, 43ANTARES Collaboration, 44ANTARES Collaboration, 45ANTARES Collaboration, 46ANTARES Collaboration, 47ANTARES Collaboration, 48ANTARES Collaboration, 49ANTARES Collaboration, 50ANTARES Collaboration, 51ANTARES Collaboration, 52ANTARES Collaboration, 53ANTARES Collaboration, 54ANTARES Collaboration, 55ANTARES Collaboration, 56ANTARES Collaboration, 57ANTARES Collaboration, 58ANTARES Collaboration, 59ANTARES Collaboration, 60ANTARES Collaboration, 61ANTARES Collaboration, 62ANTARES Collaboration, 63ANTARES Collaboration, 64ANTARES Collaboration, 65ANTARES Collaboration, 66ANTARES Collaboration, 67ANTARES Collaboration, 68ANTARES Collaboration, 69ANTARES Collaboration, 70ANTARES Collaboration, 71ANTARES Collaboration, 72ANTARES Collaboration, 73ANTARES Collaboration, 74ANTARES Collaboration, 75ANTARES Collaboration, 76ANTARES Collaboration, 77ANTARES Collaboration, 78ANTARES Collaboration, 79ANTARES Collaboration, 80ANTARES Collaboration, 81ANTARES Collaboration, 82ANTARES Collaboration, 83ANTARES Collaboration, 84ANTARES Collaboration, 85ANTARES Collaboration, 86ANTARES Collaboration, 87ANTARES Collaboration, 88ANTARES Collaboration, 89ANTARES Collaboration, 90ANTARES Collaboration, 91ANTARES Collaboration, 92ANTARES Collaboration, 93ANTARES Collaboration, 94ANTARES Collaboration, 95ANTARES Collaboration, 96ANTARES Collaboration, 97ANTARES Collaboration, 98ANTARES Collaboration, 99ANTARES Collaboration, 100ANTARES Collaboration, 101ANTARES Collaboration, 102ANTARES Collaboration, 103ANTARES Collaboration, 104ANTARES Collaboration, 105ANTARES Collaboration, 106ANTARES Collaboration, 107ANTARES Collaboration, 108ANTARES Collaboration, 109ANTARES Collaboration, 110ANTARES Collaboration, 111ANTARES Collaboration, 112ANTARES Collaboration, 113ANTARES Collaboration, 114ANTARES Collaboration, 115ANTARES Collaboration, 116ANTARES Collaboration, 117ANTARES Collaboration, 118ANTARES Collaboration, 119ANTARES Collaboration, 120ANTARES Collaboration, 121IceCube Collaboration, 122IceCube Collaboration, 123IceCube Collaboration, 124IceCube Collaboration, 125IceCube Collaboration, 126IceCube Collaboration, 127IceCube Collaboration, 128IceCube Collaboration, 129IceCube Collaboration, 130IceCube Collaboration, 131IceCube Collaboration, 132IceCube Collaboration, 133IceCube Collaboration, 134IceCube Collaboration, 135IceCube Collaboration, 136IceCube Collaboration, 137IceCube Collaboration, 138IceCube Collaboration, 139IceCube Collaboration, 140IceCube Collaboration, 141IceCube Collaboration, 142IceCube Collaboration, 143IceCube Collaboration, 144IceCube Collaboration, 145IceCube Collaboration, 146IceCube Collaboration, 147IceCube Collaboration, 148IceCube Collaboration, 149IceCube Collaboration, 150IceCube Collaboration, 151IceCube Collaboration, 152IceCube Collaboration, 153IceCube Collaboration, 154IceCube Collaboration, 155IceCube Collaboration, 156IceCube Collaboration, 157IceCube Collaboration, 158IceCube Collaboration, 159IceCube Collaboration, 160IceCube Collaboration, 161IceCube Collaboration, 162IceCube Collaboration, 163IceCube Collaboration, 164IceCube Collaboration, 165IceCube Collaboration, 166IceCube Collaboration, 167IceCube Collaboration, 168IceCube Collaboration, 169IceCube Collaboration, 170IceCube Collaboration, 171IceCube Collaboration, 172IceCube Collaboration, 173IceCube Collaboration, 174IceCube Collaboration, 175IceCube Collaboration, 176IceCube Collaboration, 177IceCube Collaboration, 178IceCube Collaboration, 179IceCube Collaboration, 180IceCube Collaboration, 181IceCube Collaboration, 182IceCube Collaboration, 183IceCube Collaboration, 184IceCube Collaboration, 185IceCube Collaboration, 186IceCube Collaboration, 187IceCube Collaboration, 188IceCube Collaboration, 189IceCube Collaboration, 190IceCube Collaboration, 191IceCube Collaboration, 192IceCube Collaboration, 193IceCube Collaboration, 194IceCube Collaboration, 195IceCube Collaboration, 196IceCube Collaboration, 197IceCube Collaboration, 198IceCube Collaboration, 199IceCube Collaboration, 200IceCube Collaboration, 201IceCube Collaboration, 202IceCube Collaboration, 203IceCube Collaboration, 204IceCube Collaboration, 205IceCube Collaboration, 206IceCube Collaboration, 207IceCube Collaboration, 208IceCube Collaboration, 209IceCube Collaboration, 210IceCube Collaboration, 211IceCube Collaboration, 212IceCube Collaboration, 213IceCube Collaboration, 214IceCube Collaboration, 215IceCube Collaboration, 216IceCube Collaboration, 217IceCube Collaboration, 218IceCube Collaboration, 219IceCube Collaboration, 220IceCube Collaboration, 221IceCube Collaboration, 222IceCube Collaboration, 223IceCube Collaboration, 224IceCube Collaboration, 225IceCube Collaboration, 226IceCube Collaboration, 227IceCube Collaboration, 228IceCube Collaboration, 229IceCube Collaboration, 230IceCube Collaboration, 231IceCube Collaboration, 232IceCube Collaboration, 233IceCube Collaboration, 234IceCube Collaboration, 235IceCube Collaboration, 236IceCube Collaboration, 237IceCube Collaboration, 238IceCube Collaboration, 239IceCube Collaboration, 240IceCube Collaboration, 241IceCube Collaboration, 242IceCube Collaboration, 243IceCube Collaboration, 244IceCube Collaboration, 245IceCube Collaboration, 246IceCube Collaboration, 247IceCube Collaboration, 248IceCube Collaboration, 249IceCube Collaboration, 250IceCube Collaboration, 251IceCube Collaboration, 252IceCube Collaboration, 253IceCube Collaboration, 254IceCube Collaboration, 255IceCube Collaboration, 256IceCube Collaboration, 257IceCube Collaboration, 258IceCube Collaboration, 259IceCube Collaboration, 260IceCube Collaboration, 261IceCube Collaboration, 262IceCube Collaboration, 263IceCube Collaboration, 264IceCube Collaboration, 265IceCube Collaboration, 266IceCube Collaboration, 267IceCube Collaboration, 268IceCube Collaboration, 269IceCube Collaboration, 270IceCube Collaboration, 271IceCube Collaboration, 272IceCube Collaboration, 273IceCube Collaboration, 274IceCube Collaboration, 275IceCube Collaboration, 276IceCube Collaboration, 277IceCube Collaboration, 278IceCube Collaboration, 279IceCube Collaboration, 280IceCube Collaboration, 281IceCube Collaboration, 282IceCube Collaboration, 283IceCube Collaboration, 284IceCube Collaboration, 285IceCube Collaboration, 286IceCube Collaboration, 287IceCube Collaboration, 288IceCube Collaboration, 289IceCube Collaboration, 290IceCube Collaboration, 291IceCube Collaboration, 292IceCube Collaboration, 293IceCube Collaboration, 294IceCube Collaboration, 295IceCube Collaboration, 296IceCube Collaboration, 297IceCube Collaboration, 298IceCube Collaboration, 299IceCube Collaboration, 300IceCube Collaboration, 301IceCube Collaboration, 302IceCube Collaboration, 303IceCube Collaboration, 304IceCube Collaboration, 305IceCube Collaboration, 306IceCube Collaboration, 307IceCube Collaboration, 308IceCube Collaboration, 309IceCube Collaboration, 310IceCube Collaboration, 311IceCube Collaboration, 312IceCube Collaboration, 313IceCube Collaboration, 314IceCube Collaboration, 315IceCube Collaboration, 316IceCube Collaboration, 317IceCube Collaboration, 318IceCube Collaboration, 319IceCube Collaboration, 320IceCube Collaboration, 321IceCube Collaboration, 322IceCube Collaboration, 323IceCube Collaboration, 324IceCube Collaboration, 325IceCube Collaboration, 326IceCube Collaboration, 327IceCube Collaboration, 328IceCube Collaboration, 329IceCube Collaboration, 330IceCube Collaboration, 331IceCube Collaboration, 332IceCube Collaboration, 333IceCube Collaboration, 334IceCube Collaboration, 335IceCube Collaboration, 336IceCube Collaboration, 337IceCube Collaboration, 338IceCube Collaboration, 339IceCube Collaboration, 340IceCube Collaboration, 341IceCube Collaboration, 342IceCube Collaboration, 343IceCube Collaboration, 344IceCube Collaboration, 345IceCube Collaboration, 346IceCube Collaboration, 347IceCube Collaboration, 348IceCube Collaboration, 349IceCube Collaboration, 350IceCube Collaboration, 351IceCube Collaboration, 352IceCube Collaboration, 353IceCube Collaboration, 354IceCube Collaboration, 355IceCube Collaboration, 356IceCube Collaboration, 357IceCube Collaboration, 358IceCube Collaboration, 359IceCube Collaboration, 360IceCube Collaboration, 361IceCube Collaboration, 362IceCube Collaboration, 363IceCube Collaboration, 364IceCube Collaboration, 365IceCube Collaboration, 366IceCube Collaboration, 367IceCube Collaboration, 368IceCube Collaboration, 369IceCube Collaboration, 370IceCube Collaboration, 371IceCube Collaboration, 372IceCube Collaboration, 373IceCube Collaboration, 374IceCube Collaboration, 375IceCube Collaboration, 376IceCube Collaboration, 377IceCube Collaboration, 378IceCube Collaboration, 379IceCube Collaboration, 380IceCube Collaboration, 381IceCube Collaboration, 382IceCube Collaboration, 383IceCube Collaboration, 384IceCube Collaboration, 385IceCube Collaboration, 386IceCube Collaboration, 387IceCube Collaboration, 388IceCube Collaboration, 389IceCube Collaboration, 390IceCube Collaboration, 391IceCube Collaboration, 392IceCube Collaboration, 393IceCube Collaboration, 394IceCube Collaboration, 395IceCube Collaboration, 396IceCube Collaboration, 397IceCube Collaboration, 398IceCube Collaboration, 399IceCube Collaboration, 400IceCube Collaboration, 401IceCube Collaboration, 402IceCube Collaboration, 403IceCube Collaboration, 404IceCube Collaboration, 405IceCube Collaboration, 406IceCube Collaboration, 407IceCube Collaboration, 408IceCube Collaboration, 409IceCube Collaboration, 410IceCube Collaboration, 411IceCube Collaboration, 412IceCube Collaboration, 413IceCube Collaboration, 414IceCube Collaboration, 415IceCube Collaboration, 416IceCube Collaboration, 417IceCube Collaboration, 418IceCube Collaboration, 419IceCube Collaboration, 420IceCube Collaboration, 421IceCube Collaboration, 422IceCube Collaboration, 423IceCube Collaboration, 424IceCube Collaboration, 425IceCube Collaboration, 426IceCube Collaboration, 427IceCube Collaboration, 428IceCube Collaboration, 429IceCube Collaboration, 430IceCube Collaboration, 431IceCube Collaboration, 432IceCube Collaboration, 433IceCube Collaboration, 434IceCube Collaboration, 435IceCube Collaboration, 436IceCube Collaboration, 437ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 438ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 439ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 440ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 441ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 442ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 443ANTARES Collaboration, IceCube 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Collaboration, 1355ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1356ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1357ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1358ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1359ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1360ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1361ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1362ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1363ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1364ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1365ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1366ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1367ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1368ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1369ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1370ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1371ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1372ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1373ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1374ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1375ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1376ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1377ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1378ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1379ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1380ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1381ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1382ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1383ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1384ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1385ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1386ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1387ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1388ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1389ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1390ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1391ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1392ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1393ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1394ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, 1395ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration

We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on Sept. 14th, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and ANTARES neutrino detectors. Read More

We identify carrier scattering at densities below which it has previously been observed in semiconductor quantum wells. These effects are evident in the peakshapes of 2D double-quantum spectra, which change as a function of excitation density. At high excitation densities ($\geq 10^{9}$ carriers/,cm$^{-2}$) we observe untilted peaks similar to those reported in previous experiments. Read More

A search for Lorentz- and CPT-violating signals in the double beta decay spectrum of $^{136}$Xe has been performed using an exposure of 100 kg$\cdot$yr with the EXO-200 detector. No significant evidence of the spectral modification due to isotropic Lorentz-violation was found, and a two-sided limit of $-2.65 \times 10^{-5 } \; \textrm{GeV} < \mathring{a}^{(3)}_{\text{of}} < 7. Read More

2016Jan
Authors: IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, T. C. Arlen, J. Auffenberg, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. -H. Becker, E. Beiser, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz-Vélez, V. di Lorenzo, H. Dujmovic, J. P. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C. -C. Fösig, T. Fuchs, T. K. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, D. Gier, L. Gladstone, M. Glagla, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Góra, D. Grant, Z. Griffith, C. Ha, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, M. Jurkovic, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, A. Kheirandish, M. Kim, T. Kintscher, J. Kiryluk, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, G. Kroll, M. Kroll, G. Krückl, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, M. Mandelartz, R. Maruyama, K. Mase, H. S. Matis, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, L. Paul, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, S. Richter, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, L. Sabbatini, H. -G. Sander, A. Sandrock, J. Sandroos, S. Sarkar, K. Schatto, M. Schimp, P. Schlunder, T. Schmidt, S. Schoenen, S. Schöneberg, A. Schönwald, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, A. Stasik, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll

We present the results and methodology of a search for neutrinos produced in the decay of charged pions created in interactions between protons and gamma-rays during the prompt emission of 807 gamma-ray bursts (GRBs) over the entire sky. This three-year search is the first in IceCube for shower-like Cherenkov light patterns from electron, muon, and tau neutrinos correlated with GRBs. We detect five low-significance events correlated with five GRBs. Read More

We investigate the robustness of the resonance like feature centred at around a 750 GeV invariant mass in the 13 TeV diphoton data, recently released by the ATLAS collaboration. We focus on the choice of empirical function used to model the continuum diphoton background in order to quantify the uncertainties in the analysis due to this choice. We extend the function chosen by the ATLAS collaboration to one with two components. Read More

We report on the development of on-chip microcavities and show their potential as a platform for cavity quantum electrodynamics experiments. Microcavity arrays were formed by the controlled buckling of SiO2/Ta2O5 Bragg mirrors, and exhibit a reflectance-limited finesse of 3500 and mode volumes as small as 35lambda^3. We show that the cavity resonance can be thermally tuned into alignment with the D2 transition of 87Rb, and outline two methods for providing atom access to the cavity. Read More

2016Jan
Authors: IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, T. C. Arlen, J. Auffenberg, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. -H. Becker, E. Beiser, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen, A. H. Cruz Silva, M. Danninger, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz-Vélez, V. di Lorenzo, J. P. Dumm, M. Dunkman, B. Eberhardt, J. Edsjö, T. Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C. -C. Fösig, T. Fuchs, T. K. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, D. Gier, L. Gladstone, M. Glagla, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Góra, D. Grant, Z. Griffith, A. Groß, C. Ha, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, M. Jurkovic, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, A. Kheirandish, J. Kiryluk, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, G. Kroll, M. Kroll, G. Krückl, J. Kunnen, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, M. Mandelartz, R. Maruyama, K. Mase, H. S. Matis, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, L. Paul, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, S. Richter, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, L. Sabbatini, H. -G. Sander, A. Sandrock, J. Sandroos, S. Sarkar, C. Savage, K. Schatto, M. Schimp, P. Schlunder, T. Schmidt, S. Schoenen, S. Schöneberg, A. Schönwald, L. Schulte, L. Schumacher, P. Scott, D. Seckel, S. Seunarine, H. Silverwood, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, A. Stasik, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll

We present an improved event-level likelihood formalism for including neutrino telescope data in global fits to new physics. We derive limits on spin-dependent dark matter-proton scattering by employing the new formalism in a re-analysis of data from the 79-string IceCube search for dark matter annihilation in the Sun, including explicit energy information for each event. The new analysis excludes a number of models in the weak-scale minimal supersymmetric standard model (MSSM) for the first time. Read More

As neutrinoless double-beta decay experiments become more sensitive and intrinsic radioactivity in detector materials is reduced, previously minor contributions to the background must be understood and eliminated. With this in mind, cosmogenic backgrounds have been studied with the EXO-200 experiment. Using the EXO-200 TPC, the muon flux (through a flat horizontal surface) underground at the Waste Isolation Pilot Plant (WIPP) has been measured to be {\Phi} = 4. Read More

Despite its continued observational successes, there is a persistent (and growing) interest in extending cosmology beyond the standard model, $\Lambda$CDM. This is motivated by a range of apparently serious theoretical issues, involving such questions as the cosmological constant problem, the particle nature of dark matter, the validity of general relativity on large scales, the existence of anomalies in the CMB and on small scales, and the predictivity and testability of the inflationary paradigm. In this paper, we summarize the current status of $\Lambda$CDM as a physical theory, and review investigations into possible alternatives along a number of different lines, with a particular focus on highlighting the most promising directions. Read More

2015Nov
Authors: The IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, I. Ansseau, M. Archinger, C. Arguelles, T. C. Arlen, J. Auffenberg, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K. -H. Becker, E. Beiser, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Díaz-Vélez, V. di Lorenzo, J. P. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, T. Fischer-Wasels, S. Flis, C. -C. Fösig, T. Fuchs, T. K. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, D. Gier, L. Gladstone, M. Glagla, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Góra, D. Grant, Z. Griffith, A. Groß, C. Ha, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, M. Jurkovic, A. Kappes, T. Karg, A. Karle, M. Kauer, A. Keivani, J. L. Kelley, J. Kemp, A. Kheirandish, J. Kiryluk, J. Kläs, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, G. Kroll, M. Kroll, G. Krückl, J. Kunnen, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, M. Mandelartz, R. Maruyama, K. Mase, H. S. Matis, R. Maunu, F. McNally, K. Meagher, M. Medici, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, L. Paul, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, S. Richter, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, L. Sabbatini, H. -G. Sander, A. Sandrock, J. Sandroos, S. Sarkar, K. Schatto, M. Schimp, T. Schmidt, S. Schoenen, S. Schöneberg, A. Schönwald, L. Schulte, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, A. Stasik, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, C. Wendt, S. Westerhoff, B. J. Whelan, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll. The Pierre Auger Collaboration, :, A. Aab, P. Abreu, M. Aglietta, E. J. Ahn, I. Al Samarai, I. F. M. Albuquerque, I. Allekotte, P. Allison, A. Almela, J. Alvarez Castillo, J. Alvarez-Muñiz, R. Alves Batista, M. Ambrosio, A. Aminaei, L. Anchordoqui, B. Andrada, S. Andringa, C. Aramo, F. Arqueros, N. Arsene, H. Asorey, P. Assis, J. Aublin, G. Avila, N. Awal, A. M. Badescu, C. Baus, J. J. Beatty, K. H. Becker, J. A. Bellido, C. Berat, M. E. Bertaina, X. Bertou, P. L. Biermann, P. Billoir, S. G. Blaess, A. Blanco, M. Blanco, J. Blazek, C. Bleve, H. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, N. Borodai, A. M. Botti, J. Brack, I. Brancus, T. Bretz, A. Bridgeman, F. L. Briechle, P. Buchholz, A. Bueno, S. Buitink, M. Buscemi, K. S. Caballero-Mora, B. Caccianiga, L. Caccianiga, M. Candusso, L. Caramete, R. Caruso, A. Castellina, G. Cataldi, L. Cazon, R. Cester, A. G. Chavez, A. Chiavassa, J. A. Chinellato, J. C. Chirinos Diaz, J. Chudoba, R. W. Clay, R. Colalillo, A. Coleman, L. Collica, M. R. Coluccia, R. Conceição, F. Contreras, M. J. Cooper, A. Cordier, S. Coutu, C. E. Covault, R. Dallier, S. D'Amico, B. Daniel, S. Dasso, K. 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Tsutsumi, Y. Uchihori, S. Udo, F. Urban, G. Vasiloff, T. Wong, R. Yamane, H. Yamaoka, K. Yamazaki, J. Yang, K. Yashiro, Y. Yoneda, S. Yoshida, H. Yoshii, R. Zollinger, Z. Zundel

This paper presents the results of different searches for correlations between very high-energy neutrino candidates detected by IceCube and the highest-energy cosmic rays measured by the Pierre Auger Observatory and the Telescope Array. We first consider samples of cascade neutrino events and of high-energy neutrino-induced muon tracks, which provided evidence for a neutrino flux of astrophysical origin, and study their cross-correlation with the ultrahigh-energy cosmic ray (UHECR) samples as a function of angular separation. We also study their possible directional correlations using a likelihood method stacking the neutrino arrival directions and adopting different assumptions on the size of the UHECR magnetic deflections. Read More

The quantum condensate of Cooper-pairs forming a superconductor was originally conceived to be translationally invariant. In theory, however, pairs can exist with finite momentum $Q$ and thereby generate states with spatially modulating Cooper-pair density. While never observed directly in any superconductor, such a state has been created in ultra-cold $^{6}$Li gas. Read More