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1. Supporting Cyber Security of Power Distribution Systems by Detecting Differences Between Real-time Micro-Synchrophasor Measurements and Cyber-Reported SCADA (Final Report)

Author: Anna Scaglione, C. P. McParland, Aaron Snyder, Reinhard Gentz, Sean Peisert, Alex McEachren, Galen Rasche, Ciaran Roberts, and Mahdi Jamei
Subjects: Distribution system, Power (social and political), SCADA, Computer science, Mahdi, Computer security, computer.software_genre, computer
Abstract: Author(s): Peisert, Sean; Roberts, Ciaran; Scaglione, Anna; Jamei, Mahdi; Gentz, Reinhard; Mcparland, Charles; McEachren, Alex; Rasche, Galen; Snyder, Aaron
Published: 2020

2. OpenHiCAMM: High-Content Screening Software for Complex Microscope Imaging Workflows

Author: William W. Fisher, Benjamin W. Booth, Susan E. Celniker, Keith Beattie, Ann S. Hammonds, Erwin Frise, and C. P. McParland
Subjects: 0301 basic medicine, Microscope, Computer science, Systems biology, ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION, Bioengineering, Image processing, Article, law.invention, 03 medical and health sciences, 0302 clinical medicine, Software, law, lcsh:Science, Multidisciplinary, business.industry, Robotics, 3. Good health, Range (mathematics), 030104 developmental biology, Workflow, Networking and Information Technology R&D (NITRD), High-content screening, Biomedical Imaging, lcsh:Q, Generic health relevance, Artificial intelligence, business, 030217 neurology & neurosurgery, Computer hardware
Abstract: SUMMARY High-content image acquisition is generally limited to cells grown in culture, requiring complex hardware and preset imaging modalities. Here we report an open source software package, OpenHiCAMM (Open Hi Content Acquisition for μManager), that provides a flexible framework for integration of generic microscope-associated robotics and image processing with sequential work-flows. As an example, we imaged Drosophila embryos, detecting the embryos at low resolution, followed by re-imaging the detected embryos at high resolution, suitable for computational analysis and screening. The OpenHiCAMM package is easy to use and adapt for automating complex microscope image tasks. It expands our abilities for high-throughput image-based screens to a new range of biological samples, such as organoids, and will provide a foundation for bioimaging systems biology., Graphical abstract
Published: 2018

3. NEUTRINO ASTRONOMY AND COSMIC RAYS AT THE SOUTH POLE: LATEST RESULTS FROM AMANDA AND PERSPECTIVES FOR ICECUBE

Author: P. Ekström, P. Berghaus, M. Kestel, T. DeYoung, D. Z. Besson, T. J. Sumner, R. H. Minor, A. R. Fazely, S. Böser, Kael Hanson, S. Patton, P. Niessen, I. Taboada, R. G. Stokstad, T. Castermans, Carlos Pena-Garay, K. Hultqvist, R. Wischnewski, R. Hardtke, J. K. Becker, C. Pérez de los Heros, T. Becka, Yi Wang, Paolo Desiati, D. R. Nygren, P. O. Hulth, D. Steele, R. W. Ellsworth, T. Hauschildt, Johan Lundberg, S. Schlenstedt, T. Straszheim, Adam Bouchta, J. L. Kelley, Christian Bohm, David A. Schneider, Allan Hallgren, H. Wissing, P. Miocinovic, D.W. Atlee, Kyle T. Mandli, J. Cavin, J. W. Nam, George Japaridze, R. Ganugapati, D. Hays, L. Thollander, D. F. Cowen, A. Achterberg, Jodi Cooley, D. Berley, G. C. Hill, R. Porrata, Marek Kowalski, A. Silvestri, R. Paulos, S. H. Seo, T. Stezelberger, J. Yeck, Elisa Resconi, Hakki Ögelman, A. C. Pohl, Pawel Marciniewski, H. Leich, J. Pretz, P. B. Price, Peter Mészáros, S. Stoyanov, R. Ehrlich, D. Seckel, E. Blaufuss, D. J. Boersma, S. Hundertmark, M. Krasberg, M. Hellwig, H. G. Sander, B. Collin, K. Rawlins, Heiko Geenen, Torsten Harenberg, D. Hardtke, M. Ribordy, K. Helbing, Kurt Woschnagg, R. Koch, I. Liubarsky, Christian Spiering, Ph. Olbrechts, C. T. Day, J. Hodges, James Madsen, Paul Evenson, G. W. Sullivan, James E. Braun, S. Richter, J. Rodríguez Martino, C. H. Wiebusch, K. Münich, N. Langer, C. De Clercq, A. W. Jones, John Clem, Soebur Razzaque, L. Gerhardt, Dmitry Chirkin, M. Solarz, Olga Botner, S. Yoshida, T. Neunhöffer, Albrecht Karle, T. Messarius, Anna Davour, Justin Vandenbroucke, Elisa Bernardini, M. Bartelt, A. J. Smith, R. M. Gunasingha, J. Ahrens, Y. Minaeva, Markus Ackermann, S. W. Barwick, W. R. Edwards, R. Morse, N. Kitamura, D. Bertrand, William Carithers, R. Schwarz, C.P. Burgess, M. Walter, T. Burgess, Todor Stanev, Janet Jacobsen, J. A. Coarasa, R. Nahnhauer, R. C. Bay, H. Miyamoto, Xinhua Bai, John N. Bahcall, Jean Gallagher, Glenn Spiczak, S. R. Klein, A. Gross, L. C. Voicu, G. Kohnen, Othmane Bouhali, B. Hughey, K. H. Sulanke, Michael Stamatikos, D. Turčan, C. Walck, J. M. Joseph, Thomas K. Gaisser, G. B. Yodh, Wolfgang Wagner, K. Kuehn, W. Chinowsky, N. van Eijndhoven, K. Schinarakis, Gerald Przybylski, H. S. Matis, Matthias Leuthold, P. Herquet, P. Steffen, J. E. Sopher, Francis Halzen, Jan Conrad, T. Feser, O. Tarasova, K. Hoshina, Wolfgang Rhode, D. Hubert, L. Köpke, J. Bergmans, S. Tilav, K. H. Kampert, H. Kawai, C. P. McParland, E. Kujawski, A. Goldschmidt, K.-H. Becker, and H. Albrecht
Subjects: Physics, Nuclear and High Energy Physics, Photomultiplier, Astronomy, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Solar neutrino problem, Atomic and Molecular Physics, and Optics, Coincidence, law.invention, Telescope, Neutrino detector, law, Neutrino astronomy, Neutrino
Abstract: The AMANDA neutrino telescope has been in operation at the South Pole since 1996. The present final array configuration, operational since 2000, consists of 677 photomultiplier tubes arranged in 19 strings, buried at depths between 1500 and 2000 m in the ice. The most recent results on a multi-year search for point sources of neutrinos will be shown. The study of events triggered in coincidence with the surface array SPASE and AMANDA provided a result on cosmic ray composition. Expected improvements from IceCube/IceTop will also be discussed.
Published: 2005

4. Results from the AMANDA neutrino telescope

Author: P. Niessen, I. Taboada, Y. Minaeva, C.P. Burgess, D. Bertrand, P. Ekström, K. Rawlins, T. Becka, James Madsen, M. Kestel, J. L. Kelley, C. P. McParland, T. DeYoung, P. B. Price, T. Burgess, T. Neunhöffer, M. Ribordy, A. Karle, A. Goldschmidt, S. Böser, Elisa Resconi, Gerald Przybylski, R. Porrata, Kurt Woschnagg, A. Silvestri, D. Steele, Glenn Spiczak, D. F. Cowen, A. Gross, L. Gerhardt, Dmitry Chirkin, T. Messarius, D. J. Boersma, Torsten Harenberg, Othmane Bouhali, Ph. Olbrecht, Hakki Ögelman, B. Hughey, J. W. Nam, Matthias Leuthold, D. R. Nygren, M. Solarz, K. Helbing, Kyle T. Mandli, P. Steffen, J. Rodríguez Martino, R. C. Bay, Jan Conrad, T. Feser, S. Tilav, R. Nahnhauer, J. Ahrens, C. H. Wiebusch, R. Ganugapati, C. Walck, R. Hardtke, J. K. Becker, Olga Botner, L. Thollander, T. Hauschildt, David A. Schneider, C. Spiering, Thomas K. Gaisser, G. B. Yodh, M. Bartelt, P. Miocinovic, Adam Bouchta, C.P. de los Heros, Allan Hallgren, G. C. Hill, K. Münich, Heiko Geenen, Xinhua Bai, K.-H. Becker, T. Castermans, K. Hultqvist, H. Albrecht, C. De Clercq, Karl-Heinz Sulanke, Markus Ackermann, S. W. Barwick, S. Hundertmark, James E. Braun, M. Walter, Ph. Herquet, Kael Hanson, Yi Wang, Paolo Desiati, M. Krasberg, H. Leich, S. Schlenstedt, Joseph T. Hodges, H. S. Matis, Francis Halzen, K. Kuehn, K. Schinarakis, Jodi Cooley, S. Richter, M. Hellwig, H. G. Sander, B. Collin, D. Hubert, I. Liubarsky, L. Köpke, R. Morse, K. H. Kampert, R. Schwarz, Wolfgang Rhode, M. Kowalski, Elisa Bernardini, R. G. Stokstad, R. Wischnewski, Michael Stamatikos, P. O. Hulth, H. Wissing, Wolfgang Wagner, A. C. Pohl, Pawel Marciniewski, Anna Davour, and Janet Jacobsen
Subjects: Physics, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, High Energy Physics::Phenomenology, Dark matter, Astronomy, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Solar neutrino problem, Atomic and Molecular Physics, and Optics, law.invention, Telescope, Neutrino detector, law, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino astronomy, Neutrino
Abstract: The Amanda neutrino telescope at the South Pole has been taking data since 1996. Stepwise upgraded, it reached its final stage in January 2000. We present results from the search for extraterrestrial neutrinos, neutrinos from dark matter annihilation and magnetic monopoles.
Published: 2004

5. Measurement of the cosmic ray composition at the knee with the SPASE-2/AMANDA-B10 detectors

Author: T. Messarius, M. Solarz, A. Silvestri, Freddy Binon, T. Burgess, S. Böser, J. P Dewulf, P. B. Price, A. C. Pohl, Y. Minaeva, R. Schwarz, Hakki Ögelman, J. Rodríguez Martino, Kyle T. Mandli, I. Taboada, D. Bertrand, T. O. B. Schmidt, J. Ahrens, K. Rawlins, D. J. Boersma, A. Biron, Kurt Woschnagg, P. Ekström, R. Nahnhauer, M. Hellwig, Matthias Leuthold, Paul Evenson, D. R. Nygren, E. Andres, H. G. Sander, P. Steffen, C. P. McParland, Dmitry Chirkin, Michael Stamatikos, James Madsen, Jan Conrad, T. Feser, R. Porrata, T. DeYoung, Staffan Carius, I. Liubarsky, M. Ribordy, Xinhua Bai, L. Gerhardt, A. Goldschmidt, Gerald Przybylski, Glenn Spiczak, D. Ross, R. Engel, K.-H. Becker, K. H. Sulanke, B. Hughey, T. Neunhöffer, R. Hardtke, T. Becka, M. Gaug, James Kim, Albrecht Karle, R. Morse, R. C. Bay, P. Niessen, Todor Stanev, Yajun Wang, S. Schlenstedt, R. Ganugapati, D. Hubert, C. Wiedemann, Olga Botner, D. Steele, C. Walck, Ph. Herquet, S. Tilav, P. C. Mock, D. F. Cowen, Marek Kowalski, P. Miocinovic, Kael Hanson, Thomas K. Gaisser, G. B. Yodh, L. Köpke, Paolo Desiati, Ph. Olbrechts, H. Leich, C. Pérez de los Heros, T. Castermans, Wolfgang Rhode, C. De Clercq, Christopher Wiebusch, Markus Ackermann, S. W. Barwick, Othmane Bouhali, W. Wu, David A. Schneider, G. C. Hill, Heiko Geenen, Pawel Marciniewski, Anna Davour, Janet Jacobsen, Wolfgang Wagner, P. O. Hulth, H. Wissing, Elisa Bernardini, Jim Hinton, R. G. Stokstad, R. Wischnewski, P. Lindahl, Christian Spiering, S. Hundertmark, K. Rochester, K. Kuehn, Alan Watson, J. I. Lamoureux, K. Schinarakis, Jodi Cooley, T. Hauschildt, K. Hultqvist, S. Young, T. Miller, J. Lloyd-Evans, Adam Bouchta, S. Richter, H. S. Matis, Allan Hallgren, Francis Halzen, E. Dickinson, and Elisa Resconi
Subjects: Astroparticle physics, Physics, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Cosmic Rays, Mass composition, Neutrino astronomy, Atomic mass, Air shower, Ultra-high-energy cosmic ray, Neutrino, Cherenkov radiation
Abstract: The mass composition of high-energy cosmic rays at energies above 1015 eV can provide crucial information for the understanding of their origin. Air showers were measured simultaneously with the SPASE-2 air shower array and the AMANDA-B10 Cherenkov telescope at the South Pole. This combination has the advantage to sample almost all high-energy shower muons and is thus a new approach to the determination of the cosmic ray composition. The change in the cosmic ray mass composition was measured versus existing data from direct measurements at low energies. Our data show an increase of the mean log atomic mass 〈lnA〉 by about 0.8 between 500 TeV and 5 PeV. This trend of an increasing mass through the "knee" region is robust against a variety of systematic effects. © 2004 Elsevier B.V. All rights reserved.
Published: 2004

6. Muon track reconstruction and data selection techniques in AMANDA

Author: P. B. Price, T. O. B. Schmidt, C. Pérez de los Heros, T. Becka, M. Kestel, Kurt Woschnagg, T. DeYoung, Dmitry Chirkin, Staffan Carius, D. Steele, S. Böser, Jodi Cooley, Matthias Leuthold, Elisa Bernardini, D. R. Nygren, R. Ganugapati, P. Herquet, D. F. Cowen, Marek Kowalski, P. Steffen, M. Solarz, Jan Conrad, T. Feser, S. Richter, I. Taboada, T. Castermans, H. S. Matis, K. Rawlins, M. Hellwig, P. Miocinovic, Yajun Wang, H. G. Sander, Francis Halzen, Michael Stamatikos, S. Schlenstedt, C. P. McParland, R. Hardtke, Markus Gaug, B. Collin, D. J. Boersma, James Madsen, C. Wiedemann, A. Goldschmidt, I. Liubarsky, David A. Schneider, A. Silvestri, J. P Dewulf, G. C. Hill, R. G. Stokstad, C. H. Wiebusch, Hakki Ögelman, R. Wischnewski, P. Lindahl, Christian Spiering, Y. Minaeva, R. C. Bay, K.-H. Becker, M. Ribordy, K. Helbing, Heiko Geenen, R. Nahnhauer, J. Rodríguez Martino, K. Kuehn, K. Schinarakis, T. Burgess, Othmane Bouhali, T. Messarius, R. Morse, L. Gerhardt, J. Ahrens, Ph. Olbrechts, K. Münich, K. Hultqvist, T. Neunhöffer, Albrecht Karle, A. Biron, Glenn Spiczak, Xinhua Bai, J. W. Nam, L. Thollander, B. Hughey, H. Leich, S. Tilav, P. C. Mock, R. Schwarz, Kael Hanson, Paolo Desiati, R. Porrata, A. C. Pohl, Gerald Przybylski, K. H. Sulanke, Olga Botner, D. Bertrand, C. De Clercq, S. W. Barwick, C. Walck, Thomas K. Gaisser, G. B. Yodh, Torsten Harenberg, Elisa Resconi, J. K. Becker, T. Hauschildt, Adam Bouchta, Allan Hallgren, Ole Streicher, S. Hundertmark, J. I. Lamoureux, P. Niessen, D. Hubert, Axel Groß, L. Köpke, D. Ross, Pawel Marciniewski, Anna Davour, Janet Jacobsen, Wolfgang Wagner, P. O. Hulth, H. Wissing, Wolfgang Rhode, and P. Ekström
Subjects: Antarctic Muon And Neutrino Detector Array, Physics, AMANDA, Nuclear and High Energy Physics, Particle physics, Neutrino astrophysics, Neutrino telescope, Track reconstruction, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), Detector, FOS: Physical sciences, Astrophysics, IceCube Neutrino Observatory, Neutrino detector, High Energy Physics::Experiment, Muon neutrino, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Instrumentation, Lepton
Abstract: The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500m and 2000m. The primary goal of this detector is to discover astrophysical sources of high energy neutrinos. A high-energy muon neutrino coming through the earth from the Northern Hemisphere can be identified by the secondary muon moving upward through the detector. The muon tracks are reconstructed with a maximum likelihood method. It models the arrival times and amplitudes of Cherenkov photons registered by the photo-multipliers. This paper describes the different methods of reconstruction, which have been successfully implemented within AMANDA. Strategies for optimizing the reconstruction performance and rejecting background are presented. For a typical analysis procedure the direction of tracks are reconstructed with about 2 degree accuracy., 40 pages, 16 Postscript figures, uses elsart.sty
Published: 2004

7. Calibration and survey of AMANDA with the SPASE detectors

Author: G. M. Splczak, Yajun Wang, S. Schlenstedt, P. Niessen, D. Bertrand, C. Wiedemann, I. Taboada, R. C. Bay, L. Gerhardt, P. Ekström, David A. Schneider, Ph. Herquet, T. Becka, C. Pérez de los Heros, Xinhua Bai, T. Messarius, G. C. Hill, Kael Hanson, C. Wiebusch, S. Böser, Todor Stanev, Staffan Carius, K. Rawlins, R. Schwarz, Ph. Olbrechts, Heiko Geenen, Matthias Leuthold, D. R. Nygren, M. Gaug, James Madsen, Paolo Desiati, K. H. Sulanke, D. Steele, P. Steffen, Jodi Cooley, R. Porrata, R. Ganugapati, C. P. McParland, R. Engel, A. Biron, Elisa Bernardini, Hakki Ögelman, Jan Conrad, T. Feser, Kyle T. Mandli, D. F. Cowen, S. Young, Marek Kowalski, P. B. Price, Jim Hinton, A. Goldschmidt, Gerald Przybylski, A. Silvestri, T. O. B. Schmidt, M. Ribordy, M. Hellwig, H. G. Sander, Kurt Woschnagg, L. Köpke, Paul Evenson, B. Hughey, T. Neunhöffer, James Kim, Albrecht Karle, Y. Minaeva, R. Hardtke, Dmitry Chirkin, R. G. Stokstad, K.-H. Becker, R. Wischnewski, S. Richter, I. Liubarsky, J. Rodríguez Martino, Ch. Weinheimer, H. Leich, T. DeYoung, Othmane Bouhali, P. Miocinovic, Wolfgang Rhode, J. Ahrens, A. C. Pohl, Michael Stamatikos, W. Wu, R. Morse, D. Ross, S. Tilav, P. C. Mock, K. Kuehn, K. Schinarakis, H. S. Matis, Freddy Binon, T. Burgess, Francis Halzen, Olga Botner, P. Lindahl, Christian Spiering, K. Rochester, Alan Watson, P. O. Hulth, H. Wissing, Wolfgang Wagner, M. Solarz, Pawel Marciniewski, T. Hauschildt, Anna Davour, J. Lloyd-Evans, Janet Jacobsen, K. Hultqvist, Adam Bouchta, Allan Hallgren, P. Romenesko, Elisa Resconi, D. Martello, T. Castermans, C. De Clercq, S. W. Barwick, C. Walck, Thomas K. Gaisser, G. B. Yodh, S. Hundertmark, J. I. Lamoureux, T. C. Miller, and P. Doksus
Subjects: Antarctic Muon And Neutrino Detector Array, Physics, Nuclear and High Energy Physics, Muon, Detector, Astronomy, Cosmic ray, Particle detector, Air shower, Neutrino detector, Cosmic rays, Neutrino telescopes, Coincident, Instrumentation
Abstract: We report on the analysis of air showers observed in coincidence by the Antarctic Muon and Neutrino detector array (AMANDA-B10) and the South Pole Air Shower Experiment (SPASE-1 and SPASE-2). We discuss the use of coincident events for calibration and survey of the deep AMANDA detector as well as the response of AMANDA to muon bundles. This analysis uses data taken during 1997 when both SPASE-1 and SPASE-2 were in operation to provide a stereo view of AMANDA. © 2003 Elsevier B.V. All rights reserved.
Published: 2004

8. Status of the IceCube Neutrino Observatory

Author: Olga Botner, C. Pérez de los Heros, John N. Bahcall, T. Becka, Othmane Bouhali, K. Hultqvist, R. C. Bay, K. Rawlins, S. Yoshida, M. Ribordy, N. van Eijndhoven, Gerald Przybylski, W Carithers, A. C. Pohl, S. Hundertmark, J. Cavin, A. W. Jones, James Madsen, D. Steele, H. Kawai, C. P. McParland, H. S. Matis, Ph. Herquet, J. I. Lamoureux, G. W. Sullivan, Soebur Razzaque, R. Paulos, R. G. Stokstad, Anna Davour, A. Goldschmidt, R. Wischnewski, J. Pretz, Ph. Olbrechts, Francis Halzen, R. H. Minor, Kael Hanson, R. Ganugapati, T. Hauschildt, Janet Jacobsen, D. F. Cowen, M. Solarz, Marek Kowalski, K.-H. Becker, Adam Bouchta, R. Schwarz, R. M. Gunasingha, Y. Minaeva, S. Patton, P. B. Price, Paolo Desiati, Allan Hallgren, R.-R Wang, Christian Bohm, Michael Stamatikos, R. Hardtke, George Japaridze, David A. Schneider, J. A. Goodman, Kurt Woschnagg, Hakki Ögelman, P. Niessen, D. Hubert, Wolfgang Wagner, K. Helbing, D. Berley, G. C. Hill, Paul Evenson, Todor Stanev, I. Taboada, S. Schlenstedt, C. Wiedemann, Christian Spiering, P. O. Hulth, H. Miyamoto, Dmitry Chirkin, Elisa Resconi, D. Seckel, Jean Gallagher, L. Köpke, Heiko Geenen, A. R. Fazely, H. Leich, H. Wissing, S. Tilav, N. Kitamura, R. Nahnhauer, Elisa Bernardini, J. Ahrens, D. R. Nygren, T. Neunhöffer, C. Walck, T. Messarius, K. Schinarakis, P. Steffen, Albrecht Karle, Thomas K. Gaisser, Jodi Cooley, Xinhua Bai, Jan Conrad, T. Feser, Wolfgang Rhode, T. J. Sumner, T. Castermans, Peter Mészáros, C. De Clercq, W. Chinowsky, D. Bertrand, S. Richter, M. Hellwig, R. W. Ellsworth, H. G. Sander, B. Collin, I. Liubarsky, C. H. Wiebusch, R. Morse, T. Stezelberger, D. Hays, R. Ehrlich, S. Böser, A. J. Smith, K. H. Sulanke, T. Burgess, M. Kestel, T. DeYoung, E. Blaufuss, D. Z. Besson, D. J. Boersma, Glenn Spiczak, B. Hughey, R. Koch, and P. Miocinovic
Subjects: Physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, Astrophysics, Solar neutrino problem, IceCube Neutrino Observatory, law.invention, Telescope, Neutrino detector, Space and Planetary Science, law, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Neutrino astronomy
Abstract: The IceCube neutrino telescope, to be constructed near the Antarctic South Pole, represents the next generation of neutrino telescope. Its large 1 km3 size will make it uniquely sensitive to the detection of neutrinos from astrophysical sources. The current design of the detector is presented. The basic performance of the detector and its ability to search for neutrinos from various astrophysical sources has been studied using detailed simulations and is discussed.
Published: 2004

9. Hardware controls for the STAR experiment at RHIC

Author: J. T.M. Chrin, Z. Sandler, S. Jacobson, M Bordua, E. Yamamoto, J. Lin, J. C. Dunlop, D Reichhold, M. Cherney, J. Gross, V. Ghazikhanian, M. A. Howe, C. Lionberger, S. R. Klein, Y Shi, W. M. Zhang, F. S. Bieser, C. P. McParland, I. Sakrejda, T. S. McShane, J. Schambach, R. Willson, M. I. Ferguson, S. Lewis, J. Meier, G LoCurto, P. Kravtsov, and G. C. Harper
Subjects: Physics, Nuclear and High Energy Physics, business.industry, Detector, Industrial control system, Star (graph theory), Particle detector, Software, Control system, business, Instrumentation, Computer hardware, VMEbus, STAR detector
Abstract: The STAR detector sits in a high radiation area when operating normally; therefore it was necessary to develop a robust system to remotely control all hardware. The STAR hardware controls system monitors and controls approximately 14,000 parameters in the STAR detector. Voltages, currents, temperatures, and other parameters are monitored. Effort has been minimized by the adoption of experiment-wide standards and the use of pre-packaged software tools. The system is based on the Experimental Physics and Industrial Control System (EPICS) [1] . VME processors communicate with subsystem-based sensors over a variety of field busses, with High-level Data Link Control (HDLC) being the most prevalent. Other features of the system include interfaces to accelerator and magnet control systems, a web-based archiver, and C++-based communication between STAR online, run control and hardware controls and their associated databases. The system has been designed for easy expansion as new detector elements are installed in STAR.
Published: 2003

10. Physics and Results from the AMANDA-II High Energy Neutrino Telescope

Author: H. G. Sander, P. Ekström, R. Schwarz, M. Kowalski, P. Lindahl, Staffan Carius, X. Bai, P. O. Hulth, T. Hauschildt, Kyler Kuehn, Allan Hallgren, H. S. Matis, C. Wiedemann, P. B. Price, H. Wissing, P. Miocinovic, C. Walck, Stefan Richter, Thomas K. Gaisser, G. B. Yodh, C. Pérez de los Heros, S. Böser, M. Gaug, M. Hellwig, Dmitry Chirkin, Gerald Przybylski, A. Silvestri, Francis Halzen, S. Hundertmark, Matthias Leuthold, K. Hultqvist, M. Solarz, Kael Hanson, Elisa Bernardini, Kyle T. Mandli, Elisa Resconi, D. R. Nygren, P. Doksus, K. Rawlins, M. Ribordy, Olga Botner, T. Castermans, P. Steffen, Hakki Ögelman, J. Rodríguez Martino, T. Messarius, Jan Conrad, T. Feser, C. De Clercq, R. Nahnhauer, Steven W. Barwick, Jodi Cooley, J. P Dewulf, S. W. Barwick, S. Young, J. Ahrens, Y. Minaeva, L. Gerhardt, Paolo Desiati, R. G. Stokstad, R. Wischnewski, P. Herquet, Karl-Heinz Sulanke, R. Ganupati, H. Leich, Wolfgang Wagner, T. Burgess, D. Bertrand, R. Morse, J. I. Lamoureux, K. Schinarakis, Freddy Binon, A. C. Pohl, Pawel Marciniewski, P. Sudhoff, Glenn Spiczak, Anna Davour, D. F. Cowen, Donald P. Schneider, T. Neunhöffer, Timothy W. Schmidt, K.-H. Becker, J. Madsen, S. Tilav, C. P. McParland, A. Goldschmidt, A. Biron, C. Spiering, Ph. Olbrechts, A. Karle, Othmane Bouhali, C. H. Wiebusch, G. C. Hill, L. Thollander, Heiko Geenen, Tyce DeYoung, R. Hardtke, I. Taboada, T. Becka, Janet Jacobsen, Wolfgang Rhode, K. Woschnagg, D. Ross, P. Niessen, D. Steele, and L. Köpke
Subjects: Physics, Telescope, Neutrino detector, law, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, Measurements of neutrino speed, Astronomy, Neutrino astronomy, Solar neutrino problem, Neutrino, Neutrino oscillation, law.invention
Abstract: This paper briefly describes the principle of operation and science goals of the AMANDA high energy neutrino telescope located at the South Pole, Antarctica. Results from an earlier phase of the telescope, called AMANDA-BIO, demonstrate both reliable operation and the broad astrophysical reach of this device, which includes searches for a variety of sources of ultrahigh energy neutrinos: generic point sources, Gamma-Ray Bursts and diffuse sources. The predicted sensitivity and angular resolution of the telescope were confirmed by studies of atmospheric muon and neutrino backgrounds. We also report on the status of the analysis from AMANDA-II, a larger version with far greater capabilities. At this stage of analysis, details of the ice properties and other systematic uncertainties of the AMANDA-II telescope are under study, but we have made progress toward critical science objectives. In particular, we present the first preliminary flux limits from AMANDA-II on the search for continuous emission from astrophysical point sources, and report on the search for correlated neutrino emission from Gamma Ray Bursts detected by BATSE before decommissioning in May 2000. During the next two years, we expect to exploit the full potential of AMANDA-II with the installation of a new data acquisition system that records full waveforms from the in-ice optical sensors.
Published: 2003

11. Software-Based Challenges of Developing the Future Distribution Grid

Author: C. P. McParland, Emma Stewart, and Sila Kiliccote
Subjects: Computer science, business.industry, Usability, computer.software_genre, Grid, Automation, Visualization, Data modeling, Semantic grid, Software, Distributed generation, Systems engineering, Data mining, business, computer
Abstract: The software that the utility industry currently uses may be insufficient to analyze the distribution grid as it rapidly modernizes to include active resources such as distributed generation, switch and voltage control, automation, and increasingly complex loads. Although planners and operators have traditionally viewed the distribution grid as a passive load, utilities and consultants increasingly need enhanced analysis that incorporates active distribution grid loads in order to ensure grid reliability. Numerous commercial and open-source tools are available for analyzing distribution grid systems. These tools vary in complexity from providing basic load-flow and capacity analysis under steady-state conditions to time-series analysis and even geographical representations of dynamic and transient events. The need for each type of analysis is not well understood in the industry, nor are the reasons that distribution analysis requires different techniques and toolsboth from those now available and from those used for transmission analysis. In addition, there is limited understanding of basic capability of the tools and how they should be practically applied to the evolving distribution system. The study reviews the features and state of the art capability of current tools, including usability and visualization, basic analysis functionality, advanced analysis including inverters, and renewable generation and load modeling. We also discuss the need for each type of distribution grid system analysis. In addition to reviewing basic functionality current models, we discuss dynamics and transient simulation in detail and draw conclusions about existing software?s ability to address the needs of the future distribution grid as well as the barriers to modernization of the distribution grid that are posed by the current state of software and model development. Among our conclusions are that accuracy, data transfer, and data processingabilities are key to future distribution grid modeling, and measured data sources are a key missing element . Modeling tools need to be calibrated based on measured grid data to validate their output in varied conditions such as high renewables penetration and rapidly changing topology. In addition, establishing a standardized data modeling format would enable users to transfer data among tools to take advantage of different analysis features. ?
Published: 2014

12. Elliptic Flow inAu+AuCollisions at√sNN=130GeV

Author: N. Stone, Christophe Pierre Suire, A. Lebedev, B. Miller, M. M. de Moura, M. Dialinas, P. Middlekamp, J. Scheblien, V. Ghazikhanian, A. Etkin, A. H. Tang, A. P. Meschanin, R.Kh. Kutuev, J. Berger, J. L. Romero, V. Fine, J. Engelage, T. J. Humanic, Peter J. Lindstrom, D. Zimmerman, I.A. Savin, N. T. Porile, Yu A. Matulenko, M. Horsley, Thomas LeCompte, B. Stringfellow, J. Sedlmeir, L. Smykov, E. Finch, T. S. McShane, J. W. Harris, Joakim Nystrand, V. B. Dunin, J. Grabski, P. Seyboth, D. Dayton, C. J. Liaw, R. Bossingham, J. N. Marx, C. Drancourt, S. Tonse, W. S. Deng, J. G. Cramer, R. A. Scheetz, A. Stolpovsky, H. Hümmler, L. Kotchenda, G. Koehler, E. Gushin, G. J. Kunde, P. Yepes, V. Eckardt, M. Kramer, A. I. Pavlinov, Y. Panebratsev, D. Grosnick, Granville Ott, G. Eppley, A. V. Brandin, V. Trofimov, J. M. Landgraf, M. Strikhanov, K. Krueger, M. B. Tonjes, E. I. Shakaliev, A. Yokosawa, Jinghui Yang, E. Sugarbaker, J. Hunter, H. Z. Huang, V. Morozov, A. Tarchini, S. V. Razin, K. Wilson, G. Rai, Y. Shi, G. Van Buren, J. M. Nelson, P. A. DeYoung, J. Pluta, C. Roy, H. Stroebele, J. Carroll, C. Byrd, N. Xu, G. D. Westfall, D. Padrazo, R. Wells, C. Struck, W. Pinganaud, D. Hardtke, F. Laue, J.F. Amsbaugh, Jay Roberts, N. Adams, David Fritz, J. Sandweiss, G. LoCurto, A. C. Saulys, S. R. Klein, C. E. Allgower, R. D. Majka, J. Zhu, Sergey Voloshin, J. Sowinski, Matthew Nguyen, W. Peryt, J. Takahashi, J. Wolf, C. Feliciano, Y. Fisyak, L. Greiner, K. J. Foley, J. Schambach, E. L. Hjort, S. Pirogov, A. Ogawa, Ian Johnson, Krista M. Marks, S. E. Vigdor, Vladimir Petrov, C. L. Kunz, Z. Li, O. Barannikova, D. L. Olson, F. P. Brady, Gerald W Hoffmann, S. P. Chernenko, D. Seliverstov, A. Schüttauf, Christian Claude Kuhn, W. J. Llope, Q. Li, C. O. Blyth, C. F. Moore, M. Cherney, H. Fessler, W. Christie, Thomas Michael Cormier, D.E. Greiner, T. Krupien, Torre Wenaus, Masashi Kaneta, Ross Schlueter, W. M. Zhang, Andrey Vasiliev, D. Hill, Richard C. Jared, M. Calderón de la Barca Sánchez, R. Weidenbach, T. Nguyen, A. Cardenas, Peter Martin Jacobs, N. Schmitz, S. Chatopadhyay, P. Nevski, M. Lopez-Noriega, A. Klyachko, R. Witt, E. Yamamoto, J. Klay, Thomas A. Trainor, W. R. Edwards, P. Sappenfield, N.D. Gagunashvili, J. Baudot, E. A. Matyushevski, P. Kuczewski, J. C. Dunlop, A. A. Derevschikov, K. Olchanski, V. I. Danilov, C. P. Lansdell, Wilfred J. Braithwaite, E. Mogavero, R.J.M. Snellings, Janet Elizabeth Seger, J. Lin, M. A. C. Lamont, S. B. Nurushev, Z. Milosevich, B. Lasiuk, J. Wisdom, Y. V. Zanevski, F. Retiere, W. Hunt, V. Kormilitsyne, D. Russ, B. E. Bonner, J. T.M. Chrin, G. S. Mutchler, H. Diaz, J. R. Hall, Zubayer Ahammed, G. A. Ososkov, M. J. LeVine, B. Norman, J. Gross, H. Long, K. Bradley, Yu Chen, Wen-Chang Chen, N. G. Minaev, O. D. Tsai, R. P. Scharenberg, Marie Germain, R. Seymour, M. A. Howe, B. Choi, R. Marstaller, W. Betts, Vladimir Tikhomirov, Salahuddin Ahmad, I. Polk, H. S. Matis, G. C. Harper, A. S. Hirsch, P. Kravtsov, A. Maliszewski, Alexander Kovalenko, L. V. Nogach, L. C. Bland, S. Bennett, H. J. Crawford, I. Vakula, C. Adler, F. S. Bieser, L. Wood, A. N. Zubarev, C. A. Ogilvie, G. Brugalette, V. S. Shvetcov, L. S. Schroeder, J. Meier, H. Liu, S. U. Pandey, A. E. Yakutin, I. Flores, Morton Kaplan, V. Perevotchikov, C. A. Whitten, M. Pentia, Marek Gazdzicki, L. Lakehal-Ayat, D. Lopiano, S. Trentalange, A. Ridiger, W. W. Jacobs, M. I. Ferguson, J. Lamas-Valverde, C. Gojak, M. Botlo, Guy Paic, I. Sakrejda, T. Ngo, E. Platner, B. Minor, V. Lindenstruth, V. A. Nikitin, S. Heppelmann, D. Flierl, Ma Bloomer, John Z. H. Zhang, A. Chikanian, S. S. Shimanskii, J. Mitchell, E. G. Judd, L. Martin, Jeffrey G. Reid, B. K. Srivastava, I. M. Vasilevski, K. E. Shestermanov, V. V. Belaga, Lincoln D. Carr, J. Gans, S. Lange, L. Arnold, Boris Hippolyte, G. Skoro, M. Heffner, J. E. Draper, J. Puskar-Pasewicz, R. Morse, V. Grigoriev, J. P. Coffin, O. V. Rogachevski, N. Bouillo, M. DeMello, S. J. Lindenbaum, N. Mikhalin, A. Boucham, H. Ward, M. Oldenburg, Peter Graham Jones, R. L. Ray, V. Emelianov, D. Keane, A. R. Baldwin, A. A. P. Suaide, L. Didenko, Damien Bonnet, Nikolai Smirnov, R. Stock, S. Y. Panitkin, E. Potrebenikova, W. J. Leonhardt, S. Bekele, S. Bouvier, V. P. Kenney, L. G. Efimov, Frank Jm Geurts, Yu. Ivanshin, J. Castillo, S. W. Wissink, R. L. Brown, W. Dominik, P. Jensen, A. Ishihara, T. Ljubicic, Alexander Khodinov, Robert Stone, M. Tokarev, G. Guilloux, Robert R. J. Maier, D. DiMassimo, E. Anderssen, A. M. VanderMolen, H. H. Wieman, H. Caines, S. Jacobson, D. Shuman, R. Willson, D. G. Underwood, J. Wirth, D. Reichhold, T. J. Hallman, T. J. M. Symons, K. Turner, A. Szanto de Toledo, A. M. Poskanzer, J. Tarzian, P. He, K. Solberg, T. Pawlak, A. Vanyashin, Z. Sandler, B. Caylor, R. S. Longacre, V. L. Rykov, J. Porter, G. Igo, J. Seyboth, P. Fachini, D. D. Weerasundara, Mingshui Chen, M. Grau, S. Margetis, O. A. Grachov, M. Schulz, J. R. Lutz, Rainer Arno Ernst Renfordt, J. Balewski, H. G. Ritter, Claude Andre Pruneau, H. Arnesen, R. Zoulkarneev, R. Bellwied, A. S. Konstantinov, K. H. Ackermann, D. M. Moltz, A. A. Kuznetsov, Ivan Kotov, T. Noggle, V. M. Leontiev, Olivier Ravel, J. Whitfield, T. Ullrich, D. Roehrich, B. Erazmus, Z. Z. Xu, D. Cebra, C. Consiglio, M. Beddo, Yu Melnick, P. Leszczynski, J. Bercovitz, T. Herston, J. Riso, Lee Stuart Barnby, V. A. Moiseenko, Marcelo Gameiro Munhoz, D. J. Prindle, E. J. Stephenson, M. A. Lisa, W. A. Love, T. Nussbaum, Daniel Ferenc, Fuqiang Wang, H. Bichsel, G. Odyniec, V. I. Yurevich, E. S. Braithwaite, J. Boehm, T. Eggert, David Lynn, L. Madansky, R. Sanchez, J. Dioguardi, J. H. Thomas, L. Conin, G. Visser, G. S. Averichev, C. P. McParland, H. M. Spinka, J. Rasson, Chinh Vu, and Matthew J. Anderson
Subjects: Physics, Particle physics, Time projection chamber, Hadron, Elliptic flow, General Physics and Astronomy, Observable, Particle accelerator, Charged particle, law.invention, Nuclear physics, law, Pseudorapidity, Nuclear Experiment, Relativistic Heavy Ion Collider
Abstract: Elliptic flow from nuclear collisions is a hadronic observable sensitive to the early stages of system evolution. We report first results on elliptic flow of charged particles at midrapidity in Au+Au collisions at √(sNN) = 130 GeV using the STAR Time Projection Chamber at the Relativistic Heavy Ion Collider. The elliptic flow signal, v₂, averaged over transverse momentum, reaches values of about 6% for relatively peripheral collisions and decreases for the more central collisions. This can be interpreted as the observation of a higher degree of thermalization than at lower collision energies. Pseudorapidity and transverse momentum dependence of elliptic flow are also presented.
Published: 2001

13. Λ hyperons in 2 A GeV Ni + Cu collisions

Author: J. A. Hauger, H. G. Ritter, S. Wang, Salvatore Costa, C. P. McParland, G. Rai, Renato Potenza, Antonio Insolia, J. C. Kintner, D. L. Olson, J. L. Romero, J. O. Rasmussen, B. K. Srivastava, Y. Shao, M. L. Gilkes, Sebastiano Albergo, J. L. Chance, M. A. McMahan, Z. Caccia, D. Cebra, R. P. Scharenberg, M. L. Tincknell, H. S. Matis, E. Hjort, H. Liu, J. Romanski, A. Scott, P. Warren, N. T. Porile, Y. Choi, M. A. Lisa, M. Justice, F. P. Brady, A. S. Hirsch, T. Wienold, R. L. McGrath, A. D. Chacon, D. Keane, D. Weerasundara, James B. Elliott, Cristina Tuve, M. D. Partlan, G.V. Russo, F. S. Bieser, K.L. Wolf, H. H. Wieman, and T. J. M. Symons
Subjects: Physics, Nuclear and High Energy Physics, Time projection chamber, 010308 nuclear & particles physics, Hyperon, Lambda, 01 natural sciences, Nuclear physics, Transverse plane, 0103 physical sciences, Transverse mass, Invariant mass, Multiplicity (chemistry), Impact parameter, Nuclear Experiment, 010306 general physics
Abstract: A sample of Lambda's produced in 2 A*GeV Ni + Cu collisions has been obtained with the EOS Time Projection Chamber at the Bevalac. Low background in the invariant mass distribution allows for the unambiguous demonstration of Lambda directed flow. The transverse mass spectrum at mid-rapidity has the characteristic shoulder-arm shape of particles undergoing radial transverse expansion. A linear dependence of Lambda multiplicity on impact parameter is observed, from which a total Lambda + Sigma^0 production cross section of $112 +/- 24 mb is deduced. Detailed comparisons with the ARC and RVUU models are made.
Published: 1998

14. Dynamics of radial collective energy in near central collisions for1AGeVAu+C

Author: A. Scott, H. Sann, P. Danielewicz, M. A. McMahan, N. N. Ajitanand, T. Wienold, S. Wang, J. A. Hauger, J. B. Elliott, T. J. M. Symons, J. Romanski, F. P. Brady, R. Potenza, D. Keane, P. Chung, A. D. Chacon, H. H. Wieman, M. L. Gilkes, S. Albergo, M. Justice, P. Warren, V. Lindenstruth, J. L. Chance, S. Costa, H. G. Ritter, M. L. Tincknell, A. S. Hirsch, D. Cebra, N. T. Porile, R. L. McGrath, G. V. Russo, E. L. Hjort, G. Rai, J. O. Rasmussen, Roy A. Lacey, C. P. McParland, M. D. Partlan, Z. Caccia, D. L. Olson, A. Insolia, R. P. Scharenberg, H. S. Matis, M. A. Lisa, Y. Choi, J. Lauret, John M. Alexander, B. K. Srivastava, J. L. Romero, Y. Shao, C. Tuve, Wolfgang Müller, F. S. Bieser, K.L. Wolf, and J. C. Kintner
Subjects: Physics, Nuclear and High Energy Physics, Range (particle radiation), Transverse plane, Thermal, Quasiparticle, Coulomb, Atomic physics, Nuclear Experiment, Kinetic energy, Excitation, Energy (signal processing)
Abstract: Transverse kinetic energies of individual fragments have been measured over a broad range of emitter excitation energies for the reaction 1AGeV Au+C. For excitation energies leading to large intermediate mass fragment multiplicities, these transverse energies require large collective radial expansion of the emitting systems. However, the traditional decomposition of the transverse energy into a thermal component and a Coulomb and collective component proportional to the fragment mass cannot account for this expansion. Expansion velocities show an increase with decreasing fragment Z and thus indicate fractionation of the collective energy for the expanding system. This collective energy increases with emitter excitation up to about 50{percent} of the energy deposited for a nuclear system with total energy {approximately}12AMeV. The bulk of the collective energy is carried away by ejectiles of Z{le}3. {copyright} {ital 1998} {ital The American Physical Society}
Published: 1998

15. Multifragmentation of the remnant produced in the reaction of1AGeV gold with carbon

Author: M. A. McMahan, Cristina Tuve, J. O. Rasmussen, M. D. Partlan, C. P. McParland, F. P. Brady, Y. Shao, R. P. Scharenberg, and K. Wolf, S. Wang, H. S. Matis, V. Lindenstruth, M. A. Lisa, J. C. Kintner, A. Scott, J. L. Chance, H. Sann, Y. Choi, D. Cebra, H. G. Ritter, F. S. Bieser, P. Warren, Renato Potenza, J. B. Elliott, D. Keane, B. K. Srivastava, Sebastiano Albergo, E. L. Hjort, J. L. Romero, H. H. Wieman, G. Rai, T. J. M. Symons, M. L. Gilkes, Z. Caccia, T. Wienold, J. A. Hauger, D. L. Olson, J. Romanski, Wolfgang Müller, M. L. Tincknell, N. T. Porile, Salvatore Costa, Andrew S. Hirsch, A. Insolia, A. D. Chacon, G.V. Russo, and M. Justice
Subjects: Physics, Nuclear and High Energy Physics, Isotope, Atomic number, Multiplicity (chemistry), Atomic physics, Nuclear Experiment, Nuclear matter, Nucleon, Excitation, Charged particle, Effective nuclear charge
Abstract: A high-statistics exclusive study of the multifragmentation of 1A GeV gold on carbon has been performed. Particles with Z{le}2 show evidence of emission in a first prompt stage as well as in a second equilibrium stage whereas fragments with Z{ge}3 appear to be emitted essentially only in the second stage. Two methods for the separation of the Z{le}2 particles into the two stages are given and they are in agreement. The yields for each stage are determined as a function of the event charged particle multiplicity m. The mass, nuclear charge, excitation energy per nucleon, and temperature of the remnant left after the first stage and their fluctuations have been determined as a function of m. The expansion of the remnant to fragment freeze-out is examined. The freeze-out temperature is determined from double isotope ratios as a function of m and isentropic trajectories are obtained in the temperature-density plane. The caloric curve shows a monotonic increase with excitation energy. Some of the energy is in the form of radial flow. Overall, the results are consistent with a previous statistical analysis of the data which suggests that, over a certain range of excitation energies, multifragmentation involves a continuous phase transition. {copyright}more » {ital 1998} {ital The American Physical Society}« less
Published: 1998

16. Calibration and survey of AMANDA with the SPASE detectors

Author: J. Ahrens, X. Bai, S. W. Barwick, R. C. Bay, T. Becka, K. H. Becker, E. Bernardini, D. Bertrand, F. Binon, A. Biron, S. Boser, O. Botner, A. Bouchta, O. Bouhali, T. Burgess, S. Carius, T. Castermans, D. C.h.i.r.k.i.n.J. Conrad, J. Cooley, D. F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, J. P. Dewulf, E. Dickinson, P. Doksus, P. Ekstrom, R. Engel, P. Evenson, T. Feser, T. K. Gaisser, R. Ganugapati, M. Gaug, H. Geenen, L. Gerhardt, A. Goldschmidt, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, P. Herquet, G. C. Hill, J. A. Hinton, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, A. Karle, J. Kim, L. Kopke, M. Kowalski, K. Kuehn, J. I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, J. Lloyd Evans, J. Madsen, K. Mandli, P. Marciniewski, H. S. Matis, C. P. McParland, T. Messarius, T. C. Miller, Y. Minaeva, P. MioWinovic, P. C. Mock, R. Morse, T. Neunhoffer, P. Niessen, D. R. Nygren, H. O. gelman, P.h. Olbrechts, C. Perez de los Heros, A. C. Pohl, R. Porrata, P. B. Price, G. T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, K. Rochester, J. Rodrıguez Martino, P. Romenesko, D. Ross, H. G. Sander, T. Schmidt, K. Schinarakis, S. Schlenstedt, D. Schneider, R. Schwarz, A. Silvestri, M. Solarz, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, D. Steele, P. Steffen, R. G. Stokstad, K. H. Sulanke, I. Taboada, S. Tilav, C. Walck, W. Wagner, Y. R. Wang, A. A. Watson, C. Weinheimer, C. H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, W. Wu, G. Yodh, S. Young, MARTELLO, Daniele, J., Ahren, X., Bai, S. W., Barwick, R. C., Bay, T., Becka, K. H., Becker, E., Bernardini, D., Bertrand, F., Binon, A., Biron, S., Boser, O., Botner, A., Bouchta, O., Bouhali, T., Burge, S., Cariu, T., Casterman, Conrad, D. C. h. i. r. k. i. n. J., J., Cooley, D. F., Cowen, A., Davour, C., De Clercq, T., Deyoung, P., Desiati, J. P., Dewulf, E., Dickinson, P., Doksu, P., Ekstrom, R., Engel, P., Evenson, T., Feser, T. K., Gaisser, R., Ganugapati, M., Gaug, H., Geenen, L., Gerhardt, A., Goldschmidt, A., Hallgren, F., Halzen, K., Hanson, R., Hardtke, T., Hauschildt, M., Hellwig, P., Herquet, G. C., Hill, J. A., Hinton, B., Hughey, P. O., Hulth, K., Hultqvist, S., Hundertmark, J., Jacobsen, A., Karle, J., Kim, L., Kopke, M., Kowalski, K., Kuehn, J. I., Lamoureux, H., Leich, M., Leuthold, P., Lindahl, I., Liubarsky, J., Lloyd Evan, J., Madsen, K., Mandli, P., Marciniewski, Martello, Daniele, H. S., Mati, C. P., Mcparland, T., Messariu, T. C., Miller, Y., Minaeva, P., Miowinovic, P. C., Mock, R., Morse, T., Neunhoffer, P., Niessen, D. R., Nygren, H. O., Gelman, Olbrechts, P. h., C., Perez de los Hero, A. C., Pohl, R., Porrata, P. B., Price, G. T., Przybylski, K., Rawlin, E., Resconi, W., Rhode, M., Ribordy, S., Richter, K., Rochester, J., Rodrıguez Martino, P., Romenesko, D., Ro, H. G., Sander, T., Schmidt, K., Schinaraki, S., Schlenstedt, D., Schneider, R., Schwarz, A., Silvestri, M., Solarz, G. M., Spiczak, C., Spiering, M., Stamatiko, T., Stanev, D., Steele, P., Steffen, R. G., Stokstad, K. H., Sulanke, I., Taboada, S., Tilav, C., Walck, W., Wagner, Y. R., Wang, A. A., Watson, C., Weinheimer, C. H., Wiebusch, C., Wiedemann, R., Wischnewski, H., Wissing, K., Woschnagg, W., Wu, G., Yodh, and S., Young
Subjects: Neutrino telescopes, Cosmic ray
Abstract: We report on the analysis of air showers observed in coincidence by the Antarctic Muon and Neutrino detector array (AMANDA-B10) and the South Pole Air Shower Experiment (SPASE-1 and SPASE-2). We discuss the use of coincident events for calibration and survey of the deep AMANDA detector as well as the response of AMANDA to muon bundles. This analysis uses data taken during 1997 when both SPASE-1 and SPASE-2 were in operation to provide a stereo view of AMANDA.
Published: 2004

17. ΔResonance Production inN58i+CuCollisions atE=1.97AGeV

Author: J. O. Rasmussen, A. S. Hirsch, Alwyn C. Scott, Sebastiano Albergo, T. J. M. Symons, Y. Shao, M. L. Gilkes, Y. Choi, G.V. Russo, M. A. McMahan, J. L. Romero, G. Rai, M. L. Tincknell, N. T. Porile, M. Justice, P. Warren, F. S. Bieser, K.L. Wolf, S. Wang, E. L. Hjort, Z. Caccia, M. D. Partlan, H. H. Wieman, R. P. Scharenberg, H. S. Matis, D. Keane, J. L. Chance, D. L. Olson, D. Cebra, Renato Potenza, T. Wienold, J. B. Elliott, J. C. Kintner, A. D. Chacon, Salvatore Costa, A. Insolia, C. P. McParland, J. Romanski, M. A. Lisa, B. K. Srivastava, F. P. Brady, Cristina Tuve, H. G. Ritter, and J. A. Hauger
Subjects: Baryon, Nuclear physics, Physics, Nuclear reaction, Hadron, General Physics and Astronomy, Resonance, Production (computer science), Elementary particle, Invariant mass, Atomic physics, Nuclear Experiment, Delta baryon
Abstract: Invariant mass analyses of (p,{pi}{sup {plus_minus}}) pairs in {sup 58}Ni+Cu collisions at 1.97A GeV have been performed and show correlations resulting from the decays of the {Delta} resonance, the {Lambda} baryon, and possibly the N{sup {asterisk}}(1440) resonance. A reduction in the {Delta} mass is observed and the mass reduction increases with collision centrality. Events generated by the relativistic cascade model (ARC) also reveal a mass reduction. The mass reduction is related to the size of the reaction volume and the details of {Delta} production mechanisms in heavy ion collisions. {copyright} {ital 1997} {ital The American Physical Society}
Published: 1997

18. Pion Flow and Antiflow in1.15AGeVAu+Au

Author: G. Rai, D. Keane, A. Scott, F. S. Bieser, M. L. Tincknell, K.L. Wolf, Y. Shao, N. T. Porile, H. H. Wieman, G.V. Russo, Renato Potenza, M. L. Gilkes, J. B. Elliott, T. J. M. Symons, J. O. Rasmussen, J. C. Kintner, J. L. Romero, A. D. Chacon, Salvatore Costa, B. K. Srivastava, A. Insolia, T. Wienold, M. A. McMahan, Sebastiano Albergo, Cristina Tuve, H. G. Ritter, Andrew S. Hirsch, R. P. Scharenberg, P. Warren, F. P. Brady, H. S. Matis, E. L. Hjort, D. L. Olson, J. A. Hauger, Y. Choi, M. D. Partlan, S. Wang, Z. Caccia, M. Justice, J. Romanski, M. A. Lisa, J. L. Chance, D. Cebra, and C. P. McParland
Subjects: Nuclear physics, Physics, Particle physics, Pion, Flow (mathematics), TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY, General Physics and Astronomy, Impact parameter
Abstract: Transverse flow has been studied as a function of impact parameter for pions and protons from the reaction 1.15A GeV {sup 197}Au+{sup 197}Au. We observe an {open_quotes}antiflow{close_quotes} behavior for both {pi}{sup +} and {pi}{sup -} in peripheral collisions. {copyright} {ital 1997} {ital The American Physical Society}
Published: 1997

19. The Energy Dependence of Flow in Ni Induced Collisions from400Ato1970AMeV

Author: M. Justice, R. P. Scharenberg, H. S. Matis, T. J. M. Symons, M. L. Gilkes, B. K. Srivastava, Y. Choi, Sebastiano Albergo, F. S. Bieser, S. Wang, K.L. Wolf, Andrew S. Hirsch, T. Wienold, Renato Potenza, D. Keane, J. B. Elliott, Antonio Insolia, C. P. McParland, J. L. Romero, H. H. Wieman, Salvatore Costa, J. C. Kintner, F. P. Brady, M. A. Lisa, A. Scott, M. A. McMahan, J. L. Chance, D. Cebra, P. Warren, E. L. Hjort, G. Rai, J. Romanski, Cristina Tuve, M. L. Tincknell, N. T. Porile, Z. Caccia, M. D. Partlan, A. D. Chacon, G.V. Russo, Y. Shao, J. O. Rasmussen, D. L. Olson, H. G. Ritter, and J. A. Hauger
Subjects: Physics, 010308 nuclear & particles physics, Computer Science::Information Retrieval, General Physics and Astronomy, chemistry.chemical_element, Nuclear matter, 01 natural sciences, 7. Clean energy, Copper, Nuclear physics, Nickel, chemistry, Flow (mathematics), 0103 physical sciences, Atomic physics, Nuclear Experiment, 010306 general physics, Scaling, Energy (signal processing)
Abstract: We study the energy dependence of collective (hydrodynamic-like) nuclear matter flow in (400{endash}1970){ital A} MeV Ni+Au and (1000{endash}1970){ital A} MeV Ni+Cu reactions. The flow increases with energy, appears to reach a maximum, and then to decrease at higher energies. A way of comparing the energy dependence of flow values for different projectile-target mass combinations is introduced, which demonstrates a more-or-less common scaling behavior among flow values from different systems. {copyright} {ital 1997} {ital The American Physical Society}
Published: 1997

20. In-Plane Retardation of Collective Expansion inAu+AuCollisions

Author: F. P. Brady, M. A. McMahan, H. G. Ritter, J. L. Romero, V. Lindenstruth, R. P. Scharenberg, J. L. Chance, F. S. Bieser, H. S. Matis, K.L. Wolf, D. Cebra, A. Scott, Antonio Insolia, D. L. Olson, Y. Choi, M. L. Tincknell, J. Romanski, D. Keane, D. Weerasundara, A. D. Chacon, N. T. Porile, S. Wang, Cristina Tuve, M. A. Lisa, Sebastiano Albergo, G.V. Russo, H. H. Wieman, Andrew S. Hirsch, H. Liu, G. Rai, Renato Potenza, M. L. Gilkes, J. B. Elliott, J. O. Rasmussen, Z. Caccia, C. P. McParland, J. C. Kintner, P. Warren, Salvatore Costa, M. D. Partlan, E. L. Hjort, J. A. Hauger, Y. Shao, B. K. Srivastava, M. Justice, and T. J. M. Symons
Subjects: Physics, In plane, Classical mechanics, General Physics and Astronomy
Published: 1996

21. Radial Flow inAu+AuCollisions atE=(0.25−1.15)AGeV

Author: J. Romanski, M. A. Lisa, M. A. McMahan, Z. Caccia, Y. Shao, M. Justice, A. Scott, D. Keane, Cristina Tuve, F. S. Bieser, R. P. Scharenberg, H. S. Matis, H. H. Wieman, K.L. Wolf, J. L. Chance, D. Cebra, Antonio Insolia, F. P. Brady, B. K. Srivastava, Gary Westfall, Y. Choi, D. L. Olson, M. D. Partlan, G. V. Russo, S. Wang, J. O. Rasmussen, T. J. M. Symons, A. D. Chacon, J. A. Hauger, P. Warren, C. P. McParland, Renato Potenza, Sebastiano Albergo, G. Rai, J. B. Elliott, E. L. Hjort, J. L. Romero, H. G. Ritter, Andrew S. Hirsch, M. L. Gilkes, Salvatore Costa, M. L. Tincknell, N. T. Porile, and J. C. Kintner
Subjects: Physics, 010308 nuclear & particles physics, media_common.quotation_subject, General Physics and Astronomy, 16. Peace & justice, 01 natural sciences, Radial velocity, Quantum mechanics, 0103 physical sciences, Justice (virtue), Radial flow, 010306 general physics, media_common, Mathematical physics
Abstract: Author(s): Lisa, M.A.; Albergo, S.; Bieser, F.; Brady, F.P.; Caccia, Z.; Cebra, D.A.; Chacon, A.D.; Chance, J.L.; Choi, Y.; Costa, S.; Elliott, J.B.; Gilkes, M.L.; Huager, J.A.; Hirsch, A.S.; Hjort, E.L.; Insolia, A.; Justice, M.; Keane, D.; Kintner, J.; Matis, H.S.; McMahan, M.; McParland, C.; Olson, D.L.; Partlan, M.D.; Porile, N.T.; Potenza, R.; Rai, G.; Rasmussen, J.O.; Ritter, Hans G.; Romanski, J.; Romero, J.L.; Russo, G.V.; Scharenberg, R.P.; Scott, A.; Shao, Y.; Srivastava, B.K.; Symons, T.J.M.; Tincknell, M.L.; Tuve, C.; Wang, S.; Warren, P.; Westfall, G.D.; Wieman, H.H.; Wolf, K.
Published: 1995

22. OpenADR open source toolkit: Developing open source software for the Smart Grid

Author: C. P. McParland
Subjects: Demand response, World Wide Web, Load management, Open source, Smart grid, Software, Computer science, business.industry, Server, The Internet, business, Software engineering, Protocol (object-oriented programming)
Abstract: Demand response (DR) is becoming an increasingly important part of power grid planning and operation. The advent of the Smart Grid, which mandates its use, further motivates selection and development of suitable software protocols to enable DR functionality. The OpenADR protocol has been developed and is being standardized to serve this goal. We believe that the development of a distributable, open source implementation of OpenADR will benefit this effort and motivate critical evaluation of its capabilities, by the wider community, for providing wide-scale DR services.
Published: 2011

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

Author: C. Pérez de los Heros, B. D. Fox, T. Krings, Jenni Adams, J.-P. Hülß, E. Blaufuss, N. van Eijndhoven, D. Bertrand, J. Tooker, M. Wallraff, M. Gurtner, H. S. Matis, R. Gozzini, J. W. Nam, Hermann Kolanoski, P. O. Hulth, J. Eisch, A. Tepe, C. Roucelle, G. de Vries-Uiterweerd, Thomas Meures, M. Schunck, G. Wikström, T. Griesel, M. C. Stoufer, S. Schlenstedt, D. Turcan, N. Milke, Francis Halzen, George Japaridze, D. R. Nygren, S. Odrowski, R. Ehrlich, S. M. Movit, Laura C. Bradley, M. Merck, K. Wiebe, J. L. Kelley, Markus Ahlers, S. Hickford, R. G. Stokstad, G. Kroll, B. Semburg, C. Terranova, H. Wissing, A. Olivas, P. Roth, O. Fadiran, M. R. Duvoort, R. Lehmann, R. Wischnewski, S. Grullon, M. J. Carson, D. Rutledge, S. Panknin, R. Porrata, K. Rawlins, P. Berghaus, O. Depaepe, S. Stoyanov, Ph. Herquet, O. Engdegård, K. Kuehn, Carsten Rott, T. Straszheim, Samvel Ter-Antonyan, Christopher Wiebusch, Q. Swillens, Fabian Kislat, Karen Andeen, A. Slipak, S. Tilav, M. Bissok, J. M. Clem, S. Euler, D. Z. Besson, K. Beattie, Jon Dumm, J. van Santen, M. Prikockis, T. Waldenmaier, Joanna Kiryluk, Timo Karg, Kael Hanson, M. Danninger, O. Schulz, Y. Hasegawa, Xianwu Xu, T. Abu-Zayyad, S. Seunarine, L. Demirörs, T. Kowarik, A. Homeier, J. Lünemann, Elisa Resconi, Dirk Lennarz, E. Middell, H. Landsman, R. W. Ellsworth, Elisa Bernardini, R. Nahnhauer, A. Tamburro, C. Bohm, K. Mase, B. Voigt, P. Nießen, Johan Lundberg, Pratik Majumdar, K.-H. Becker, J. Berdermann, Rasha Abbasi, M. Ribordy, Xinhua Bai, Teresa Montaruli, J. Dreyer, Nathan Whitehorn, S. Cohen, R. C. Bay, Y. Abdou, B. Ruzybayev, Damian Pieloth, R. L. Imlay, Peter Mészáros, J. Petrovic, M. V. D'Agostino, D. Hubert, A. Schukraft, K. Laihem, R. M. Gunasingha, Juan Carlos Diaz-Velez, W. Huelsnitz, Subir Sarkar, Paolo Desiati, David A. Schneider, R. Ganugapati, A. C. Pohl, C. Ha, J. J. Beatty, T. Castermans, D. Berley, G. C. Hill, M. L. Benabderrahmane, Dirk Ryckbosch, M. Olivo, J. A. Goodman, Michael J. Baker, D. F. Cowen, Larissa Paul, K. Helbing, D. Breder, D. J. Boersma, L. Gladstone, C. T. Day, K. Hoshina, D. Seckel, P. B. Price, R. J. Lauer, L. Köpke, A. R. Fazely, Tyce DeYoung, P. A. Toale, A. Silvestri, M. Stamatikos, M. Krasberg, Glenn Spiczak, E. A. Strahler, G. Stephens, S. Westerhoff, C. De Clercq, I. Taboada, David A. Williams, Albrecht Karle, S.J. Lafebre, Paraic A. Kenny, Juanan Aguilar, Spencer Klein, T. O. B. Schmidt, C. P. McParland, Reina H. Maruyama, Jens Madsen, S. W. Barwick, A. Wiedemann, O. Tarasova, K. Meagher, J. Auffenberg, M. Kowalski, Todor Stanev, Takao Kuwabara, C. Wendt, A. Goldschmidt, Kara Hoffman, Y. Sestayo, J. K. Becker, W. R. Edwards, F. Descamps, H. Miyamoto, S. Hussain, Kurt Woschnagg, D. J. Koskinen, Paul Evenson, R. Franke, C. Walck, A. Lucke, M. M. Foerster, Christian Spiering, B. Christy, Thomas K. Gaisser, G. B. Yodh, Wolfgang Rhode, J. C. Gallagher, J. M. Joseph, Allan Hallgren, J. P. Rodrigues, T. Stezelberger, S. Bechet, S. Yoshida, A. Ishihara, J. Bolmont, R. Morse, P. Redl, Dmitry Chirkin, Chad Finley, S. Knops, Alexander Kappes, Karl-Heinz Kampert, Kirill Filimonov, Justin Vandenbroucke, F. Rothmaier, K. Hultqvist, Darren Grant, H. G. Sander, Chun Xu, Karl-Heinz Sulanke, G. W. Sullivan, N. Kemming, James E. Braun, D. Tosi, Gerald Przybylski, M. Inaba, M. Labare, Henrik J. Johansson, Axel Groß, M. Walter, A. Rizzo, Anna Franckowiak, S. H. Seo, N. Potthoff, K. Schatto, G. Kohnen, M. Ono, J. L. Bazo Alba, K. Han, T. Feusels, Olga Botner, J. E. Jacobsen, L. Gerhardt, A. Piegsa, S. J. Patton, A. Van Overloop, Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Nuclear and High Energy Physics, Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Physics::Instrumentation and Detectors, Solar neutrino, Dark matter, FOS: Physical sciences, Astrophysics, 01 natural sciences, 7. Clean energy, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 0103 physical sciences, ddc:530, 010306 general physics, Cosmic rays, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Annihilation, Muon, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Massless particle, Neutrino detector, High Energy Physics::Experiment, Other gauge bosons, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, Lepton
Abstract: A search for muon neutrinos from Kaluza-Klein dark matter annihilations in the Sun has been performed with the 22-string configuration of the IceCube neutrino detector using data collected in 104.3 days of live-time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured lightest Kaluza-Klein particle (LKP) WIMPs in the Sun and converted to limits on the LKP-proton cross-sections for LKP masses in the range 250 -- 3000 GeV. These results are the most stringent limits to date on LKP annihilation in the Sun., 6 pages, 5 figures
Published: 2010

24. Home Network Technologies and Automating Demand Response

Author: C. P. McParland
Subjects: ComputingMilieux_THECOMPUTINGPROFESSION, ComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATION, business.industry, Distribution (economics), Energy consumption, Environmental economics, Automation, GeneralLiterature_MISCELLANEOUS, Demand response, Production (economics), The Internet, Electricity, business, National laboratory
Abstract: Home Network Technologies and Automating Demand Response Charles McParland, Lawrence Berkeley National Laboratory December 2008
Published: 2009

25. Open Automated Demand Response Communications Specification (Version 1.0)

Author: Ed Koch, C. P. McParland, Girish Ghatikar, Mary Ann Piette, Sila Kiliccote, Peter Palensky, and Dan Hennage
Subjects: Demand response, Smart grid, Computer science, business.industry, Open standard, Event (computing), Interoperability, Industrial control system, Software engineering, business, Automation, Information exchange
Abstract: The development of the Open Automated Demand Response Communications Specification, also known as OpenADR or Open Auto-DR, began in 2002 following the California electricity crisis. The work has been carried out by the Demand Response Research Center (DRRC), which is managed by Lawrence Berkeley National Laboratory. This specification describes an open standards-based communications data model designed to facilitate sending and receiving demand response price and reliability signals from a utility or Independent System Operator to electric customers. OpenADR is one element of the Smart Grid information and communications technologies that are being developed to improve optimization between electric supply and demand. The intention of the open automated demand response communications data model is to provide interoperable signals to building and industrial control systems that are preprogrammed to take action based on a demand response signal, enabling a demand response event to be fully automated, with no manual intervention. The OpenADR specification is a flexible infrastructure to facilitate common information exchange between the utility or Independent System Operator and end-use participants. The concept of an open specification is intended to allow anyone to implement the signaling systems, the automation server or the automation clients.
Published: 2009

26. Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector

Author: E. Blaufuss, Jenni Adams, A. Schukraft, K. Laihem, J.-P. Hülß, S. Hickford, R. G. Stokstad, M. C. Stoufer, S. Schlenstedt, H. S. Matis, Dirk Ryckbosch, D. Rutledge, R. Wischnewski, H. Leich, D. Turcan, S. M. Movit, Francis Halzen, O. Fadiran, P. Berghaus, Christopher Wiebusch, J. W. Nam, S. Euler, J. Petrovic, M. V. D'Agostino, Albrecht Karle, R. M. Gunasingha, D. R. Nygren, K. Rawlins, Damian Pieloth, D. Hubert, James Madsen, Jon Dumm, M. Prikockis, T. Waldenmaier, Teresa Montaruli, C. Pérez de los Heros, John Heise, M. R. Duvoort, S. Odrowski, Marek Kowalski, P. Roth, J. J. Beatty, A. Piegsa, H. Landsman, M. Krasberg, Joanna Kiryluk, Karen Andeen, Todor Stanev, C. Wendt, A. Wiedemann, Christian Bohm, K. Hoshina, Glenn Spiczak, M. Danninger, C. T. Day, David A. Schneider, M. Olivo, J. A. Goodman, L. Köpke, A. Slipak, S. Tilav, F. Descamps, D. Breder, H. Miyamoto, K. Meagher, Reina H. Maruyama, N. Milke, George Japaridze, D. Berley, G. C. Hill, E. A. Strahler, M. Schunck, K. Mase, T. Kowarik, S. Yoshida, W. R. Edwards, Y. Hasegawa, A. Mohr, Laura C. Bradley, Spencer Klein, Michael J. Baker, S. J. Patton, K. H. Becker, R. Franke, O. Depaepe, M. Tluczykont, L. Gladstone, P. Nießen, R. Nahnhauer, G. Wikström, T. Griesel, B. Voigt, S. Stoyanov, O. Engdegård, C. Walck, A. Lucke, P. B. Price, Peter Mészáros, A. R. Fazely, Tyce DeYoung, Thomas K. Gaisser, G. B. Yodh, Kara Hoffman, Y. Sestayo, P. A. Toale, S. Grullon, R. Gozzini, Xinhua Bai, John Clem, T. Straszheim, K. Kuehn, S. Seunarine, M. Stamatikos, Carsten Rott, J. Lünemann, D. J. Boersma, R. C. Bay, Juan Carlos Diaz-Velez, Q. Swillens, S. Panknin, Fabian Kislat, A. Tepe, J. L. Kelley, Markus Ahlers, Ph. Herquet, Kael Hanson, C. P. McParland, G. Stephens, S. Westerhoff, O. Tarasova, T. O. B. Schmidt, M. Bissok, Dirk Lennarz, D. Z. Besson, A. Van Overloop, E. Middell, Karl-Heinz Sulanke, K. Beattie, Wolfgang Rhode, R. Porrata, S. Böser, A. Goldschmidt, Xianwu Xu, Kurt Woschnagg, O. Schulz, C. Roucelle, Elisa Bernardini, R. L. Imlay, Christian Spiering, Konstancja Satalecka, Paul Evenson, M. Ono, S. Knops, Justin Vandenbroucke, Elisa Resconi, Samvel Ter-Antonyan, K. Münich, W. Huelsnitz, J. L. Bazo Alba, Paolo Desiati, J. P. Rodrigues, J. Berdermann, M. Ribordy, S. Bechet, K. Helbing, H. G. Sander, T. Stezelberger, S. Hussain, Chad Finley, D. Bertrand, Dmitry Chirkin, J. K. Becker, T. Feusels, S. Klepser, T. Castermans, Alexander Kappes, J. E. Jacobsen, F. Rothmaier, P. Redl, Rasha Abbasi, L. Gerhardt, R. J. Lauer, C. Ha, K. Hultqvist, Darren Grant, M. M. Foerster, A. Silvestri, Timo Karg, Nathan Whitehorn, I. Taboada, Aya Ishihara, J. Auffenberg, C. De Clercq, T. Burgess, J. Dreyer, J. C. Gallagher, Y. Abdou, S.J. Lafebre, M. L. Benabderrahmane, G. W. Sullivan, James E. Braun, M. Gurtner, David A. Williams, Markus Ackermann, Allan Hallgren, S. W. Barwick, Johan Lundberg, Pratik Majumdar, B. D. Fox, R. Ehrlich, Paraic A. Kenny, Takao Kuwabara, B. Christy, Seth M. Cohen, D. Seckel, J. Bolmont, Karl-Heinz Kampert, R. Ganugapati, A. C. Pohl, Kirill Filimonov, A. Olivas, D. F. Cowen, J. M. Joseph, R. Morse, Subir Sarkar, P. O. Hulth, J. Eisch, G. de Vries-Uiterweerd, B. Semburg, C. Terranova, M. Merck, M. Walter, A. Rizzo, H. Wissing, L. Demirörs, R. W. Ellsworth, S. H. Seo, Hermann Kolanoski, M. Labare, K. Han, Axel Groß, Olga Botner, Henrik J. Johansson, Anna Franckowiak, N. Potthoff, G. Kohnen, D. Tosi, N. van Eijndhoven, Gerald Przybylski, and M. Inaba
Subjects: Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics::Instrumentation and Detectors, Dark matter, FOS: Physical sciences, General Physics and Astronomy, 01 natural sciences, 7. Clean energy, Nuclear physics, WIMP, 0103 physical sciences, ddc:550, 010306 general physics, Neutrino oscillation, Neutrino Telescope, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Muon, Annihilation, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Neutrino detector, 13. Climate action, Neutralino, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live-time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the WIMP-proton cross-sections for WIMP masses in the range 250 - 5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun., 5 pages, 4 figures. Accepted for publication in Phys. Rev. Lett
Published: 2009

27. The IceCube data acquisition system: Signal capture, digitization, and timestamping

Author: Chris Wendt, Spencer Klein, Subir Sarkar, J. M. Joseph, A. Laundrie, Chad Finley, D. Bertrand, Ignacio Taboada, C. P. McParland, Albrecht Karle, J. Ludvig, A. Silvestri, E. Kujawski, P. B. Price, T. O. B. Schmidt, S. Klepser, H. Kawai, Kara Hoffman, Y. Sestayo, Peter Mészáros, Karen Andeen, J. Ahrens, K. Mase, K. Meagher, Kurt Woschnagg, Paul Evenson, Henrik J. Johansson, A. Goldschmidt, J. Pretz, M. Danninger, Wolfgang Rhode, J. L. Kelley, Todor Stanev, Dawn Williams, W. Huelsnitz, K. Hoshina, A. Piegsa, Aya Ishihara, Markus Ahlers, M. M. Foerster, Dmitry Chirkin, K. Beattie, O. Schulz, Alexander Kappes, M. Gurtner, K. Helbing, Glenn Spiczak, S. Kleinfelder, Kael Hanson, F. Descamps, H. Miyamoto, R. Morse, B. Hughey, Anna Franckowiak, N. Potthoff, Jay Gallagher, K. H. Becker, Allan Hallgren, A. Meli, Steven W. Barwick, Johan Lundberg, T. Waldenmaier, J. W. Nam, M. Ribordy, R. Porrata, C. Vogt, B. D. Fox, P. Berghaus, J. Auffenberg, S. Euler, K. Laihem, K. Rawlins, Damian Pieloth, George Japaridze, D. Hubert, C. Walck, S. J. Patton, Reina H. Maruyama, M. Labare, D. Z. Besson, Samvel Ter-Antonyan, Chance W. Lewis, Paolo Desiati, R. Franke, K. Münich, A. Lucke, K. Kuehn, W. R. Edwards, Thomas K. Gaisser, G. B. Yodh, O. Engdegård, Chinh Vu, Dirk Ryckbosch, R. Ganugapati, A. C. Pohl, J. E. Sopher, D. F. Cowen, S. Stoyanov, D. Glowacki, A. Groß, H. F. Chen, R. Ehrlich, A. Olivas, Carsten Rott, K. Han, H. Wissing, C. Ha, M. Merck, A. Mohr, James Madsen, Soebur Razzaque, T. DeYoung, S. Hussain, L. Köpke, Dave Nygren, R. Nahnhauer, M. Hellwig, A. Van Overloop, Elisa Resconi, C. Roucelle, B. Bingham, Nathan Whitehorn, R. Gozzini, S. Schlenstedt, P. Herquet, S. Odrowski, Marek Kowalski, T. Straszheim, H. S. Matis, R.H. Minor, Joanna Kiryluk, E. Blaufuss, Olga Botner, H. G. Sander, D. Wharton, M. R. Duvoort, A. J. Smith, A. Tepe, O. Tarasova, R. L. Imlay, C. Wiedemann, W.J. Robbins, Julia Becker, D. Turcan, M. Ono, Teresa Montaruli, S. Westerhof, P. Sandstrom, Francis Halzen, T. Burgess, P. Redl, Karl-Heinz Sulanke, B. Christy, R. W. Ellsworth, J. Dreyer, H. Landsman, J. L. Bazo Alba, O. Fadiran, S. Grullon, V. Viscomi, Xianwu Xu, J. P. Dumm, S. Panknin, F. Rothmaier, J. Bolmont, G. Kohnen, D. Breeder, T. Kowarik, O. Depaepe, J.-P. Hülß, D. Leier, D. Tosi, M. Krasberg, Fabian Kislat, T. Messarius, J. P. Rodrigues, J. Lünemann, T. Stezelberger, J. C. Díaz-Vélez, James E. Braun, M. V. D'Agostino, B. Voigt, Darren Grant, T. Feusels, Q. Swillens, M. Baker, L. Demirörs, N. van Eijndhoven, Karl-Heinz Kampert, Kirill Filimonov, C. Song, W. Carithers, J. E. Jacobsen, R. Hardtke, G. W. Sullivan, S. Tilav, Xinhua Bai, M. Olivo, Klas Hultqvist, R. C. Bay, L. Gerhardt, H. Waldmann, C. T. Day, A. Mokhtarani, R. J. Lauer, C. Pérez de los Heros, John Heise, S. Yoshida, S. Seunarine, Christian Spiering, Gerald Przybylski, M. Inaba, E. A. Strahler, S. Böser, M. C. Stoufer, C. De Clercq, Christian Bohm, Konstancja Satalecka, D. Hays, Joseph T. Hodges, T. Becka, Justin Vandenbroucke, D. Rutledge, H. Leich, M. Walter, A. Rizzo, Markus Ackermann, S. M. Movit, S. H. Seo, Rasha Abbasi, D. Berley, John Clem, David A. Schneider, G. C. Hill, A. Muratas, D. J. Boersma, L. Gladstone, D. Seckel, G. Wikström, T. Griesel, Hermann Kolanoski, A. R. Fazely, P. A. Toale, A. W. Jones, T. Castermans, P. Roth, Christopher Wiebusch, Anna Davour, J. Haugen, D. Wahl, Timo Karg, P. O. Hulth, J. Eisch, M. Tluczykont, T. Kuwabara, G. de Vries-Uiterweerd, B. Semburg, Elisa Bernardini, J. Petrovic, R. M. Gunasingha, J. A. Goodman, Jenni Adams, S. Hickford, R. G. Stokstad, R. Wischnewski, Y. Hasegawa, and P. Nießen
Subjects: AMANDA, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, FOS: Physical sciences, Astrophysics, Neutrino telescope, Signal, High Energy Physics - Experiment, IceCube Neutrino Observatory, Nuclear physics, High Energy Physics - Experiment (hep-ex), Icecube, Data acquisition, Signal digitization, ddc:530, Nuclear Experiment (nucl-ex), Nuclear Experiment, Instrumentation, Physics, business.industry, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, Timestamping, Instrumentation and Detectors (physics.ins-det), Analog signal, Transmission (telecommunications), Systems design, Timestamp, business, Computer hardware
Abstract: IceCube is a km-scale neutrino observatory under construction at the South Pole with sensors both in the deep ice (InIce) and on the surface (IceTop). The sensors, called Digital Optical Modules (DOMs), detect, digitize and timestamp the signals from optical Cherenkov-radiation photons. The DOM Main Board (MB) data acquisition subsystem is connected to the central DAQ in the IceCube Laboratory (ICL) by a single twisted copper wire-pair and transmits packetized data on demand. Time calibration is maintained throughout the array by regular transmission to the DOMs of precisely timed analog signals, synchronized to a central GPS-disciplined clock. The design goals and consequent features, functional capabilities, and initial performance of the DOM MB, and the operation of a combined array of DOMs as a system, are described here. Experience with the first InIce strings and the IceTop stations indicates that the system design and performance goals have been achieved., 42 pages, 20 figures, submitted to Nuclear Instruments and Methods A
Published: 2009

28. ERRATUM: 'Search for High-Energy Muon Neutrinos from the 'Naked-Eye' GRB 080319B with the Icecube Neutrino Telescope' (2009, ApJ, 701, 1721)

Author: Karl-Heinz Sulanke, A. Piegsa, Karen Andeen, G. W. Sullivan, James E. Braun, S. Grullon, S. Panknin, S. J. Patton, J. M. Joseph, P. Berghaus, Fabian Kislat, R. Nahnhauer, A. Van Overloop, K. H. Kampert, F. Rothmaier, K. Hultqvist, M. V. D'Agostino, C. T. Day, David A. Schneider, K. Han, E. A. Strahler, S. Euler, M. Danninger, Darren Grant, J. L. Kelley, Markus Ahlers, M. Labare, P. Roth, C. P. McParland, Johan Lundberg, M. Ono, J. L. Bazo Alba, Olga Botner, I. Taboada, D. Berley, G. C. Hill, T. Castermans, Chad Finley, N. Milke, Pratik Majumdar, George Japaridze, C. Terranova, Dirk Lennarz, A. Goldschmidt, S. Hussain, T. Feusels, Michael J. Baker, R. Porrata, Samvel Ter-Antonyan, J. E. Jacobsen, R. Morse, Damian Pieloth, D. Hubert, L. Köpke, L. Gerhardt, D. Z. Besson, Henrik J. Johansson, D. Bertrand, R. Ganugapati, A. C. Pohl, L. Gladstone, D. Seckel, O. Engdegård, J. W. Nam, W. Huelsnitz, Timo Karg, J. M. Clem, D. F. Cowen, S. Schlenstedt, M. R. Duvoort, Anna Franckowiak, N. Potthoff, T. Burgess, Jon Dumm, M. Prikockis, T. Waldenmaier, Joanna Kiryluk, Subir Sarkar, D. R. Nygren, Elisa Resconi, Nathan Whitehorn, P. B. Price, J. Berdermann, G. Stephens, S. Westerhoff, M. Tluczykont, P. Herquet, S. Odrowski, Marek Kowalski, A. Wiedemann, K. Helbing, M. Stamatikos, A. Silvestri, A. Slipak, S. Tilav, Jens Madsen, O. Tarasova, Todor Stanev, C. Wendt, M. Gurtner, T. Kowarik, H. G. Sander, F. Descamps, G. Kohnen, H. Miyamoto, T. O. B. Schmidt, Christian Spiering, Y. Hasegawa, Kael Hanson, D. Tosi, E. Blaufuss, P. Nießen, B. Voigt, R. Franke, K. Münich, C. Walck, D. Rutledge, J. Auffenberg, K.-H. Becker, B. D. Fox, K. Hoshina, S. Knops, Justin Vandenbroucke, Kurt Woschnagg, A. Lucke, Glenn Spiczak, M. M. Foerster, Xinhua Bai, Paul Evenson, Thomas K. Gaisser, G. B. Yodh, N. van Eijndhoven, H. Leich, J. C. Gallagher, M. Schunck, W. R. Edwards, A. Schukraft, K. Laihem, Q. Swillens, M. C. Stoufer, Gerald Przybylski, M. Inaba, Paolo Desiati, Reina H. Maruyama, A. Mohr, Dmitry Chirkin, K. Rawlins, Allan Hallgren, Laura C. Bradley, Alexander Kappes, Dirk Ryckbosch, R. L. Imlay, O. Depaepe, M. Krasberg, S. Stoyanov, S. M. Movit, Albrecht Karle, K. Kuehn, J. Lünemann, M. Merck, D. J. Boersma, R. C. Bay, Peter Mészáros, R. Gozzini, Juan Carlos Diaz-Velez, S. Böser, S. Klepser, A. R. Fazely, A. Tepe, S. Yoshida, K. Meagher, Teresa Montaruli, R. J. Lauer, J.-P. Hülß, C. De Clercq, K. Mase, H. S. Matis, C. Roucelle, K. Beattie, David A. Williams, D. Turcan, Francis Halzen, O. Schulz, J. Dreyer, Markus Ackermann, S. W. Barwick, O. Fadiran, M. Ribordy, P. O. Hulth, J. Eisch, C. Ha, M. L. Benabderrahmane, G. de Vries-Uiterweerd, Paraic A. Kenny, Takao Kuwabara, B. Semburg, E. Middell, Elisa Bernardini, H. Wissing, B. Christy, A. Ishihara, J. Bolmont, J. Petrovic, R. M. Gunasingha, Axel Groß, M. Walter, A. Rizzo, S. H. Seo, Carsten Rott, T. Straszheim, M. Bissok, Julia Becker, Xianwu Xu, C. Bohm, C. Pérez de los Heros, John Heise, M. Olivo, J. A. Goodman, G. Wikström, T. Griesel, Spencer Klein, D. Breder, Kara Hoffman, Y. Sestayo, Tyce DeYoung, P. A. Toale, S. Seunarine, Wolfgang Rhode, Rasha Abbasi, S. Bechet, P. Redl, Jenni Adams, L. Demirörs, Kirill Filimonov, Christopher Wiebusch, S. Hickford, R. G. Stokstad, R. Wischnewski, S. Cohen, R. W. Ellsworth, J. P. Rodrigues, T. Stezelberger, Y. Abdou, H. Landsman, Konstancja Satalecka, Hermann Kolanoski, R. Ehrlich, A. Olivas, Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Muon, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Solar neutrino, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Astronomy and Astrophysics, Astrophysics, Solar neutrino problem, 01 natural sciences, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Neutrino detector, Space and Planetary Science, 0103 physical sciences, Naked eye, Neutrino, Neutrino astronomy, 010306 general physics, Gamma-ray burst, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: We have noticed some mistakes in formulae (A2) and (A5) in the appendix of our paper. The errors are not present in the code used in the analysis and hence none of the plots or results is affected. The correct formulae are below.
Published: 2009

29. A TPC detector for the study of high multiplicity heavy ion collisions

Author: C.W. Harnden, G. Odyniec, T. J. M. Symons, C. P. McParland, R. Wright, S. Abbott, F. S. Bieser, R. Jones, G. Rai, H. S. Matis, A. Arthur, H. G. Ritter, H. H. Wieman, S. Kleinfelder, M. Wright, M. Nakamura, H.G. Pugh, A. Rudge, D. L. Olson, K.L. Lee, and J. Bercovitz
Subjects: Nuclear physics, Physics, Nuclear and High Energy Physics, Time projection chamber, Physics::Instrumentation and Detectors, Projectile, Nuclear Theory, Detector, Sampling (statistics), Heavy ion, High multiplicity, Nuclear Experiment, Front end electronics
Abstract: The design of a Time Projection Chamber (TPC) detector with complete pad coverage is presented. The TPC will allow the measurements of high multiplicity (~200 tracks), relativistic nucleus-nucleus collisions initiated with the heaviest, most energetic projectiles available at the LBL BEVALAC accelerator facility. The front end electronics, composed of over 15,000 time sampling channels, will be located on the chamber.
Published: 1991

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

Author: A. Achterberg, M. Ackermann, J. Adams, J. Ahrens, K. Andeen, J. Auffenberg, X. Bai, B. Baret, S. W. Barwick, R. Bay, K. Beattie, T. Becka, J. K. Becker, K.-H. Becker, P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. Besson, E. Blaufuss, D. J. Boersma, C. Bohm, J. Bolmont, S. Böser, O. Botner, A. Bouchta, J. Braun, T. Burgess, T. Castermans, D. Chirkin, B. Christy, J. Clem, D. F. Cowen, M. V. D’Agostino, A. Davour, C. T. Day, C. De Clercq, L. Demirörs, F. Descamps, P. Desiati, T. DeYoung, J. C. Diaz-Velez, J. Dreyer, J. P. Dumm, M. R. Duvoort, W. R. Edwards, R. Ehrlich, J. Eisch, R. W. Ellsworth, P. A. Evenson, O. Fadiran, A. R. Fazely, K. Filimonov, C. Finley, M. M. Foerster, B. D. Fox, A. Franckowiak, R. Franke, T. K. Gaisser, J. Gallagher, R. Ganugapati, H. Geenen, L. Gerhardt, A. Goldschmidt, J. A. Goodman, R. Gozzini, T. Griesel, A. Groß, S. Grullon, R. M. Gunasingha, M. Gurtner, C. Ha, A. Hallgren, F. Halzen, K. Han, K. Hanson, D. Hardtke, R. Hardtke, J. E. Hart, Y. Hasegawa, T. Hauschildt, D. Hays, J. Heise, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, J. Hodges, K. D. Hoffman, B. Hommez, K. Hoshina, D. Hubert, B. Hughey, J.-P. Hülß, P. O. Hulth, K. Hultqvist, S. Hundertmark, M. Inaba, A. Ishihara, J. Jacobsen, G. S. Japaridze, H. Johansson, A. Jones, J. M. Joseph, K.-H. Kampert, A. Kappes, T. Karg, A. Karle, H. Kawai, J. L. Kelley, F. Kislat, N. Kitamura, S. R. Klein, S. Klepser, G. Kohnen, H. Kolanoski, L. Köpke, M. Kowalski, T. Kowarik, M. Krasberg, K. Kuehn, M. Labare, H. Landsman, R. Lauer, H. Leich, D. Leier, I. Liubarsky, J. Lundberg, J. Lünemann, J. Madsen, R. Maruyama, K. Mase, H. S. Matis, T. McCauley, C. P. McParland, A. Meli, T. Messarius, P. Mészáros, H. Miyamoto, A. Mokhtarani, T. Montaruli, A. Morey, R. Morse, S. M. Movit, K. Münich, R. Nahnhauer, J. W. Nam, P. Nießen, D. R. Nygren, H. Ögelman, A. Olivas, S. Patton, C. Peña-Garay, C. Pérez de los Heros, A. Piegsa, D. Pieloth, A. C. Pohl, R. Porrata, J. Pretz, P. B. Price, G. T. Przybylski, K. Rawlins, S. Razzaque, E. Resconi, W. Rhode, M. Ribordy, A. Rizzo, S. Robbins, P. Roth, F. Rothmaier, C. Rott, D. Rutledge, D. Ryckbosch, H.-G. Sander, S. Sarkar, K. Satalecka, S. Schlenstedt, T. Schmidt, D. Schneider, D. Seckel, B. Semburg, S. H. Seo, Y. Sestayo, S. Seunarine, A. Silvestri, A. J. Smith, M. Solarz, C. Song, J. E. Sopher, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, T. Stezelberger, R. G. Stokstad, M. C. Stoufer, S. Stoyanov, E. A. Strahler, T. Straszheim, K.-H. Sulanke, G. W. Sullivan, T. J. Sumner, I. Taboada, O. Tarasova, A. Tepe, L. Thollander, S. Tilav, M. Tluczykont, P. A. Toale, D. Tosi, D. Turčan, N. van Eijndhoven, J. Vandenbroucke, A. Van Overloop, V. Viscomi, B. Voigt, W. Wagner, C. Walck, H. Waldmann, M. Walter, Y.-R. Wang, C. Wendt, C. H. Wiebusch, C. Wiedemann, G. Wikström, D. R. Williams, R. Wischnewski, H. Wissing, K. Woschnagg, X. W. Xu, G. Yodh, S. Yoshida, and J. D. Zornoza
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Cosmic ray, Elementary particle, Massless particle, Neutrino detector, Muon collider, High Energy Physics::Experiment, Neutrino, Lepton
Abstract: A search for TeV-PeV muon neutrinos with AMANDA-II data collected between 2000 and 2003 established an upper limit of E2Φ90%C:L
Published: 2008

31. Detection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector

Author: A. Achterberg, M. Ackermann, J. Adams, J. Ahrens, K. Andeen, J. Auffenberg, X. Bai, B. Baret, S. W. Barwick, R. Bay, K. Beattie, T. Becka, J. K. Becker, K.-H. Becker, M. Beimforde, P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. Besson, E. Blaufuss, D. J. Boersma, C. Bohm, J. Bolmont, S. Böser, O. Botner, A. Bouchta, J. Braun, C. Burgess, T. Burgess, T. Castermans, D. Chirkin, B. Christy, J. Clem, D. F. Cowen, M. V. D’Agostino, A. Davour, C. T. Day, C. De Clercq, L. Demirörs, F. Descamps, P. Desiati, T. DeYoung, J. C. Diaz-Velez, J. Dreyer, J. P. Dumm, M. R. Duvoort, W. R. Edwards, R. Ehrlich, J. Eisch, R. W. Ellsworth, P. A. Evenson, O. Fadiran, A. R. Fazely, K. Filimonov, C. Finley, M. M. Foerster, B. D. Fox, A. Franckowiak, R. Franke, T. K. Gaisser, J. Gallagher, R. Ganugapati, H. Geenen, L. Gerhardt, A. Goldschmidt, J. A. Goodman, R. Gozzini, T. Griesel, S. Grullon, A. Groß, R. M. Gunasingha, M. Gurtner, C. Ha, A. Hallgren, F. Halzen, K. Han, K. Hanson, D. Hardtke, R. Hardtke, J. E. Hart, Y. Hasegawa, T. Hauschildt, D. Hays, J. Heise, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, J. Hodges, K. D. Hoffman, B. Hommez, K. Hoshina, D. Hubert, B. Hughey, J.-P. Hülß, P. O. Hulth, K. Hultqvist, S. Hundertmark, M. Inaba, A. Ishihara, J. Jacobsen, G. S. Japaridze, H. Johansson, A. Jones, J. M. Joseph, K.-H. Kampert, A. Kappes, T. Karg, A. Karle, H. Kawai, J. L. Kelley, F. Kislat, N. Kitamura, S. R. Klein, S. Klepser, G. Kohnen, H. Kolanoski, L. Köpke, M. Kowalski, T. Kowarik, M. Krasberg, K. Kuehn, M. Labare, H. Landsman, R. Lauer, H. Leich, D. Leier, I. Liubarsky, J. Lundberg, J. Lünemann, J. Madsen, R. Maruyama, K. Mase, H. S. Matis, T. McCauley, C. P. McParland, K. Meagher, A. Meli, T. Messarius, P. Mészáros, H. Miyamoto, A. Mokhtarani, T. Montaruli, A. Morey, R. Morse, S. M. Movit, K. Münich, R. Nahnhauer, J. W. Nam, P. Nießen, D. R. Nygren, A. Olivas, S. Patton, C. Peña-Garay, C. Pérez de los Heros, A. Piegsa, D. Pieloth, A. C. Pohl, R. Porrata, J. Pretz, P. B. Price, G. T. Przybylski, K. Rawlins, S. Razzaque, P. Redl, E. Resconi, W. Rhode, M. Ribordy, A. Rizzo, S. Robbins, P. Roth, F. Rothmaier, C. Rott, D. Rutledge, D. Ryckbosch, H.-G. Sander, S. Sarkar, K. Satalecka, S. Schlenstedt, T. Schmidt, D. Schneider, D. Seckel, B. Semburg, S. H. Seo, Y. Sestayo, S. Seunarine, A. Silvestri, A. J. Smith, C. Song, J. E. Sopher, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, T. Stezelberger, R. G. Stokstad, M. C. Stoufer, S. Stoyanov, E. A. Strahler, T. Straszheim, K.-H. Sulanke, G. W. Sullivan, T. J. Sumner, I. Taboada, O. Tarasova, A. Tepe, L. Thollander, S. Tilav, M. Tluczykont, P. A. Toale, D. Tosi, D. Turčan, N. van Eijndhoven, J. Vandenbroucke, A. Van Overloop, G. de Vries-Uiterweerd, V. Viscomi, B. Voigt, W. Wagner, C. Walck, H. Waldmann, M. Walter, Y.-R. Wang, C. Wendt, C. H. Wiebusch, G. Wikström, D. R. Williams, R. Wischnewski, H. Wissing, K. Woschnagg, X. W. Xu, G. Yodh, S. Yoshida, and J. D. Zornoza
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, education.field_of_study, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, Population, Detector, Astrophysics (astro-ph), High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Solar neutrino problem, Astrophysics, Neutrino detector, Astronomia, Measurements of neutrino speed, ddc:530, High Energy Physics::Experiment, Neutrino astronomy, Neutrino, education
Abstract: The IceCube neutrino detector is a cubic kilometer TeV to PeV neutrino detector under construction at the geographic South Pole. The dominant population of neutrinos detected in IceCube is due to meson decay in cosmic-ray air showers. These atmospheric neutrinos are relatively well understood and serve as a calibration and verification tool for the new detector. In 2006, the detector was approximately 10% completed, and we report on data acquired from the detector in this configuration. We observe an atmospheric neutrino signal consistent with expectations, demonstrating that the IceCube detector is capable of identifying neutrino events. In the first 137.4 days of live time, 234 neutrino candidates were selected with an expectation of 211±76.1(syst) ±14.5(stat) events from atmospheric neutrinos. © 2007 The American Physical Society.
Published: 2007

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

Author: H. Landsman, S. Schlenstedt, J. L. Kelley, John Clem, D. Rutledge, C. Wiedemann, H. Leich, D. J. Boersma, R. Porrata, Konstancja Satalecka, D. Hays, Jenni Adams, L. Gerhardt, George Japaridze, J. Auffenberg, C. Ha, K. Rawlins, Hakki Ögelman, S. H. Seo, J.D. Zornoza, D. Leier, Christian Spiering, Kara Hoffman, Y. Sestayo, Subir Sarkar, A. J. Smith, R. G. Stokstad, Wolfgang Rhode, A. Meli, R. Wischnewski, B. Hommez, Delia Tosi, James Madsen, Soebur Razzaque, P. B. Price, W. Wagner, Joseph T. Hodges, Justin Vandenbroucke, T. Burgess, A. Piegsa, M. Solarz, J. M. Joseph, I. Liubarsky, Ph. Herquet, N. Kitamura, B. Christy, K. Mase, A. Ishihara, T. O. B. Schmidt, J. Bolmont, R. Ehrlich, Kael Hanson, A. Olivas, Teresa Montaruli, T. J. Sumner, G. Kohnen, S. Grullon, R. M. Gunasingha, L. Demirörs, Elisa Resconi, M. Ribordy, E. Blaufuss, S. Böser, J. E. Hart, S. Seunarine, F. Rothmaier, Michael Stamatikos, A. Morey, K. Beattie, B. D. Fox, Kurt Woschnagg, Paul Evenson, P. Berghaus, T. Kowarik, K. Hultqvist, R. W. Ellsworth, J. A. Goodman, Fabian Kislat, N. van Eijndhoven, R. Morse, K. Helbing, A. Franckowiak, Albrecht Karle, Yi Wang, Paolo Desiati, Gerald Przybylski, M. Inaba, D. Z. Besson, T. McCauley, A. Van Overloop, Dmitry Chirkin, S. Robbins, M. C. Stoufer, J. Pretz, M. Krasberg, H. Waldmann, S. M. Movit, V. Viscomi, S. Patton, B. Voigt, Xinhua Bai, Alexander Kappes, M. Hellwig, Hermann Kolanoski, R. Gozzini, P. Meszaros, J. Dreyer, K. Han, M. Labare, A. W. Jones, Elisa Bernardini, K. H. Sulanke, H. G. Sander, P. Roth, A. Tepe, Todor Stanev, S. Yoshida, Olga Botner, A. Mokhtarani, Dawn Williams, K. Hoshina, Carlos Pena-Garay, C. Wendt, Johan Lundberg, Glenn Spiczak, O. Tarasova, H. Miyamoto, John S. Gallagher, M. Tluczykont, Chad Finley, D. Bertrand, D. F. Cowen, J. K. Becker, Christian Bohm, David A. Schneider, J.P. Hulss, H. Kawai, R. Ganugapati, A. C. Pohl, J. E. Sopher, S. R. Klein, D. Berley, G. C. Hill, A. Achterberg, B. Hughey, D. Seckel, K. Kuehn, W. R. Edwards, Heiko Geenen, A. R. Fazely, R. Franke, Tyce DeYoung, P. A. Toale, M. Gurtner, C. Walck, T. Karg, M. M. Foerster, S. Klepser, H. A. B. Johansson, T. Hauschildt, Thomas K. Gaisser, G. B. Yodh, Ignacio Taboada, Adam Bouchta, C.P. de los Heros, Allan Hallgren, T. Castermans, R. J. Lauer, C. De Clercq, D. R. Nygren, S. Hundertmark, Marek Kowalski, Markus Ackermann, T. Stezelberger, S. W. Barwick, G. W. Sullivan, H. S. Matis, M. V. D'Agostino, C. Song, D. Turcan, F. Descamps, Francis Halzen, O. Fadiran, C. T. Day, M. Walter, A. Rizzo, E. A. Strahler, T. Messarius, A. Gross, A. Silvestri, Karen Andeen, R. Nahnhauer, J. Ahrens, Anna Davour, J. Braun, Janet Jacobsen, P. O. Hulth, J. Eisch, B. Semburg, Damian Pieloth, D. Hubert, H. Wissing, L. Köpke, Kirill Filimonov, T. Straszheim, M. R. Duvoort, B. Baret, S. Tilav, Y. Hasegawa, K. H. Kampert, C. P. McParland, J. Lünemann, A. Goldschmidt, D. Hardtke, R. C. Bay, K.-H. Becker, Juan Carlos Diaz-Velez, S. Stoyanov, Dirk Ryckbosch, Carsten Rott, K. Münich, J. W. Nam, L. Thollander, Xianwu Xu, J. P. Dumm, Reina H. Maruyama, H. Wiebusch, R. Hardtke, P. Niessen, John Heise, T. Becka, G. Wikström, and T. Griesel
Subjects: Astroparticle physics, Physics, Nuclear and High Energy Physics, Range (particle radiation), Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), High Energy Physics::Phenomenology, FOS: Physical sciences, Flux, Cosmic ray, Astrophysics, Spectral line, Astronomia, Neutron detection, ddc:530, High Energy Physics::Experiment, Neutrino
Abstract: A search for TeV - PeV muon neutrinos from unresolved sources was performed on AMANDA-II data collected between 2000 and 2003 with an equivalent livetime of 807 days. This diffuse analysis sought to find an extraterrestrial neutrino flux from sources with non-thermal components. The signal is expected to have a harder spectrum than the atmospheric muon and neutrino backgrounds. Since no excess of events was seen in the data over the expected background, an upper limit of E^{2}\Phi_{90% C.L.} < 7.4 x 10^{-8} GeV cm^{-2} s^{-1} sr^{-1} is placed on the diffuse flux of muon neutrinos with a \Phi \propto E^{-2} spectrum in the energy range 16 TeV to 2.5 PeV. This is currently the most sensitive \Phi \propto E^{-2} diffuse astrophysical neutrino limit. We also set upper limits for astrophysical and prompt neutrino models, all of which have spectra different than \Phi \propto E^{-2}., Comment: 47 pages, 13 figures. This includes the original document and an erratum for the effective area tables
Published: 2007

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

Author: M. V. D'Agostino, C. Song, Albrecht Karle, C. T. Day, J. Pretz, J. M. Joseph, I. Liubarsky, Matthias Leuthold, K. Hultqvist, D. R. Nygren, R. Ehrlich, A. Olivas, E. A. Strahler, Carlos Pérez de los Heros, Jenni Adams, Marek Kowalski, D. Leier, T. Messarius, Kara Hoffman, Wolfgang Rhode, A. Meli, Christian Bohm, S. H. Seo, J.D. Zornoza, David A. Schneider, K. Kuehn, W. R. Edwards, H. Waldmann, P. Berghaus, Todor Stanev, Dawn Williams, C. Wendt, W. Wagner, T. Feser, Christian Spiering, F. Descamps, P. Roth, H. S. Matis, H. Miyamoto, J. E. Hart, K. Rawlins, D. Berley, M. Ribordy, G. C. Hill, R. G. Stokstad, Joseph T. Hodges, Justin Vandenbroucke, M. Kestel, Johan Lundberg, C. Walck, H. A. B. Johansson, H. Landsman, B. Christy, James Madsen, Soebur Razzaque, K. Helbing, N. Kitamura, Thomas K. Gaisser, G. B. Yodh, R. Morse, D. Turcan, Francis Halzen, N. van Eijndhoven, A. Ishihara, J. Bolmont, D. Seckel, M. Tluczykont, J. Dreyer, Teresa Montaruli, T. Castermans, K. Hoshina, D. Z. Besson, Glenn Spiczak, L. Gerhardt, Gerald Przybylski, S. Klepser, S. Robbins, B. Hommez, Heiko Geenen, A. R. Fazely, Tyce DeYoung, A. Piegsa, P. A. Toale, J. L. Kelley, D. Hays, E. Blaufuss, C. De Clercq, O. Fadiran, D. F. Cowen, B. Hughey, A. W. Jones, R. Ganugapati, A. C. Pohl, J. E. Sopher, K. Mase, T. McCauley, M. C. Stoufer, A. Achterberg, Markus Ackermann, S. W. Barwick, M. Solarz, S. M. Movit, K. Han, John Clem, C.P. Burgess, D. J. Boersma, D. Rutledge, D.W. Atlee, Ignacio Taboada, K. Beattie, Olga Botner, A. Morey, H. Leich, O. Tarasova, Subir Sarkar, X. W. Xu, A. Mokhtarani, Christopher Wiebusch, R. Wischnewski, M. Hellwig, A. Van Overloop, Hermann Kolanoski, R. Porrata, Peter Mészáros, J. P. Hulss, Elisa Bernardini, P. B. Price, K. H. Sulanke, H. G. Sander, T. J. Sumner, L. Demirörs, R. M. Gunasingha, Hakki Ögelman, A. J. Smith, T. O. B. Schmidt, G. Kohnen, T. Stezelberger, R. W. Ellsworth, T. Burgess, John N. Bahcall, S. Seunarine, Michael Stamatikos, S. Grullon, J. A. Goodman, Kurt Woschnagg, B. Voigt, Xinhua Bai, Paul Evenson, Dmitry Chirkin, J. W. Nam, L. Thollander, Karen Andeen, S. Stoyanov, K. Münich, P. Steffen, R. Nahnhauer, J. Lünemann, J. Ahrens, D. Hardtke, R. C. Bay, Juan Carlos Diaz-Velez, A. Gross, A. Silvestri, M. Walter, A. Rizzo, George Japaridze, S. Hundertmark, G. W. Sullivan, Elisa Resconi, S. Patton, Carlos Pena-Garay, Torsten Harenberg, Kirill Filimonov, Ph. Herquet, John Heise, Damian Pieloth, D. Hubert, T. Becka, K.-H. Becker, H. Wissing, L. Köpke, J. K. Becker, D. Bertrand, S. Böser, H. Kawai, Kael Hanson, S. R. Klein, T. Hauschildt, J. C. Gallagher, Adam Bouchta, Allan Hallgren, G. Wikström, M. Gurtner, T. Straszheim, R. Gozzini, Dirk Ryckbosch, A. Tepe, Yi Wang, Paolo Desiati, P. Niessen, K. H. Kampert, M. Krasberg, B. D. Fox, C. P. McParland, Carsten Rott, S. Yoshida, A. Goldschmidt, J. P. Dumm, J. Eisch, R. Hardtke, M. R. Duvoort, B. Baret, S. Tilav, P. O. Hulth, S. Schlenstedt, Anna Davour, J. Braun, and Janet Jacobsen
Subjects: Astroparticle physics, Physics, Nuclear and High Energy Physics, Muon, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Solar neutrino, Astrophysics (astro-ph), High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Solar neutrino problem, Sky, Astronomia, Measurements of neutrino speed, High Energy Physics::Experiment, ddc:530, Neutrino, Neutrino astronomy, media_common
Abstract: We report the results of a five-year survey of the northern sky to search for point sources of high energy neutrinos. The search was performed on the data collected with the AMANDA-II neutrino telescope in the years 2000 to 2004, with a live-time of 1001 days. The sample of selected events consists of 4282 upward going muon tracks with high reconstruction quality and an energy larger than about 100 GeV. We found no indication of point sources of neutrinos and set 90% confidence level flux upper limits for an all-sky search and also for a catalog of 32 selected sources. For the all-sky search, our average (over declination and right ascension) experimentally observed upper limit \Phi^{0}=(E/TeV)^\gamma d\Phi/dE to a point source flux of muon and tau neutrino (detected as muons arising from taus) is \Phi_{\nu_\mu}^{0} + \Phi_{\nu_\tau}^{0} = 11.1 x 10^{-11} TeV^-1 cm^-2 s^-1, in the energy range between 1.6 TeV and 2.5 PeV for a flavor ratio \Phi_{\nu_\mu}^{0} / \Phi_{\nu_\tau}^{0}= 1 and assuming a spectral index \gamma=2. It should be noticed that this is the first time we set upper limits to the flux of muon and tau neutrinos. In previous papers we provided muon neutrino upper limits only neglecting the sensitivity to a signal from tau neutrinos, which improves the limits by 10% to 16%. The value of the average upper limit presented in this work corresponds to twice the limit on the muon neutrino flux \Phi_{\nu_\mu}^{0} = 5.5 \cdot 10^{-11} TeV^-1 cm^-2 s^-1. A stacking analysis for preselected active galactic nuclei and a search based on the angular separation of the events were also performed. We report the most stringent flux upper limits to date, including the results of a detailed assessment of systematic uncertainties., Comment: 32 pages, 9 figures, submitted to Phys. Rev. D
Published: 2007

34. Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of 27 December 2004 with the AMANDA-II detector

Author: A. Achterberg, M. Ackermann, J. Adams, J. Ahrens, K. Andeen, D. W. Atlee, J. N. Bahcall, X. Bai, B. Baret, M. Bartelt, S. W. Barwick, R. Bay, K. Beattie, T. Becka, J. K. Becker, K.-H. Becker, P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. Besson, E. Blaufuss, D. J. Boersma, C. Bohm, J. Bolmont, S. Böser, O. Botner, A. Bouchta, J. Braun, C. Burgess, T. Burgess, T. Castermans, D. Chirkin, B. Christy, J. Clem, D. F. Cowen, M. V. D’Agostino, A. Davour, C. T. Day, C. De Clercq, L. Demirörs, F. Descamps, P. Desiati, T. DeYoung, J. C. Diaz-Velez, J. Dreyer, J. P. Dumm, M. R. Duvoort, W. R. Edwards, R. Ehrlich, J. Eisch, R. W. Ellsworth, P. A. Evenson, O. Fadiran, A. R. Fazely, T. Feser, K. Filimonov, B. D. Fox, T. K. Gaisser, J. Gallagher, R. Ganugapati, H. Geenen, L. Gerhardt, A. Goldschmidt, J. A. Goodman, R. Gozzini, S. Grullon, A. Groß, R. M. Gunasingha, M. Gurtner, A. Hallgren, F. Halzen, K. Han, K. Hanson, D. Hardtke, R. Hardtke, T. Harenberg, J. E. Hart, T. Hauschildt, D. Hays, J. Heise, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, J. Hodges, K. D. Hoffman, B. Hommez, K. Hoshina, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, J.-P. Hülß, A. Ishihara, J. Jacobsen, G. S. Japaridze, A. Jones, J. M. Joseph, K.-H. Kampert, A. Karle, H. Kawai, J. L. Kelley, M. Kestel, N. Kitamura, S. R. Klein, S. Klepser, G. Kohnen, H. Kolanoski, L. Köpke, M. Krasberg, K. Kuehn, H. Landsman, H. Leich, I. Liubarsky, J. Lundberg, J. Madsen, K. Mase, H. S. Matis, T. McCauley, C. P. McParland, A. Meli, T. Messarius, P. Mészáros, H. Miyamoto, A. Mokhtarani, T. Montaruli, A. Morey, R. Morse, S. M. Movit, K. Münich, R. Nahnhauer, J. W. Nam, P. Nießen, D. R. Nygren, H. Ögelman, Ph. Olbrechts, A. Olivas, S. Patton, C. Peña-Garay, C. Pérez de los Heros, A. Piegsa, D. Pieloth, A. C. Pohl, R. Porrata, J. Pretz, P. B. Price, G. T. Przybylski, K. Rawlins, S. Razzaque, F. Refflinghaus, E. Resconi, W. Rhode, M. Ribordy, A. Rizzo, S. Robbins, P. Roth, C. Rott, D. Rutledge, D. Ryckbosch, H.-G. Sander, S. Sarkar, S. Schlenstedt, T. Schmidt, D. Schneider, D. Seckel, S. H. Seo, S. Seunarine, A. Silvestri, A. J. Smith, M. Solarz, C. Song, J. E. Sopher, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, P. Steffen, T. Stezelberger, R. G. Stokstad, M. C. Stoufer, S. Stoyanov, E. A. Strahler, T. Straszheim, K.-H. Sulanke, G. W. Sullivan, T. J. Sumner, I. Taboada, O. Tarasova, A. Tepe, L. Thollander, S. Tilav, P. A. Toale, D. Turčan, N. van Eijndhoven, J. Vandenbroucke, A. Van Overloop, B. Voigt, W. Wagner, C. Walck, H. Waldmann, M. Walter, Y.-R. Wang, C. Wendt, C. H. Wiebusch, G. Wikström, D. R. Williams, R. Wischnewski, H. Wissing, K. Woschnagg, X. W. Xu, G. Yodh, S. Yoshida, and J. D. Zornoza
Subjects: Astroparticle physics, Physics, Muon, Solar flare, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), Gamma ray, General Physics and Astronomy, Astronomy, FOS: Physical sciences, Astrophysics, Galaxy, law.invention, Pulsar, law, Astronomia, High Energy Physics::Experiment, Neutrino, Flare
Abstract: On December 27th 2004, a giant gamma flare from the Soft Gamma-ray Repeater 1806-20 saturated many satellite gamma-ray detectors. This event was by more than two orders of magnitude the brightest cosmic transient ever observed. If the gamma emission extends up to TeV energies with a hard power law energy spectrum, photo-produced muons could be observed in surface and underground arrays. Moreover, high-energy neutrinos could have been produced during the SGR giant flare if there were substantial baryonic outflow from the magnetar. These high-energy neutrinos would have also produced muons in an underground array. AMANDA-II was used to search for downgoing muons indicative of high-energy gammas and/or neutrinos. The data revealed no significant signal. The upper limit on the gamma flux at 90% CL is dN/dE < 0.05 (0.5) TeV^-1 m^-2 s^-1 for gamma=-1.47 (-2). Similarly, we set limits on the normalization constant of the high-energy neutrino emission of 0.4 (6.1) TeV^-1 m^-2 s^-1 for gamma=-1.47 (-2)., 14 pages, 3 figures
Published: 2006

35. The IceCube prototype string in Amanda

Author: Kael Hanson, J. K. Becker, S. Stoyanov, P. Roth, Peter Mészáros, K. Han, B. Hommez, M. M. Foerster, Yi Wang, Paolo Desiati, D. Z. Besson, J. Lünemann, C.P. Burgess, E. A. Strahler, R. C. Bay, D. Bertrand, S. H. Seo, J.D. Zornoza, A. C. Pohl, S. R. Klein, G. S. Japaridze, J. Bolmont, A. Tepe, A. W. Jones, M. Krasberg, R. Hardtke, T. Hauschildt, P. Berghaus, Johan Lundberg, H. S. Matis, Anna Davour, K. H. Sulanke, D. Turcan, D. Hardtke, J. Braun, S. Yoshida, S. Klepser, Francis Halzen, Janet Jacobsen, M. Solarz, D. R. Nygren, T. Griesel, P. O. Hulth, J. Eisch, R. Ganugapati, J. E. Sopher, N. van Eijndhoven, P. Herquet, D. F. Cowen, J. E. Hart, K. Münich, Y. Hasegawa, T. DeYoung, S. J. Patton, J. Gallagher, Adam Bouchta, A. Piegsa, A. Achterberg, K. Andeen, C.P. de los Heros, B. Semburg, M. Labare, P. A. Evenson, Marek Kowalski, P. B. Price, S. Schlenstedt, M. Gurtner, H. Wissing, K. Mase, L. Demirors, S. Böser, R. W. Ellsworth, M. Tluczykont, Allan Hallgren, David A. Schneider, J.P. Hulss, T. O. B. Schmidt, A. Gross, G. C. Hill, B. D. Fox, A. Van Overloop, B. Baret, J. W. Nam, S. Grullon, Kurt Woschnagg, L. Thollander, F. Descamps, R. Ehrlich, D. Seckel, Heiko Geenen, P. A. Toale, J. Adams, A. Morey, J. P. Dumm, H. Landsman, A. R. Fazely, K. Kuehn, R. M. Gunasingha, Wolfgang Wagner, Dmitry Chirkin, T. Burgess, G. Kohnen, Albrecht Karle, J. L. Kelley, D. J. Boersma, Michael Stamatikos, Timo Karg, Gerald Przybylski, M. Walter, J. A. Goodman, A. Silvestri, K. Hoshina, David R. Williams, A. J. S. Smith, T. J. Sumner, H. Kolanoski, M. R. Duvoort, Glenn Spiczak, S. M. Movit, M. Ribordy, T. Stezelberger, R. Porrata, J. Dreyer, L. Gerhardt, J. Heise, K. Helbing, P. Steffen, Olga Botner, B. Hughey, A. Olivas, C. Song, J. N. Bahcall, Elisa Resconi, Anna Franckowiak, J. Hodges, R. Nahnhauer, Hakki Ögelman, C. T. Day, Elisa Bernardini, J. Clem, E. Blaufuss, J. Ahrens, T. Messarius, D. Hays, O. Tarasova, T. Kowarik, S. Hundertmark, B. Voigt, B. Christy, R. G. Stokstad, Xinhua Bai, R. Wischnewski, G. W. Sullivan, K. Hultqvist, N. Kitamura, Karl-Heinz Kampert, Kirill Filimonov, Carlos Pena-Garay, D. Leier, O. Fadiran, A. Rizzo, T. Straszheim, S. Robbins, Wolfgang Rhode, A. Meli, H. Waldmann, T. McCauley, Damian Pieloth, D. Hubert, Christian Spiering, L. Köpke, Justin Vandenbroucke, Subir Sarkar, K. Beattie, Surujhdeo Seunarine, K. Rawlins, James Madsen, Soebur Razzaque, K. D. Hoffman, A. Ishihara, T. Stanev, M. C. Stoufer, D. Rutledge, H. Leich, J. C. Diaz-Velez, M. V. D'Agostino, H. Kawai, M. Hellwig, H. G. Sander, J. M. Joseph, I. Liubarsky, C. H. Wiebusch, C. Wendt, Carsten Rott, R. Morse, T. Montaruli, H. Miyamoto, Xianwu Xu, C. Bohm, C. Walck, D. Berley, Thomas K. Gaisser, G. B. Yodh, P. Niessen, G. Wikstrom, I. Taboada, J. Auffenberg, T. Castermans, H. Johansson, T. Becka, J. Pretz, V. Viscomi, K.-H. Becker, A. Mokhtarani, C. De Clercq, M. Inaba, Markus Ackermann, Dirk Ryckbosch, S. W. Barwick, W. R. Edwards, S. Tilav, R. Gozzini, C. P. McParland, and A. Goldschmidt
Subjects: Antarctic Muon And Neutrino Detector Array, Astroparticle physics, Physics, Nuclear and High Energy Physics, Photomultiplier, Photon, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), Neutrino telescope, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy, Astrophysics, Amanda, IceCube, Data acquisition, Signal digitization, Instrumentation, Cherenkov radiation
Abstract: The Antarctic Muon And Neutrino Detector Array (Amanda) is a high-energy neutrino telescope. It is a lattice of optical modules (OM) installed in the clear ice below the South Pole Station. Each OM contains a photomultiplier tube (PMT) that detects photons of Cherenkov light generated in the ice by muons and electrons. IceCube is a cubic-kilometer-sized expansion of Amanda currently being built at the South Pole. In IceCube the PMT signals are digitized already in the optical modules and transmitted to the surface. A prototype string of 41 OMs equipped with this new all-digital technology was deployed in the Amanda array in the year 2000. In this paper we describe the technology and demonstrate that this string serves as a proof of concept for the IceCube array. Our investigations show that the OM timing accuracy is 5 ns. Atmospheric muons are detected in excellent agreement with expectations with respect to both angular distribution and absolute rate.
Published: 2006

36. First year performance of the IceCube neutrino telescope

Author: A. J. Smith, R. Wischnewski, Kael Hanson, T. Burgess, K. Hoshina, Steven W. Barwick, Subir Sarkar, Christian Bohm, Glenn Spiczak, Karen Andeen, P. Steffen, D. Z. Besson, J. Haugen, H. S. Matis, F. Refflinghaus, B. Hughey, David A. Schneider, Yi Wang, Paolo Desiati, E. Blaufuss, Albrecht Karle, K. H. Becker, J. E. Sopher, K. Mase, A. Elcheikh, J. Pretz, J. W. Nam, L. Thollander, G. C. Hill, D. Turcan, Francis Halzen, A. Muratas, L. Demirörs, Claire Pettersen, D. Seckel, S. Grullon, Heiko Geenen, A. R. Fazely, Elisa Bernardini, P. A. Toale, P. Berghaus, T. McCauley, G. W. Sullivan, M. C. Stoufer, S. H. Seo, J.D. Zornoza, H. Landsman, J. Ahrens, G. Kohnen, R. W. Ellsworth, Aya Ishihara, J. M. Joseph, J.N. Bahcall, H. Miyamoto, J. C. Díaz-Vélez, T. Stezelberger, P. Wisniewski, M. Krasberg, M. V. D'Agostino, M. Kestel, M. Ribordy, Jenni Adams, A. Laundrie, S. M. Movit, K. Han, Christian Spiering, M. H. Whitney, D. Hays, Anna Davour, J.-P. Hülß, Ignacio Taboada, T. Messarius, C. Song, Olga Botner, Jay Gallagher, Joseph T. Hodges, W. Wagner, Justin Vandenbroucke, Klas Hultqvist, Peter Mészáros, K. Helbing, D. Hardtke, R. G. Stokstad, P. Herquet, A. Mokhtarani, H. Kawai, Chris Wendt, R. C. Bay, Janet Jacobsen, S. Yoshida, Xinhua Bai, C. T. Day, R. Ehrlich, A. Olivas, N. Kitamura, D. Berley, S. Stoyanov, A. W. Jones, I. Liubarsky, J. Dreyer, T. Castermans, A. Groß, E. A. Strahler, J. Cherwinka, R. M. Gunasingha, A. Silvestri, Ph. Olbrechts, B. Voigt, John Clem, M. Solarz, Christopher Wiebusch, J. E. Hart, Michael Stamatikos, C. Walck, D.W. Atlee, J. A. Goodman, R. Porrata, C.P. Burgess, J. Eisch, D. J. Boersma, J. Baccus, K. Kuehn, W. R. Edwards, C. Mackenzie, P. O. Hulth, Hermann Kolanoski, S. Böser, O. Tarasova, Hakki Ögelman, N. van Eijndhoven, R. Morse, Gerald Przybylski, T. Feser, S. Robbins, J.K. Becker, K.-H. Sulanke, M. Hellwig, H. G. Sander, George Japaridze, Elisa Resconi, S. Hundertmark, James E. Braun, T. Hauschildt, Adam Bouchta, Allan Hallgren, Torsten Harenberg, B. D. Fox, L. Gerhardt, A. Piegsa, A. Rizzo, C. De Clercq, A. Morey, A. Van Overloop, K. Rawlins, Markus Ackermann, K. Münich, M.G. Greene, D. Bertrand, S. Patton, James Madsen, Todor Stanev, Dawn Williams, Soebur Razzaque, Carlos Pena-Garay, T. DeYoung, O. Fadiran, H. Waldmann, Teresa Montaruli, P. Sandstrom, Thomas K. Gaisser, G. B. Yodh, M. Walter, S. Seunarine, D. Rutledge, M. Gurtner, R. Gozzini, M. Bartelt, A. Tepe, R. Nahnhauer, S. Klepser, K. Beattie, P. B. Price, Kurt Woschnagg, Paul Evenson, Dmitry Chirkin, Johan Lundberg, R. Ganugapati, A. C. Pohl, D. F. Cowen, A. Achterberg, Carsten Rott, Dave Nygren, Xianwu Xu, R. Hardtke, H. Wissing, C. Pérez de los Heros, John Heise, T. Becka, G. Wikström, Damian Pieloth, D. Hubert, L. Köpke, H. Leich, A. Meli, Karl-Heinz Kampert, Kirill Filimonov, Spencer Klein, Kara Hoffman, Wolfgang Rhode, J. L. Kelley, S. Schlenstedt, M. R. Duvoort, B. Baret, S. Tilav, P. Nießen, C. P. McParland, and A. Goldschmidt
Subjects: Astroparticle physics, Physics, Photomultiplier, Muon, Performance, Detector, Astrophysics (astro-ph), Astronomy, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, IceCube Neutrino Observatory, Amanda, IceCube, Detection, Data acquisition, First year, IceTop, Neutrino, South pole, Astronomia, Cherenkov radiation
Abstract: The first sensors of the IceCube neutrino observatory were deployed at the South Pole during the austral summer of 2004-2005 and have been producing data since February 2005. One string of 60 sensors buried in the ice and a surface array of eight ice Cherenkov tanks took data until December 2005 when deployment of the next set of strings and tanks began. We have analyzed these data, demonstrating that the performance of the system meets or exceeds design requirements. Times are determined across the whole array to a relative precision of better than 3 ns, allowing reconstruction of muon tracks and light bursts in the ice, of air-showers in the surface array and of events seen in coincidence by surface and deep-ice detectors separated by up to 2.5 km. © 2006 Elsevier B.V. All rights reserved.
Published: 2006

37. Optical properties of deep glacial ice at the South Pole

Author: Christian Spiering, P. Ekström, P. Berghaus, Othmane Bouhali, S. Böser, I. Liubarsky, M. Kestel, Joseph T. Hodges, C. H. Wiebusch, David A. Schneider, P. B. Price, T. Neunhöffer, G. C. Hill, Albrecht Karle, R. Morse, K. Rawlins, D. J. Boersma, Heiko Geenen, Tyce DeYoung, Y. Minaeva, K. Hultqvist, Elisa Bernardini, Kurt Woschnagg, Glenn Spiczak, Matthias Leuthold, D. R. Nygren, C.P. Burgess, M. Hellwig, B. Hughey, T. Messarius, P. Herquet, A. Silvestri, James Madsen, Dmitry Chirkin, H. G. Sander, Kael Hanson, K. Kuehn, Jan Conrad, T. Feser, B. Collin, R. G. Stokstad, L. Gerhardt, R. Wischnewski, M. Solarz, Jodi Cooley, Ignacio Taboada, M. Ribordy, K. Helbing, Olga Botner, Johan Lundberg, O. Tarasova, R. Schwarz, P. Steffen, J. Rodríguez Martino, R. Nahnhauer, T. Burgess, K. H. Sulanke, P. Miocinovic, J. Ahrens, R. Ganugapati, A. C. Pohl, S. Richter, G. Kohnen, Michael Stamatikos, Yi Wang, Paolo Desiati, D. F. Cowen, H. S. Matis, Marek Kowalski, Gerald Przybylski, H. Leich, Francis Halzen, M. Bartelt, S. Schlenstedt, Xinhua Bai, R. Porrata, D. Bertrand, Axel Groß, J. K. Becker, C. De Clercq, T. Hauschildt, Markus Ackermann, M. Walter, S. W. Barwick, Adam Bouchta, C.P. de los Heros, Allan Hallgren, R. Lang, C. Walck, P. O. Hulth, Thomas K. Gaisser, Elisa Resconi, H. Wissing, S. Hundertmark, Torsten Harenberg, Wolfgang Wagner, T. Becka, Pawel Marciniewski, Anna Davour, Janet Jacobsen, D. Steele, Wolfgang Rhode, P. Niessen, T. Castermans, Karl-Heinz Kampert, D. Hubert, L. Köpke, S. Tilav, K.-H. Becker, C. P. McParland, A. Goldschmidt, D. Hardtke, R. C. Bay, Ph. Olbrechts, K. Münich, J. W. Nam, and L. Thollander
Subjects: Atmospheric Science, Soil Science, Mineralogy, Aquatic Science, Oceanography, Light scattering, Physics::Geophysics, Ice core, Geochemistry and Petrology, Earth and Planetary Sciences (miscellaneous), Absorption (electromagnetic radiation), Physics::Atmospheric and Oceanic Physics, Earth-Surface Processes, Water Science and Technology, geography, geography.geographical_feature_category, Ecology, Scattering, Paleontology, Forestry, Glacier, Molar absorptivity, Wavelength, Geophysics, Space and Planetary Science, Attenuation coefficient, Astrophysics::Earth and Planetary Astrophysics, Geology
Abstract: We have remotely mapped optical scattering and absorption in glacial ice at the South Pole for wavelengths between 313 and 560 nm and depths between 1100 and 2350 m. We used pulsed and continuous light sources embedded with the AMANDA neutrino telescope, an array of more than six hundred photomultiplier tubes buried deep in the ice. At depths greater than 1300 m, both the scattering coefficient and absorptivity follow vertical variations in concentration of dust impurities, which are seen in ice cores from other Antarctic sites and which track climatological changes. The scattering coefficient varies by a factor of seven, and absorptivity (for wavelengths less than ∼450 nm) varies by a factor of three in the depth range between 1300 and 2300 m, where four dust peaks due to stadials in the late Pleistocene have been identified. In our absorption data, we also identify a broad peak due to the Last Glacial Maximum around 1300 m. In the scattering data, this peak is partially masked by scattering on residual air bubbles, whose contribution dominates the scattering coefficient in shallower ice but vanishes at ∼1350 m where all bubbles have converted to nonscattering air hydrates. The wavelength dependence of scattering by dust is described by a power law with exponent -0.90 ± 0.03, independent of depth. The wavelength dependence of absorptivity in the studied wavelength range is described by the sum of two components: a power law due to absorption by dust, with exponent -1.08 ± 0.01 and a normalization proportional to dust concentration that varies with depth; and a rising exponential due to intrinsic ice absorption which dominates at wavelengths greater than ∼500 nm. Copyright 2006 by the American Geophysical Union.
Published: 2006

38. Limits to the muon flux from neutralino annihilations in the Sun with the AMANDA detector

Author: K. Rawlins, R. Schwarz, Jodi Cooley, Ignacio Taboada, I. Liubarsky, A. Gross, Othmane Bouhali, Torsten Harenberg, A. C. Pohl, James Madsen, C. H. Wiebusch, T. Becka, P. Ekström, P. Berghaus, Pawel Marciniewski, S. Richter, M. Bartelt, M. Kestel, David A. Schneider, Johan Lundberg, G. C. Hill, Anna Davour, T. DeYoung, Xinhua Bai, K. Kuehn, S. Schlenstedt, Heiko Geenen, O. Tarasova, R. Morse, Karl-Heinz Kampert, C. P. McParland, Matthias Leuthold, D. J. Boersma, H. S. Matis, Glenn Spiczak, Janet Jacobsen, D. R. Nygren, R. Ganugapati, Francis Halzen, H. Leich, R. Porrata, A. Silvestri, K. Hultqvist, D. F. Cowen, D. Hubert, S. Hundertmark, P. Herquet, A. Goldschmidt, Marek Kowalski, P. B. Price, J. K. Becker, Ph. Olbrechts, Hakki Ögelman, L. Köpke, C. De Clercq, D. Steele, K. Hanson, B. Hughey, M. Ribordy, K. Helbing, K. Münich, Jan Conrad, T. Feser, L. Gerhardt, Kurt Woschnagg, K.-H. Becker, P. Steffen, Christian Spiering, S. Robbins, Markus Ackermann, S. W. Barwick, J. Rodríguez Martino, Wolfgang Rhode, P. Miocinovic, T. Hauschildt, S. Böser, Dmitry Chirkin, Joseph T. Hodges, Wolfgang Wagner, M. Hellwig, M. Walter, H. G. Sander, Elisa Bernardini, Y. Minaeva, M. V. D'Agostino, R. Nahnhauer, R. Lang, C. Walck, P. O. Hulth, Yi Wang, B. Collin, Adam Bouchta, C.P. de los Heros, Paolo Desiati, Thomas K. Gaisser, J. Ahrens, J. W. Nam, Allan Hallgren, L. Thollander, H. Wissing, P. Niessen, T. Messarius, C.P. Burgess, D. Hardtke, R. C. Bay, K. H. Sulanke, Elisa Resconi, T. Castermans, S. Tilav, Michael Stamatikos, T. Neunhöffer, Albrecht Karle, T. Burgess, D. Bertrand, R. G. Stokstad, R. Wischnewski, G. Kohnen, Gerald Przybylski, M. Solarz, and Olga Botner
Subjects: Astroparticle physics, Physics, Particle physics, Range (particle radiation), AMANDA, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Detector, Dark matter, High Energy Physics::Phenomenology, Astrophysics (astro-ph), Neutralino, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Neutrino telescopes, Nuclear physics, Neutrino detector, Muon flux, High Energy Physics::Experiment
Abstract: A search for an excess of muon-neutrinos from neutralino annihilations in the Sun has been performed with the AMANDA-II neutrino detector using data collected in 143.7 days of live-time in 2001. No excess over the expected atmospheric neutrino background has been observed. An upper limit at 90% confidence level has been obtained on the annihilation rate of captured neutralinos in the Sun, as well as the corresponding muon flux limit at the Earth, both as functions of the neutralino mass in the range 100 GeV-5000 GeV., Comment: 13 pages, 3 figures. Submitted to Astropart. Phys
Published: 2006

39. Flux limits on ultra high energy neutrinos with AMANDA-B10

Author: Kael Hanson, M. Ribordy, M. Hellwig, K. Helbing, David A. Schneider, G. C. Hill, Torsten Harenberg, Heiko Geenen, Ph. Olbrechts, P. Steffen, J. Rodríguez Martino, H. G. Sander, P. Ekström, K. Münich, Yi Wang, R. G. Stokstad, Paolo Desiati, H. S. Matis, B. Collin, J. Ahrens, R. Wischnewski, Johan Lundberg, M. Kestel, A. C. Pohl, Pawel Marciniewski, M. Solarz, T. DeYoung, J. K. Becker, R. Ganugapati, R. Nahnhauer, C.P. Burgess, Michael Stamatikos, S. Böser, S. Schlenstedt, Francis Halzen, D. Rutledge, D. F. Cowen, M. Bartelt, Marek Kowalski, H. Leich, J. W. Nam, T. Hauschildt, R. Schwarz, Anna Davour, L. Thollander, P. B. Price, T. Burgess, Adam Bouchta, A. Silvestri, Xinhua Bai, K. Rawlins, James Madsen, Axel Groß, C. H. Wiebusch, Allan Hallgren, M. Krasberg, K. H. Sulanke, J. L. Kelley, D.W. Atlee, R. Porrata, Kurt Woschnagg, Kyle T. Mandli, Janet Jacobsen, L. Gerhardt, D. Hardtke, R. C. Bay, Glenn Spiczak, Hakki Ögelman, T. Neunhöffer, Albrecht Karle, B. Hughey, S. Hundertmark, D. J. Boersma, Elisa Bernardini, Elisa Resconi, Olga Botner, R. Morse, Dmitry Chirkin, K. Hultqvist, L. C. Voicu, J. Hodges, Wolfgang Wagner, T. Messarius, K. Kuehn, K. Schinarakis, P. O. Hulth, Jodi Cooley, H. Wissing, S. Richter, James E. Braun, C. De Clercq, S. M. Movit, Markus Ackermann, S. W. Barwick, Gerald Przybylski, C. Walck, Christian Spiering, Thomas K. Gaisser, G. B. Yodh, P. Miocinovic, M. Walter, K.-H. Becker, H. Albrecht, O. Tarasova, Y. Minaeva, S. Tilav, Matthias Leuthold, D. R. Nygren, P. Herquet, Wolfgang Rhode, C. P. McParland, Jan Conrad, A. Goldschmidt, T. Feser, D. Bertrand, D. Hubert, L. Köpke, C. Pérez de los Heros, T. Becka, T. Coarasa, Karl-Heinz Kampert, D. Steele, P. Niessen, I. Taboada, T. Castermans, R. Hardtke, and Othmane Bouhali
Subjects: Physics, Particle physics, AMANDA, Muon, Physics::Instrumentation and Detectors, UHE neutrinos, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, High Energy Physics::Phenomenology, Flux, Astronomy and Astrophysics, Solar neutrino problem, Neutrino astronomy, Neutrino telescopes, Neutrino detector, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino
Abstract: Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 10 16 eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following E −2 , with an equal mix of all flavors, is limited to E 2 Φ (10 15 eV E 18 eV) ⩽ 0.99 × 10 −6 GeV cm −2 s −1 sr −1 at 90% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bounds to specific extraterrestrial neutrino flux predictions are also presented.
Published: 2005

40. Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

Author: K. Rawlins, James Madsen, H. Leich, David A. Schneider, D. J. Boersma, G. C. Hill, Heiko Geenen, J. P Dewulf, Olga Botner, Othmane Bouhali, Y. Minaeva, J.K. Becker, Glenn Spiczak, P. Miocinovic, Philip Olbrechts, T. Messarius, Christopher Wiebusch, Hakki Ögelman, Matthias Leuthold, D. R. Nygren, C. Walck, R. Ganugapati, P. Steffen, Thomas K. Gaisser, G. B. Yodh, B. Hughey, Jan Conrad, T. Feser, M. Ribordy, D. F. Cowen, I. Liubarsky, Marek Kowalski, Xinhua Bai, Gerald Przybylski, K. H. Sulanke, P. B. Price, T. O. B. Schmidt, Kurt Woschnagg, T. Hauschildt, K. Munich, I. Taboada, Dmitry Chirkin, A. Groß, C. P. McParland, Adam Bouchta, Allan Hallgren, S. Hundertmark, L. Gerhardt, A. Goldschmidt, D. Bertrand, A. Chen, R. Hardtke, C. Pérez de los Heros, T. Becka, Wolfgang Rhode, Elisa Resconi, Torsten Harenberg, Julie Lamoureux, D. Steele, P. Niessen, Wolfgang Wagner, D. Hubert, L. Köpke, Yajun Wang, S. Schlenstedt, Freddy Binon, T. Burgess, A. C. Pohl, C. Wiedemann, Pawel Marciniewski, Ph. Herquet, Kael Hanson, Paolo Desiati, R. Nahnhauer, P. Ekström, T. Neunhöffer, M. Kestel, T. DeYoung, M. Hellwig, Staffan Carius, H. G. Sander, Albrecht Karle, Anna Davour, R. Porrata, B. Collin, Janet Jacobsen, P. O. Hulth, S. Böser, H. Wissing, S. Tilav, R. Schwarz, Kyle T. Mandli, R. Morse, A. Silvestri, H. S. Matis, Michael Stamatikos, A. Biron, L. Thollander, Francis Halzen, K. Helbing, J. Rodríguez Martino, Jodi Cooley, K. Hultqvist, S. Richter, R. G. Stokstad, J. Ahrens, R. Wischnewski, P. Lindahl, Christian Spiering, K. Kuehn, K. Schinarakis, T. Castermans, C. De Clercq, S. W. Barwick, M. Gaug, Elisa Bernardini, and M. Solarz
Subjects: AMANDA, cosmic radiation [neutrino], Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, particle source [cosmic radiation], General Physics and Astronomy, FOS: Physical sciences, Astrophysics, magnetic [matter], numerical methods, ddc:550, quasar, Blazar, Astroparticle physics, Physics, photomultiplier, cosmic radiation [muon], water [Cherenkov counter], Astrophysics (astro-ph), Astronomy, Solar neutrino problem, Cosmic neutrino background, Neutrino detector, Measurements of neutrino speed, High Energy Physics::Experiment, flux [cosmic radiation], blazar [AGN], data management, Neutrino, upper limit, experimental results
Abstract: We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal., Comment: 5 pages, 5 figures, 1 table, submitted to PRL
Published: 2004

41. Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos

Author: George Japaridze, I. Taboada, P. Miocinovic, M. Hellwig, R Koch, R. M. Gunasingha, H. G. Sander, R. Paulos, R. C. Bay, Michael Stamatikos, R. Ganugapati, T. Neunhöffer, Albrecht Karle, B. Collin, D. F. Cowen, Marek Kowalski, Christian Spiering, J. A. Goodman, K. Rawlins, K. Schinarakis, C. Pérez de los Heros, T. Becka, P. Niessen, P. B. Price, T. O. B. Schmidt, I. Liubarsky, James Madsen, Soebur Razzaque, K. Helbing, T. Castermans, Jodi Cooley, A. Biron, Elisa Resconi, N. Kitamura, D. Hubert, Kurt Woschnagg, Peter Mészáros, Paul Evenson, S. Schlenstedt, M. Kestel, R. G. Stokstad, C. H. Wiebusch, S. Hundertmark, S. Tilav, K. H. Sulanke, C. De Clercq, R. Wischnewski, A. J. Smith, Dmitry Chirkin, C. Wiedemann, T. DeYoung, Jean Gallagher, J. I. Lamoureux, G. W. Sullivan, A. C. Pohl, S. Richter, Xinhua Bai, Ph. Herquet, L. Köpke, T. Burgess, D. Z. Besson, R. Morse, R. Schwarz, E. Blaufuss, D. J. Boersma, J. Ahrens, D. Bertrand, K.-H. Becker, D. Steele, K. Hultqvist, J. Cavin, R. H. Minor, Kael Hanson, William Carithers, T. J. Sumner, H. S. Matis, Elisa Bernardini, S. Patton, Ph. Olbrechts, T. Stezelberger, Paolo Desiati, Francis Halzen, R. W. Ellsworth, Wolfgang Rhode, Hakki Ögelman, H. Kawai, H. Leich, S. Böser, C. P. McParland, Olga Botner, R. Hardtke, M. Solarz, A. Goldschmidt, R. Nahnhauer, M. Ribordy, T. Messarius, S. Yoshida, D. Hays, W. Chinowsky, N. van Eijndhoven, Glenn Spiczak, B. Hughey, Gerald Przybylski, R. Ehrlich, T. Hauschildt, Adam Bouchta, R.-R Wang, Allan Hallgren, Wolfgang Wagner, P. O. Hulth, H. Wissing, D. Seckel, Anna Davour, Janet Jacobsen, Todor Stanev, H. Miyamoto, C. Walck, Thomas K. Gaisser, J. Pretz, Y. Minaeva, A. W. Jones, John N. Bahcall, Matthias Leuthold, Othmane Bouhali, D. R. Nygren, P. Steffen, Jan Conrad, T. Feser, Christian Bohm, David A. Schneider, D. Berley, G. C. Hill, Heiko Geenen, and A. R. Fazely
Subjects: Physics, Active galactic nucleus, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics (astro-ph), Gamma ray, FOS: Physical sciences, IceCube, Neutrino astronomy, Neutrino telescope, Astronomy and Astrophysics, Cosmic ray, Astrophysics, High Energy Physics::Experiment, Neutrino, Gamma-ray burst
Abstract: We present the results of a Monte-Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the detector's capability to search for muon neutrinos from sources such as active galaxies and gamma-ray bursts. We study the effective area and the angular resolution of the detector as a function of muon energy and angle of incidence. We present detailed calculations of the sensitivity of the detector to both diffuse and pointlike neutrino emissions, including an assessment of the sensitivity to neutrinos detected in coincidence with gamma-ray burst observations. After three years of datataking, IceCube will have been able to detect a point source flux of E^2*dN/dE = 7*10^-9 cm^-2s^-1GeV at a 5-sigma significance, or, in the absence of a signal, place a 90% c.l. limit at a level E^2*dN/dE = 2*10^-9 cm^-2s^-1GeV. A diffuse E-2 flux would be detectable at a minimum strength of E^2*dN/dE = 1*10^-8 cm^-2s^-1sr^-1GeV. A gamma-ray burst model following the formulation of Waxman and Bahcall would result in a 5-sigma effect after the observation of 200 bursts in coincidence with satellite observations of the gamma-rays., Comment: 33 pages, 13 figures, 6 tables
Published: 2004

42. Search for Neutrino-Induced Cascades with AMANDA

Author: Christian Spiering, D. J. Boersma, I. Liubarsky, A. Groß, Wolfgang Rhode, T. Hauschildt, M. Solarz, Jodi Cooley, R. Ganugapati, T. Burgess, C. H. Wiebusch, K. Rawlins, P. Ekström, Karl-Heinz Kampert, D. F. Cowen, Marek Kowalski, Adam Bouchta, D. Bertrand, P. B. Price, C.P. Burgess, M. Walter, D. Hubert, T. Neunhöffer, Kael Hanson, Othmane Bouhali, T. O. B. Schmidt, J. L. Kelley, Allan Hallgren, L. Köpke, M. Kestel, Albrecht Karle, Wolfgang Wagner, S. Hundertmark, Kurt Woschnagg, J. W. Nam, L. Thollander, S. Böser, T. DeYoung, R. Morse, James Madsen, Torsten Harenberg, Dmitry Chirkin, S. Richter, J. Hodges, K. H. Sulanke, K. Hultqvist, James E. Braun, R. Nahnhauer, A. Silvestri, J.K. Becker, P. O. Hulth, H. S. Matis, David A. Schneider, R. Porrata, Gerald Przybylski, M. Ribordy, K. Helbing, R. C. Bay, Francis Halzen, G. C. Hill, Matthias Leuthold, D. R. Nygren, H. Wissing, J. Rodríguez Martino, Glenn Spiczak, P. Herquet, Paolo Desiati, L. Gerhardt, A. C. Pohl, Heiko Geenen, Hakki Ögelman, P. Steffen, B. Hughey, J. Ahrens, Pawel Marciniewski, Olga Botner, Ph. Olbrechts, Elisa Resconi, Kyle T. Mandli, T. Messarius, Jan Conrad, T. Feser, Anna Davour, M. Hellwig, H. G. Sander, M. Krasberg, R. Schwarz, Janet Jacobsen, P. Miocinovic, Y. Minaeva, K. Kuehn, B. Collin, K. Schinarakis, M. Bartelt, H. Leich, Xinhua Bai, Yajun Wang, K. Munich, S. Schlenstedt, C. De Clercq, S. Tilav, Markus Ackermann, S. W. Barwick, R. Hardtke, R. G. Stokstad, R. Wischnewski, P. Niessen, K.-H. Becker, C. Walck, I. Taboada, Thomas K. Gaisser, G. B. Yodh, T. Castermans, C. Pérez de los Heros, T. Becka, Michael Stamatikos, H. Albrecht, D. Steele, Elisa Bernardini, C. P. McParland, and A. Goldschmidt
Subjects: Physics, AMANDA, Particle physics, Muon, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, Hadron, High Energy Physics::Phenomenology, Astrophysics (astro-ph), Flux, FOS: Physical sciences, Astronomy and Astrophysics, Electron, Astrophysics, Neutrino astronomy, Neutrino telescopes, High Energy Physics::Experiment, Neutrino, Event (particle physics)
Abstract: We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high energy neutrinos in the data collected with the AMANDA II detector during the year 2000. The observed event rates are consistent with the expectations for atmospheric neutrinos and muons. We place upper limits on a diffuse flux of extraterrestrial electron, tau and muon neutrinos. A flux of neutrinos with a spectrum $\Phi \propto E^{-2}$ which consists of an equal mix of all flavors, is limited to $E^2 \Phi(E)=8.6 x 10^{-7} GeV/(cm^{2} s sr)$ at a 90% confidence level for a neutrino energy range 50 TeV to 5 PeV. We present bounds for specific extraterrestrial neutrino flux predictions. Several of these models are ruled out., Comment: 18 pages, 12 figures
Published: 2004
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43. Physics and Operation of the AMANDA-II High Energy Neutrino Telescope

Author: S. W. Barwick, J. Ahrens, X. Bai, T. Becka, K.-H. Becker, D. Bertrand, F. Binon, A. Biron, S. Boser, O. Botner, O. Bouhali, T. Burgess, S. Carius, T. Castermans, D. Chirkin, J. Conrad, J. A. Cooley, D. F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, J.-P. Dewulf, P. Doksus, P. Ekstrom, T. Feser, T. K. Gaisser, M. Gaug, L. Gerhardt, A. Goldschmidt, A. Hallgren, Francis Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, P. Herquet, G. C. Hill, P. O. Hulth, K. Hultqvist, J. Hundertmark, Janet Jacobsen, A. Karle, L. Kopke, M. Kowalski, Kyler W. Kuehn, J. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, J. Madsen, P. Marciniewski, Howard S. Matis, C. P. McParland, Y. Minaeva, P. Miocinovic, R. Morse, R. Nahnhauer, T. Neunh÷ffer, P. Niessen, David R. Nygren, Hakki Ogelman, Ph. Olbrechts, C. Prez de los Heros, A. C. Pohl, P. B. Price, G. T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodrguez Martino, D. Ross, H. G. Sander, T. Schmidt, D. Schneider, R. Schwarz, A. Silvestri, M. Solarz, G. M. Spiczak, C. Spiering, D. Steele, P. Steffen, R. G. Stokstad, P. Sudhoff, K. H. Sulanke, I. Taboada, L. Thollander, S. Tilav, C. Walck, C. Weinheimer, C. H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, Gaurang B. Yodh, and S. Young
Subjects: Physics, Muon, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), FOS: Physical sciences, Flux, Astrophysics, Generic point, law.invention, Telescope, Data acquisition, law, Angular resolution, Neutrino, Gamma-ray burst
Abstract: This paper briefly describes the principle of operation and science goals of the AMANDA high energy neutrino telescope located at the South Pole, Antarctica. Results from an earlier phase of the telescope, called AMANDA-B10, demonstrate both reliable operation and the broad astrophysical reach of this device, which includes searches for a variety of sources of ultrahigh energy neutrinos: generic point sources, Gamma-Ray Bursts and diffuse sources. The predicted sensitivity and angular resolution of the telescope were confirmed by studies of atmospheric muon and neutrino backgrounds. We also report on the status of the analysis from AMANDA-II, a larger version with far greater capabilities. At this stage of analysis, details of the ice properties and other systematic uncertainties of the AMANDA-II telescope are under study, but we have made progress toward critical science objectives. In particular, we present the first preliminary flux limits from AMANDA-II on the search for continuous emission from astrophysical point sources, and report on the search for correlated neutrino emission from Gamma Ray Bursts detected by BATSE before decommissioning in May 2000. During the next two years, we expect to exploit the full potential of AMANDA-II with the installation of a new data acquisition system that records full waveforms from the in-ice optical sensors., 14 pages, 14 figures, Slightly updated from manuscript submitted to SPIE Conference (Hawaii, 2002). Sky plot and preliminary limits given for point sources using AMANDA-II. First report on GRB search using AMANDA-II. Updated acknowledgements, references and table entries
Published: 2003

44. Hardware controls for the STAR experiment at RHIC

Author: M. Bordua, J. Gross, J. Chrin, C. P. McParland, M. A. Howe, C. Lianberger, I. Sakrejda, M. Cherney, T. S. McShane, S. Jacobson, V. Ghazikhanian, P. Kravtsov, I. Ferguson, F. Bieser, G. Harper, W. Zhang, E. Yamamoto, J. Meier, and J. Lin
Subjects: Nuclear and High Energy Physics, Engineering, business.industry, Client server systems, Field bus, Industrial control system, Star (graph theory), Particle detector, Data link, Nuclear Energy and Engineering, Control system, Baseline system, Electrical and Electronic Engineering, business, Computer hardware
Abstract: A hardware controls system has been implemented for the STAR experiment at RHIC. Approximately 10000 parameters governing experiment operation are currently controlled and monitored. The system is based on the Experimental Physics and Industrial Control System (EPICS). The architecture of STAR hardware controls are presented as well as the results of operation of the integrated baseline system. Novel features of the system include a specialized field bus (High-level Data Link Control-HDLC), new EPICS record support, control DEVice (CDEV) interfaces to accelerator and magnet control systems, and C++ based communication between STAR online and hardware controls and their associated databases.
Published: 2003

45. Star detector overview

Author: L. V. Nogach, A. Stolpovsky, H. Hümmler, L. Kotchenda, P. Seyboth, T. Krupien, D. Dayton, V. A. Nikitin, C.J. Liaw, J.F. Amsbaugh, M. Castro, K. E. Shestermanov, A. R. Baldwin, M. Calderon De La Barca Sanchez, Matthew Nguyen, T. Dietel, D.E. Greiner, A. Lebedev, J. Schambach, C. P. McParland, J. Gross, S. Pirogov, R. Seymour, S. Bennett, F. Liu, L. Lakehal-Ayat, D. Zimmerman, A. Ridiger, W. Christie, R. L. Brown, Q. Li, C. Gojak, A. Hirsch, C. P. Lansdell, I.A. Savin, N. T. Porile, A. Tarchini, Alexandre Alarcon Do Passo Suaide, S. Heppelmann, D. Flierl, V. Perevoztchikov, L. Martin, Vladimir Petrov, B. Miller, M. Dialinas, D. Russ, Yu Chen, N. G. Minaev, Jinghui Yang, S. P. Chernenko, Granville Ott, R. V. Cadman, J. E. Draper, Frank Jm Geurts, Lianshou Liu, C. O. Blyth, H. Diaz, Yu A. Matulenko, W. J. Llope, M. Horsley, T. Nguyen, A. Cardenas, Sergey Voloshin, G. LoCurto, H. G. Ritter, G. Van Buren, Sergey Panitkin, B. Stringfellow, J. Sedlmeir, N. Schmitz, B. Lasiuk, H. Long, K. J. Foley, Wen-Chang Chen, S. R. Klein, H. Fessler, P. Jensen, R. K. Kutuev, M. A. Howe, K. Krueger, C. Struck, W. Deng, J. P. Coffin, D. Shuman, R. Willson, O. Barannikova, D. L. Olson, J. G. Cramer, B. Choi, O. V. Rogachevski, E. Shahaliev, C. Consiglio, L. Smykov, J. Takahashi, J. W. Watson, B. Norman, J. Wirth, R. Bossingham, W. Hunt, Damien Bonnet, J. R. Hall, M. Kopytine, Thomas LeCompte, Gary Westfall, B. D. Anderson, R. Weidenbach, C. E. Allgower, J. M. Nelson, J. Rasson, H. Stroebele, G. C. Harper, D. Reichhold, Q. J. Liu, V. S. Shvetcov, C. A. Whitten, S. Tonse, E. Sugarbaker, B. E. Bonner, Torre Wenaus, Alexander Kovalenko, V. Trofimov, M. Gazdzicki, J. Baudot, E. Platner, T. Ljubicic, Thomas A. Trainor, W. R. Edwards, G. Guilloux, A. I. Kulikov, T. J. Hallman, T. J. M. Symons, Chinh Vu, A. A. Derevschikov, M. Cherney, W. Peryt, P. Kravtsov, C. Adler, O. D. Tsai, P. G. Jones, J. Seger, M. Kramer, J. Engelage, E. Yamamoto, Y. V. Zanevski, S. Lange, I. Zborovský, Thomas Michael Cormier, F. Meissner, D. G. Underwood, Jeffrey G. Reid, S. J. Lindenbaum, I. Polk, S. Bouvier, J. T.M. Chrin, Matthew J. Anderson, Derek L. G. Hill, V. Lindenstruth, Masashi Kaneta, R. P. Scharenberg, John N. Wood, J. H. Thomas, L. Conin, G. Visser, W. M. Zhang, A. Yokosawa, J. Berger, Andrey Vasiliev, G. Eppley, P. Nevski, E. Mogavero, A. H. Tang, J. Marx, J. Sowinski, A. E. Yakutin, M. Burkes, J. W. Harris, D. Padrazo, S. Jacobson, M. I. Ferguson, D. Seliverstov, A. Schüttauf, T. S. McShane, I. Vakula, Malgorzata Anna Janik, H. S. Matis, A. N. Zubarev, C. A. Ogilvie, Z. Liu, M. Beddo, David Fritz, Mikhail Tokarev, J. Wolf, P. A. DeYoung, J. Pluta, J. Meier, I. Flores, M. Messer, A. C. Saulys, Subhasis Chattopadhyay, Nu Xu, J. M. Landgraf, Peter Martin Jacobs, K. Turner, A. V. Brandin, D. Roehrich, B. Erazmus, J. Grabski, P. Fachini, J. Tarzian, G. Koehler, M. Botlo, D. Lynn, H. M. Spinka, E. Gushin, G. J. Kunde, P. Yepes, V. Eckardt, Ma Bloomer, R. Lednicky, H. Caines, Y. Fisyak, A. Ogawa, Ian Johnson, J. Riso, R. Renfordt, Christina Markert, F. Laue, A. Szanto de Toledo, Sevil Salur, N. Bouillo, Z. Milosevich, R. E. Tribble, W. A. Love, A. Vanyashin, G. S. Averichev, S. E. Vigdor, Christian Claude Kuhn, Y. Panebratsev, F. Retiere, V. V. Belaga, H. Ward, S. B. Nurushev, G. S. Mutchler, J. Sandweiss, A. Klyachko, K. Solberg, T. Pawlak, Adam Ryszard Kisiel, Gerald W Hoffmann, D. Grosnick, N.D. Gagunashvili, C. Drancourt, J. Puskar-Pasewicz, G. Rai, J. Lin, P. Sorensen, H. Wieman, J. Porter, K. Bradley, S. U. Pandey, M. Germain, G. Brugalette, A. I. Pavlinov, L. G. Efimov, M. B. Tonjes, Richard C. Jared, Salahuddin Ahmad, E. G. Judd, F. S. Bieser, M. Schulz, K. Schweda, D. Cebra, S. Trentalange, Michael A. Thompson, V. Morozov, I. Sakrejda, B. Minor, T. Ullrich, A. Tai, L. Didenko, A. Khodinov, R. Maier, J. Amonett, Yu Melnick, Morton Kaplan, J. Klay, M. DeMello, D. Hardtke, M. Oldenburg, R. D. Majka, M. M. de Moura, M. L. Miller, V. Emelianov, D. Keane, Michal Sumbera, H. Z. Huang, Nikolai Smirnov, N. Stone, R. Stock, R. Bellwied, J. Mitchell, P. Szarwas, A. S. Konstantinov, William Jacobs, K. H. Ackermann, Yu. Ivanshin, K. Filimonov, L. C. Bland, H. Bichsel, Hank Crawford, C. Suire, D. M. Moltz, R. S. Longacre, P. Middlekamp, A. A. Kuznetsov, V. M. Leontiev, Olivier Ravel, A. Etkin, J. Whitfield, V. Faine, L. Arnold, G. Skoro, M. Heffner, J. Castillo, S. W. Wissink, R. Sanchez, J. Dioguardi, V. A. Moiseenko, Marcelo Gameiro Munhoz, D. J. Prindle, H. Zhang, J. Hunter, E. J. Stephenson, M. A. Lisa, B. Srivastava, M. Lopez-Noriega, W. Betts, Lee Stuart Barnby, Z. Sandler, Ivan Kotov, M. A.C. Lamont, T. Noggle, G. Igo, G. Odyniec, C. A. Gagliardi, J. Bercovitz, T. Herston, J. Scheblien, A. P. Meschanin, T. Nussbaum, Daniel Ferenc, Fuqiang Wang, Joakim Nystrand, R. A. Scheetz, V. I. Yurevich, J. Boehm, C. Roy, F. P. Brady, T. Eggert, E. Hjort, Thomas Humanic, P. Kuczewski, K. Olchanski, J. Wisdom, J. Carroll, Vladimir Tikhomirov, S. Margetis, R. Wells, C. Feliciano, L. Greiner, A. Ishihara, Ross Schlueter, D. DiMassimo, E. Anderssen, V. A. Okorokov, M. Guedon, A. M. VanderMolen, V. Ghazikhanian, Guy Paic, A. Chikanian, S. S. Shimanskii, A. Boucham, Zhongbin Xu, V. B. Dunin, W. J. Leonhardt, S. Bekele, Peter J. Lindstrom, E. Finch, R. Witt, J. Fu, I. M. Vasilevski, Lincoln D. Carr, J. Gans, Boris Hippolyte, J. C. Dunlop, Zubayer Ahammed, M. J. LeVine, L. S. Schroeder, S. V. Razin, M. Strikhanov, L. Gaudichet, J. L. Romero, K. Wilson, J. Kiryluk, W. Pinganaud, Jay Roberts, N. Adams, C. L. Kunz, C. F. Moore, V. Grigoriev, R. L. Ray, E. Potrebenikova, V. L. Rykov, Raimond Snellings, J. Balewski, Claude Andre Pruneau, H. Arnesen, R. Zoulkarneev, A. M. Poskanzer, D. D. Weerasundara, Mingshui Chen, M. Grau, I. Danilov, O. A. Grachov, Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), STAR, and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes)
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Elliptic flow, Star (graph theory), [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, Particle detector, Nuclear physics, Electromagnetic calorimeter, relativistic heavy ions, tracking detectors, electromagnetic calorimeters, gas detectors, silicon detectors, plus au collisions, root-s(nn)=130 gev, au+au collisions, elliptic flow, tpc, 0103 physical sciences, Quark–gluon plasma, Measuring instrument, Astrophysics::Solar and Stellar Astrophysics, High Energy Physics::Experiment, Astrophysics::Earth and Planetary Astrophysics, 010306 general physics, Instrumentation, Astrophysics::Galaxy Astrophysics, STAR detector
Published: 2003

46. Multifragmentation and the phase transition: A systematic study of the multifragmentation of1AGeVAu, La, and Kr

Author: M. A. McMahan, Wolfgang Müller, T. Wienold, D. Keane, Z. Caccia, F. S. Bieser, K.L. Wolf, Sebastiano Albergo, A. D. Chacon, J. Romanski, F. P. Brady, J. L. Romero, M. A. Lisa, A. Scott, G. Rai, Salvatore Costa, H. H. Wieman, G.V. Russo, H. G. Ritter, Cristina Tuve, V. Lindenstruth, R. P. Scharenberg, M. L. Tincknell, N. T. Porile, H. S. Matis, J. C. Kintner, T. J. M. Symons, Y. Choi, J. A. Hauger, Y. Shao, M. L. Gilkes, A. Insolia, C. P. McParland, B. K. Srivastava, J. L. Chance, D. Cebra, S. Wang, M. D. Partlan, P. Warren, E. L. Hjort, A. S. Hirsch, H. Sann, J. O. Rasmussen, Renato Potenza, J. B. Elliott, M. Justice, and D. L. Olson
Subjects: Physics, Nuclear reaction, Nuclear physics, Nuclear and High Energy Physics, Phase transition, Critical point (thermodynamics), Critical phenomena, Coulomb, Multiplicity (mathematics), Atomic physics, Nuclear Experiment, Nuclear matter, Critical exponent
Abstract: A systematic analysis of the multifragmentation (MF) in fully reconstructed events from 1A GeV Au, La and Kr collisions with C has been performed. This data is used to provide a definitive test of the variable volume version of the statistical multifragmentation model (SMM). A single set of SMM parameters directly determined by the data and the semi-empiricalmass formula are used after the adjustable inverse level density parameter, $\epsilon_{o}$ is determined by the fragment distributions. The results from SMM for second stage multiplicity, size of the biggest fragment and the intermediate mass fragments are in excellent agreement with the data. Multifragmentation thresholds have been obtained for all three systems using SMM prior to secondary decay. The data indicate that both thermal excitation energy $E_{th}^{*}$ and the isotope ratio temperature $T_{He-DT}$ decrease with increase in system size at the critical point. The breakup temperature obtained from SMM also shows the same trend as seen in the data. The SMM model is used to study the nature of the MF phase transition. The caloric curve for Kr exhibits back-bending (finite latent heat) while the caloric curves for Au and La are consistent with a continuous phase transition (nearly zero latent heat) and the values of the critical exponents $\tau$, $\beta$ and $\gamma$, both from data and SMM, are close to those for a 'liquid-gas' system for Au and La. We conclude that the larger Coulomb expansion energy in Au and La reduces the latent heat required for MF and changes the nature of the phase transition. Thus the Coulomb energy plays a major role in nuclear MF.
Published: 2002

47. Cnstructing the phase diagram of finite neutral nuclear matter

Author: Luciano G. Moretto, R. P. Scharenberg, Salvatore Costa, H. Sann, F. S. Bieser, H. S. Matis, James B. Elliott, Wolfgang Müller, K.L. Wolf, H. G. Ritter, Cristina Tuve, J. A. Hauger, P. Warren, M. Justice, Y. Choi, Renato Potenza, C. P. McParland, E. L. Hjort, G.V. Russo, J. O. Rasmussen, Z. Caccia, J. L. Chance, V. Lindenstruth, M. L. Tincknell, M. D. Partlan, D. Cebra, Antonio Insolia, A. S. Hirsch, N. T. Porile, M. A. McMahan, F. P. Brady, J. Romanski, G. J. Wozniak, M. L. Gilkes, A. Scott, T. J. M. Symons, G. Rai, M. A. Lisa, Sebastiano Albergo, T. Wienold, D. L. Olson, B. K. Srivastava, J. L. Romero, A. D. Chacon, L. W. Phair, Y. Shao, D. Keane, H. H. Wieman, S. Wang, and J. C. Kintner
Subjects: Physics, Nuclear and High Energy Physics, Quantum mechanics, small percolation lattices, fishers droplet model, critical exponents, critical-behavior, hot nuclei, multifragmentation, transition, liquid, reducibility, energy, Nuclear Theory, FOS: Physical sciences, Nuclear Experiment (nucl-ex), Nuclear Experiment, Humanities
Abstract: The fragment yields from the multifragmentation of gold, lanthanum and krypton nuclei obtained by the EOS Collaboration are examined in terms of Fisher's droplet formalism modifed to account for Coulomb energy. The critical exponents sigma and tau and the surface energy coefficient c0 are obtained. Estimates are made of the pressure-temperature and temperature-density coexistence curves of finite neutral nuclear matter as well as the location of the critical point., Comment: 14 pages, 13 figures, 6 tables, submitted to Phys. Rev. C
Published: 2002
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48. The coexistence curve of finite charged nuclear matter

Author: C. P. McParland, D. L. Olson, M. A. McMahan, Z. Caccia, M. D. Partlan, S. Wang, R. Potenza, Ralph G. Korteling, J. Romanski, H. Breuer, M. L. Tincknell, H. H. Wieman, H. Sann, N. T. Porile, B. K. Srivastava, R. P. Scharenberg, M. L. Gilkes, D. Keane, A. Ruangma, T. J. M. Symons, Sherry Yennello, Wolfgang Müller, G. V. Russo, H. S. Matis, G. J. Wozniak, Y. Shao, C. Tuve, J. O. Rasmussen, Kris Kwiatkowski, J. L. Chance, D. Cebra, E. Hjort, J. B. Elliott, V. Lindenstruth, Luc Beaulieu, P. Warren, V. E. Viola, M. Justice, J. L. Romero, F. S. Bieser, K.L. Wolf, A. Scott, S. Costa, Y. Choi, M. A. Lisa, T. Lefort, F. P. Brady, G. Rai, J. C. Kintner, A. Insolia, L. Phair, T. Wienold, A. D. Chacon, J. A. Hauger, A. S. Hirsch, L. Pienkowski, H. G. Ritter, L. G. Moretto, and S. Albergo
Subjects: Binodal, Physics, Nuclear physics, Tricritical point, Electric potential energy, Nuclear Theory, Nuclear drip line, Nuclear Experiment, Nuclear matter, Critical exponent, Effective nuclear charge, Critical point (mathematics)
Abstract: The multifragmentation data of the ISiS Collaboration and the EOS Collaboration are examined. Fisher's droplet formalism, modified to account for Coulomb energy, is used to determine the critical exponents {tau} and {sigma}, the surface energy coefficient c{sub 0}, the pressure-temperature-density coexistence curve of finite nuclear matter and the location of the critical point.
Published: 2002

49. Comparison of1AGeV197Au+Cdata with thermodynamics: The nature of the phase transition in nuclear multifragmentation

Author: M. A. McMahan, A. Scott, J. O. Rasmussen, H. G. Ritter, A. Insolia, D. L. Olson, H. Sann, P. Warren, D. Keane, G.V. Russo, M. L. Gilkes, T. Wienold, H. H. Wieman, G. Rai, J. L. Chance, Salvatore Costa, J. A. Hauger, E. L. Hjort, D. Cebra, T. J. M. Symons, Renato Potenza, M. Justice, J. B. Elliott, A. D. Chacon, M. A. Lisa, B. K. Srivastava, A. S. Hirsch, F. P. Brady, M. L. Tincknell, N. T. Porile, Z. Caccia, M. D. Partlan, S. Wang, C. P. McParland, F. S. Bieser, J. Romanski, Sebastiano Albergo, K.L. Wolf, Cristina Tuve, V. Lindenstruth, R. P. Scharenberg, H. S. Matis, Y. Choi, Y. Shao, J. L. Romero, Wolfgang Müller, and J. C. Kintner
Subjects: Physics, Nuclear and High Energy Physics, Phase transition, Fission, Critical phenomena, Nuclear Theory, Nuclear physics, Excited state, Atomic physics, Multiplicity (chemistry), Nuclear Experiment, Nucleon, Critical exponent, Excitation
Abstract: Multifragmentation MF results from 1A GeV Au on C have been compared with the Copenhagen statistical multifragmentation model ~SMM!. The complete charge, mass, and momentum reconstruction of the Au projectile was used to identify high momentum ejectiles leaving an excited remnant of mass A, charge Z, and excitation energy E* which subsequently multifragments. Measurement of the magnitude and multiplicity ~energy! dependence of the initial free volume and the breakup volume determines the variable volume parametrization of SMM. Very good agreement is obtained using SMM with the standard values of the SMM parameters. A large number of observables, including the fragment charge yield distributions, fragment multiplicity distributions, caloric curve, critical exponents, and the critical scaling function are explored in this comparison. The two stage structure of SMM is used to determine the effect of cooling of the primary hot fragments. Average fragment yields with Z>3 are essentially unaffected when the excitation energy is 170 the effective latent heat approaches zero. Thus for heavier systems this transition can be identified as a continuous thermal phase transition where a large nucleus breaks up into a number of smaller nuclei with only a minimal release of constituent nucleons. Z
Published: 2001

50. Mass dependence of the transverse momenta of Au projectile fragments at 1.0AGeV

Author: J. Romanski, H. Sann, M. A. Lisa, J. L. Chance, D. Cebra, S. Wang, Renato Potenza, J. B. Elliott, G. Rai, T. J. M. Symons, M. Justice, Wolfgang Müller, T. Wienold, M. A. McMahan, V. Lindenstruth, M. D. Partlan, D. L. Olson, A. D. Chacon, G.V. Russo, J. L. Romero, M. L. Tincknell, N. T. Porile, Z. Caccia, A. Insolia, M. Gilkes, Andrew S. Hirsch, F. S. Bieser, C. P. McParland, P. Warren, K.L. Wolf, Sebastiano Albergo, J. O. Rasmussen, E. L. Hjort, R. P. Scharenberg, H. S. Matis, A. Scott, F. P. Brady, Y. Choi, B. K. Srivastava, Y. Shao, Cristina Tuve, D. Keane, J. C. Kintner, J. A. Hauger, H. H. Wieman, H. G. Ritter, and Salvatore Costa
Subjects: Physics, Nuclear physics, Nuclear and High Energy Physics, Transverse momentum, Humanities
Abstract: J. L. Chance, F. P. Brady, J. L. Romero, S. Albergo, F. Bieser, Z. Caccia, D. Cebra, A. D. Chacon, Y. Choi,* S. Costa, J. B. Elliott, M. L. Gilkes, J. A. Hauger, A. S. Hirsch, E. L. Hjort, A. Insolia, M. Justice, D. Keane, J. C. Kintner, V. Lindenstruth, M. A. Lisa, H. S. Matis, M. McMahan, C. McParland, W. F. J. Muller, D. L. Olson, M. D. Partlan, N. T. Porile, R. Potenza, G. Rai, J. O. Rasmussen, H. G. Ritter, J. Romanski, G. V. Russo, H. Sann, R. Scharenberg, A. Scott, Y. Shao, B. K. Srivastava, T. J. M. Symons, M. Tincknell, C. Tuve, S. Wang, P. G. Warren, H. H. Wieman, T. Wienold, and K. Wolf
Published: 2001

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