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60 60

The ANTARES project

Sep 17, 2013 09/13

by T. Montaruli

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The ANTARES deep-sea neutrino telescope will be located at a depth of 2400 m in the Mediterranean Sea. Deployment of the detector will commence this Autumn and is expected to be completed by the end of 2004. With a surface area of the order of 0.1 km^2 it will be one of the largest European detectors. The aim of neutrino telescopes is to detect high-energy neutrinos from astrophysical sources whilst also providing information on the early Universe. Successful operation of ANTARES in a deep sea...
Source: http://arxiv.org/abs/astro-ph/0207531v1

23 23

Comparison of muon and neutrino times from decays of mesons in the atmosphere

Sep 23, 2013 09/13

by T. Montaruli; F. Ronga

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We propose a test to compare the speed of muons and muon neutrinos produced in the same bundles in the atmosphere. By comparing the arrival times of primary muons and muons induced by neutrinos, experiments such as Super-Kamiokande, IceCube and ANTARES could verify recent hints on the possibility that neutrinos have a velocity larger than the speed of light. For smaller detectors such as MINOS and OPERA, where it may be challenging to recognize downgoing muons induced by neutrinos inside the...
Source: http://arxiv.org/abs/1109.6238v4

35 35

Status report of the ANTARES project

Sep 22, 2013 09/13

by T. Montaruli; for ANTARES Collaboration

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The ANTARES project aims at the construction of an underwater neutrino telescope at the scale of 0.1 km^2 2400 m deep in the Mediterranean Sea. After a 4-year R&D program, the ANTARES project has entered the construction phase which will be concluded by the end of 2004. The current status of the project is reported.
Source: http://arxiv.org/abs/hep-ex/0201009v1

24 24

Galactic discrete sources of high energy neutrinos

Sep 20, 2013 09/13

by W. Bednarek; G. F. Burgio; T. Montaruli

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We review recently developed models of galactic discrete sources of high energy neutrinos. Some of them are based on a simple rescaling of the TeV $\gamma$-ray fluxes from recently detected galactic sources, such as, shell-type supernova remnants or pulsar wind nebulae. Others present detailed and originally performed modeling of processes occurring close to compact objects, i.e. neutron stars and low mass black holes, which are supposed to accelerate hadrons close to dense matter and radiation...
Source: http://arxiv.org/abs/astro-ph/0404534v1

24 24

Atmospheric and Astrophysics Neutrinos with MACRO

Sep 20, 2013 09/13

by T. Montaruli; for the MACRO Collaboration

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MACRO can detect three topologies of neutrino induced events, corresponding to different parent neutrino energies. The most numerous sample is made of upward throughgoing muons induced by atmospheric neutrinos of average energy 100 GeV. We have observed less events than expected events and the observed zenith distribution does not fit the expected one in the no-oscillation hypothesis, giving a maximum probability of 0.1 percent. Considering the neutrino (numu-nutau) oscillation hypothesis the...
Source: http://arxiv.org/abs/hep-ex/9810017v1

29 29

Detection of tau neutrinos in underwater neutrino telescopes

Sep 17, 2013 09/13

by E. Bugaev; T. Montaruli; I. Sokalski

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If neutrinos produced in astrophysics sources oscillate, neutrino telescopes can have a chance to detect signals from tau-neutrinos. We present an estimate of the 'double bang' event rate produced by tau neutrinos in cubic kilometer scale detectors.
Source: http://arxiv.org/abs/astro-ph/0305284v1

27 27

Capabilities of an Underwater Detector as a Neutrino Telescope and for the Neutrino Oscillation Search

Sep 21, 2013 09/13

by T. Montaruli for The NEMO Collaboration; M. Ambriola et al

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We report on the results of a Monte Carlo simulation study of a km^3 scale deep underwater Cherenkov detector aimed at detecting neutrinos of astrophysical origin. This analysis has been undertaken as part of the NEMO R&D project to develop such an experiment close to the Southern Italian coasts. We have studied the reconstruction capabilities of various arrays of phototubes in order to determine the detector geometries which optimize performance and cost. We have also investigated the...
Source: http://arxiv.org/abs/hep-ex/9905019v1

48 48

MACRO as a Telescope for Neutrino Astronomy

Sep 21, 2013 09/13

by T. Montaruli for The MACRO Collaboration; M. Ambrosio et al

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We use a sample of 990 upward-going muons, induced primarily by atmospheric neutrinos, to search for neutrinos of astrophysical origin. No evidence has been found using the event direction information. Flux limits of the order of 10^-15 cm^-2 s^-1 are imposed on current models for candidate point-sources. A space-time correlation search has been undertaken between 2328 BATSE gamma ray bursts (GRBs) and MACRO upward-going muons.
Source: http://arxiv.org/abs/hep-ex/9905020v1

76 76

Comparison of the FLUKA calculations with CAPRICE94 data on muons in atmosphere

Jul 20, 2013 07/13

by G. Battistoni; A. Ferrari; T. Montaruli; P. R. Sala

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In order to benchmark the 3-dimensional calculation of the atmospheric neutrino flux based on the FLUKA Monte Carlo code, muon fluxes in the atmosphere have been computed and compared with data taken by the CAPRICE94 experiment at ground level and at different altitudes in the atmosphere. For this purpose only two additions have been introduced with respect to the neutrino flux calculation: the specific solar modulation corresponding to the period of data taking and the bending of charged...
Source: http://arxiv.org/abs/hep-ph/0107241v2

46 46

Astrophysical tau neutrinos and their detection by large neutrino telescopes

Sep 21, 2013 09/13

by E. V. Bugaev; T. Montaruli; I. A. Sokalski

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We present results of the detailed Monte Carlo calculation of the rates of double-bang events in 1 km$^3$ underwater neutrino telescope with taking into account the effects of $\tau$-neutrino propagation through the Earth. As an input, the moderately optimistic theoretical predictions for diffuse neutrino spectra of AGN jets are used.
Source: http://arxiv.org/abs/astro-ph/0311086v1

36 36

Search for WIMPS using Upward-Going Muons in MACRO

Sep 21, 2013 09/13

by T. Montaruli for The MACRO Collaboration; M. Ambrosio et al

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We present updated results on the search for a neutrino signal from the core of the Earth and of the Sun induced by Weakly Interacting Massive Particles (WIMPs). In this paper we concentrate on neutralinos as WIMP candidates. The 971 and 642 events used respectively for the search from the Sun and from the Earth are compatible with the background of atmospheric neutrinos. Consequently we calculate flux limits for various search cones around these sources. Limits as a function of the neutralino...
Source: http://arxiv.org/abs/hep-ex/9905021v1

38 38

Search for a possible space-time correlation between high energy neutrinos and gamma-ray bursts

Sep 19, 2013 09/13

by T. Montaruli; F. Ronga; for the MACRO Collaboration

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We look for space-time correlations between 2233 gamma-bursts in the Batse Catalogs and 894 upward-going muons produced by neutrino interactions in the rock below or inside MACRO. Considering a search cone of 10 degrees around GRB directions and a time window of 200 s we find 0 events to be compared to 0.035 expected background events due to atmospheric neutrinos. The corresponding upper limit (90% c.l.) is 0.87 * 10^-9 cm^-2 upward-going muons per average burst.
Source: http://arxiv.org/abs/astro-ph/9812333v1

39 39

High energy extension of the FLUKA atmospheric neutrino flux

Sep 18, 2013 09/13

by G. Battistoni; A. Ferrari; T. Montaruli; P. R. Sala

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The atmospheric neutrino flux calculated with FLUKA was originally limited to 100-200 GeV for statistical reasons. In order to make it available for the analysis of high energy events, like upward through-going muons detected by neutrino telescopes, we have extended the calculation so to provide a reliable neutrino yield per primary nucleon up to about 10**6 GeV/nucleon, as far as the interaction model is concerned. We point out that the primary flux model above 100 GeV/nucleon still...
Source: http://arxiv.org/abs/hep-ph/0305208v1

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The FLUKA atmospheric neutrino flux calculation

Sep 17, 2013 09/13

by G. Battistoni; A. Ferrari; T. Montaruli; P. R. Sala

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The 3-dimensional (3-D) calculation of the atmospheric neutrino flux by means of the FLUKA Monte Carlo model is here described in all details, starting from the latest data on primary cosmic ray spectra. The importance of a 3-D calculation and of its consequences have been already debated in a previous paper. Here instead the focus is on the absolute flux. We stress the relevant aspects of the hadronic interaction model of FLUKA in the atmospheric neutrino flux calculation. This model is...
Source: http://arxiv.org/abs/hep-ph/0207035v2

33 33

A simulation code to assist designing space missions of the Airwatch type

Sep 20, 2013 09/13

by T. Montaruli; R. Bellotti; F. Cafagna; M. Circella; C. N. De Marzo; P. Lipari

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The design of an Airwatch type space mission can greatly benefit from a flexible simulation code for establishing the values of the main parameters of the experiment. We present here a code written for this purpose. The cosmic ray primary spectrum at very high energies, the atmosphere modelling, the fluorescence yield, the photon propagation and the detector response are taken into account in order to optimize the fundamental design parameters of the experiment, namely orbit height, field of...
Source: http://arxiv.org/abs/hep-ex/9810014v1

33 33

A 3-Dimensional Calculation of Atmospheric Neutrino Flux

Sep 21, 2013 09/13

by G. Battistoni; A. Ferrari; P. Lipari; T. Montaruli; P. R. Sala; T. Rancati

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An extensive 3-dimensional Monte Carlo calculation of the atmospheric neutrino flux is in progress with the FLUKA Monte Carlo code. The results are compared to those obtained under the 1-dimensional approximation, where secondary particles and decay products are assumed to be collinear to the primary cosmic ray, as usually done in most of the already existing flux calculations. It is shown that the collinear approximation gives rise to a wrong angular distribution of neutrinos, essentially in...
Source: http://arxiv.org/abs/hep-ph/9907408v1

28 28

Results from the Blazar Monitoring Campaign at the Whipple 10m Gamma-ray Telescope

Sep 21, 2013 09/13

by David Steele; for the VERITAS Collaboration; M. T. Carini; P. Charlot; O. Kurtanidze; A. Lahteenmaki; T. Montaruli; A. C. Sadun; M. Villata

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In September 2005, the observing program of the Whipple 10 m gamma-ray telescope was redefined to be dedicated almost exclusively to AGN monitoring. Since then the five Northern Hemisphere blazars that had already been detected at Whipple are monitored routinely each night that they are visible. Thanks to the efforts of a large number of multiwavelength collaborators, the first year of this program has been very successful. We report here on the analysis of Markarian 421 observations taken from...
Source: http://arxiv.org/abs/0709.3869v1

0 0.0

Design, optimization and characterization of the light concentrators of the single-mirror small size telescopes of the Cherenkov Telescope Array

Jun 30, 2018 06/18

by J. A. Aguilar; A. Basili; V. Boccone; F. Cadoux; A. Christov; D. della Volpe; T. Montaruli; L. Platos; M. Rameez; for the SST-1M sub-Consortium

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The focal-plane camera of $\gamma$-ray telescopes frequently uses light concentrators in front of light sensors. The purpose of these concentrators is to increase the effective area of the camera as well as to reduce the stray light coming at large incident angles. These light concentrators are usually based on the Winston cone design. In this contribution we present the design of an hexagonal hollow light concentrator with a lateral profile optimized using a cubic B\'ezier function to achieve...
Topics: Physics, Instrumentation and Methods for Astrophysics, Astrophysics, Instrumentation and Detectors
Source: http://arxiv.org/abs/1404.2734

9 9.0

Camera calibration strategy of the SST-1M prototype of the Cherenokov Telescope Array

Jun 28, 2018 06/18

by E. Prandini; M. Heller; E. Lyard; E. jr. Schioppa; A. Neronov; W. Bilnik; J. Błocki; L. Bogacz; T. Bulik; F. Cadoux; A. Christov; M. Curyło; D. della Volpe; M. Dyrda; Y. Favre; A. Frankowski; Ł. Grudnik; M. Grudzińska; B. Idźkowski; M. Jamrozy; M. Janiak; J. Kasperek; K. Lalik; E. Mach; D. Mandat; A. Marszałek; J. Michałowski; R. Moderski; T. Montaruli; J. Niemiec; M. Ostrowski; P. Paśko; M. Pech; A. Porcelli; M. Rameez; P. Rajda; P. Schovanek; K. Seweryn; K. Skowron; V. Sliusar; M. Sowiński; Ł. Stawarz; M. Stodulska; M. Stodulski; S. Toscano; I. Troyano Pujadas; R. Walter; M. Więcek; A. Zagdański; K. Ziętara; P. Żychowski; for the CTA Consortium

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The SST-1M telescope is one of the prototypes under construction proposed to be part of the future Cherenkov Telescope Array. It uses a standard Davis-Cotton design for the optics and telescope structure, with a dish diameter of 4 meters and a large field-of-view of 9 degrees. The innovative camera design is composed of a photo-detection plane with 1296 pixels including entrance window, light concentrators, Silicon Photomultipliers (SiPMs), and pre-amplifier stages together with a fully digital...
Topics: Instrumentation and Methods for Astrophysics, Astrophysics
Source: http://arxiv.org/abs/1508.06397

2 2.0

The SST-1M camera for the Cherenkov Telescope Array

Jun 28, 2018 06/18

by E. J. Schioppa; F. Cadoux; A. Christov; D. della Volpe; Y. Favre; M. Heller; T. Montaruli; A. Porcelli; M. Rameez; I. Troyano Pujadas; W. Bilnik; J. Blocki; L. Bogacz; T. Bulik; M. Curylo; M. Dyrda; A. Frankowski; L. Grudniki; M. Grudzinska; B. Idzkowski; M. Jamrozy; M. Janiak; J. Kasperek; K. Lalik; E. Lyard; E. Mach; D. Mandat; A. Marszalek; J. Michaowski; R. Moderski; A. Neronov; J. Niemiec; M. Ostrowski; P. Pasko; M. Pech; E. Prandini; P. Rajda; P. Schovanek; K. Seweryn; K. Skowron; V. Sliusar; M. Sowinski; L. Stawarz; M. Stodulska; M. Stodulski; S. Toscano; R. Walter; M. Wiecek; A. Zagdanski; K. Zietara; P. Zychowski

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The prototype camera of the single-mirror Small Size Telescopes (SST-1M) proposed for the Cherenkov Telescope Array (CTA) project has been designed to be very compact and to deliver high performance over thirty years of operation. The camera is composed of an hexagonal photo-detection plane made of custom designed large area hexagonal silicon photomultipliers and a high throughput, highly configurable, fully digital readout and trigger system (DigiCam). The camera will be installed on the...
Topics: Instrumentation and Methods for Astrophysics, Astrophysics
Source: http://arxiv.org/abs/1508.06453

2 2.0

Using muon rings for the optical throughput calibration of the SST-1M prototype for the Cherenkov Telescope Array

Jun 28, 2018 06/18

by S. Toscano; E. Prandini; W. Bilnik; J. Błocki; L. Bogacz; T. Bulik; F. Cadoux; A. Christov; M. Curyło; D. della Volpe; M. Dyrda; Y. Favre; A. Frankowski; Ł. Grudnik; M. Grudzińska; M. Heller; B. Idźkowski; M. Jamrozy; M. Janiak; J. Kasperek; K. Lalik; E. Lyard; E. Mach; D. Mandat; A. Marszałek; J. Michałowski; R. Moderski; T. Montaruli; A. Neronov; J. Niemiec; M. Ostrowski; P. Paśko; M. Pech; A. Porcelli; M. Rameez; P. Rajda; E. jr. Schioppa; P. Schovanek; K. Seweryn; K. Skowron; V. Sliusar; M. Sowiński; Ł. Stawarz; M. Stodulska; M. Stodulski; I. Troyano Pujadas; R. Walter; M. Więcek; A. Zagdański; K. Ziętara; P. Żychowski; for the CTA Consortium

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Imaging Atmospheric Cherenkov Telescopes (IACTs) are ground-based instruments devoted to the study of very high energy gamma-rays coming from space. The detection technique consists of observing images created by the Cherenkov light emitted when gamma rays, or more generally cosmic rays, propagate through the atmosphere. While in the case of protons or gamma-rays the images present a filled and more or less elongated shape, energetic muons penetrating the atmosphere are visualised as...
Topics: Instrumentation and Methods for Astrophysics, Astrophysics
Source: http://arxiv.org/abs/1509.00266

3 3.0

Performance of the SST-1M telescope for the Cherenkov Telescope Array observatory

Jun 28, 2018 06/18

by R. Moderski; W. Bilnik; J. Błocki; L. Bogacz; T. Bulik; F. Cadoux; A. Christov; M. Chruślińska; M. Curyło; D. della Volpe; M. Dyrda; Y. Favre; A. Frankowski; Ł. Grudnik; M. Grudzińska; M. Heller; B. Idźkowski; M. Jamrozy; M. Janiak; J. Kasperek; K. Lalik; E. Lyard; E. Mach; D. Mandat; A. Marszałek; J. Michałowski; T. Montaruli; A. Neronov; J. Niemiec; M. Ostrowski; P. Paśko; M. Pech; A. Porcelli; E. Prandini; E. Pueschel; P. Rajda; M. Rameez; P. Rozwadowski; E. jr Schioppa; P. Schovanek; K. Seweryn; K. Skowron; V. Sliusar; M. Sowiński; Ł. Stawarz; M. Stodulska; M. Stodulski; S. Toscano; I. Troyano Pujadas; R. Walter; M. Wiȩcek; A. Zagdański; K. Ziȩtara; P. Żychowski; for the CTA Consortium

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The single mirror small-size telescope (SST-1M) is one of the telescope projects being proposed for the Cherenkov Telescope Array observatory by a sub-consortium of Polish and Swiss institutions. The SST-1M prototype structure is currently being constructed at the Institute of Nuclear Physics in Cracow, Poland, while the camera will be assembled at the University of Geneva, Switzerland. This prototype enables measurements of parameters having a decisive influence on the telescope performance....
Topics: Instrumentation and Methods for Astrophysics, Astrophysics
Source: http://arxiv.org/abs/1508.06459

0 0.0

FACT -- The G-APD revolution in Cherenkov astronomy

Jun 30, 2018 06/18

by T. Bretz; H. Anderhub; M. Backes; A. Biland; V. Boccone; I. Braun; J. Buß; F. Cadoux; V. Commichau; L. Djambazov; D. Dorner; S. Einecke; D. Eisenacher; A. Gendotti; O. Grimm; H. von Gunten; C. Haller; C. Hempfling; D. Hildebrand; U. Horisberger; B. Huber; K. S. Kim; M. L. Knoetig; J. H. Köhne; T. Krähenbühl; B. Krumm; M. Lee; E. Lorenz; W. Lustermann; E. Lyard; K. Mannheim; M. Meharga; K. Meier; S. Müuller; T. Montaruli; D. Neise; F. Nessi-Tedaldi; A. K. Overkemping; A. Paravac; F. Pauss; D. Renker; W. Rhode; M. Ribordy; U. Röser; J. P. Stucki; J. Schneider; T. Steinbring; F. Temme; J. Thaele; S. Tobler; G. Viertel; P. Vogler; R. Walter; K. Warda; Q. Weitzel; M. Zänglein

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Since two years, the FACT telescope is operating on the Canary Island of La Palma. Apart from its purpose to serve as a monitoring facility for the brightest TeV blazars, it was built as a major step to establish solid state photon counters as detectors in Cherenkov astronomy. The camera of the First G-APD Cherenkov Telesope comprises 1440 Geiger-mode avalanche photo diodes (G-APD), equipped with solid light guides to increase the effective light collection area of each sensor. Since no...
Topics: Physics, Instrumentation and Methods for Astrophysics, Astrophysics, Instrumentation and Detectors
Source: http://arxiv.org/abs/1403.3573

4 4.0

Software design for the control system for Small-Size Telescopes with single-mirror of the Cherenkov Telescope Array

Jun 28, 2018 06/18

by A. Porcelli for the CTA Consortium; for the SST-1M sub-consortium; :; W. Bilnik; J. Błocki; L. Bogacz; J. Borkowski; T. Bulik; F. Cadoux; A. Christov; M. Curyło; D. della Volpe; M. Dyrda; Y. Favre; A. Frankowski; Ł. Grudnik; M. Grudzińska; M. Heller; B. Idźkowski; M. Jamrozy; M. Janiak; J. Kasperek; K. Lalik; E. Lyard; E. Mach; D. Mandat; A. Marszałek; J. Michałowski; R. Moderski; M. Rameez; T. Montaruli; A. Neronov; J. Niemiec; M. Ostrowski; P. Paśko; M. Pech; A. Porcelli; E. Prandini; P. Rajda; E. jr Schioppa; P. Schovanek; K. Seweryn; K. Skowron; V. Sliusar; M. Sowiński; Ł. Stawarz; M. Stodulska; M. Stodulski; I. Troyano Pujadas; S. Toscano; R. Walter; M. Wiȩcek; A. Zagdański; K. Ziȩtara; P. Zychowski

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The Small-Size Telescope with single-mirror (SST-1M) is a 4 m Davies-Cotton telescope and is among the proposed telescope designs for the Cherenkov Telescope Array (CTA). It is conceived to provide the high-energy ($>$ few TeV) coverage. The SST-1M contains proven technology for the telescope structure and innovative electronics and photosensors for the camera. Its design is meant to be simple, low-budget and easy-to-build industrially. Each device subsystem of an SST-1M telescope is made...
Topics: High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics, Astrophysics
Source: http://arxiv.org/abs/1508.07472

104 104

Design and Operation of FACT -- The First G-APD Cherenkov Telescope

Jul 20, 2013 07/13

by H. Anderhub; M. Backes; A. Biland; V. Boccone; I. Braun; T. Bretz; J. Buß; F. Cadoux; V. Commichau; L. Djambazov; D. Dorner; S. Einecke; D. Eisenacher; A. Gendotti; O. Grimm; H. von Gunten; C. Haller; D. Hildebrand; U. Horisberger; B. Huber; K. -S. Kim; M. L. Knoetig; J. H. K"ohne; T. Kr"ahenb"uhl; B. Krumm; M. Lee; E. Lorenz; W. Lustermann; E. Lyard; K. Mannheim; M. Meharga; K. Meier; T. Montaruli; D. Neise; F. Nessi-Tedaldi; A. -K. Overkemping; A. Paravac; F. Pauss; D. Renker; W. Rhode; M. Ribordy; U. R"oser; J. -P. Stucki; J. Schneider; T. Steinbring; F. Temme; J. Thaele; S. Tobler; G. Viertel; P. Vogler; R. Walter; K. Warda; Q. Weitzel; M. Z"anglein

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The First G-APD Cherenkov Telescope (FACT) is designed to detect cosmic gamma-rays with energies from several hundred GeV up to about 10 TeV using the Imaging Atmospheric Cherenkov Technique. In contrast to former or existing telescopes, the camera of the FACT telescope is comprised of solid-state Geiger-mode Avalanche Photodiodes (G-APD) instead of photomultiplier tubes for photo detection. It is the first full-scale device of its kind employing this new technology. The telescope is operated...
Source: http://arxiv.org/abs/1304.1710v1

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TeV and Multi-wavelength Observations of Mrk 421 in 2006-2008

Sep 21, 2013 09/13

by V. A. Acciari; E. Aliu; T. Arlen; T. Aune; M. Beilicke; W. Benbow; D. Boltuch; S. M. Bradbury; J. H. Buckley; V. Bugaev; K. Byrum; A. Cannon; A. Cesarini; L. Ciupik; W. Cui; R. Dickherber; C. Duke; A. Falcone; J. P. Finley; G. Finnegan; L. Fortson; A. Furniss; N. Galante; D. Gall; G. H. Gillanders; S. Godambe; J. Grube; R. Guenette; G. Gyuk; D. Hanna; J. Holder; C. M. Hui; T. B. Humensky; A. Imran; P. Kaaret; N. Karlsson; M. Kertzman; D. Kieda; A. Konopelko; H. Krawczynski; F. Krennrich; M. J. Lang; G. Maier; S. McArthur; M. McCutcheon; P. Moriarty; R. A. Ong; A. N. Otte; M. Ouellette; D. Pandel; J. S. Perkins; A. Pichel; M. Pohl; J. Quinn; K. Ragan; L. C. Reyes; P. T. Reynolds; E. Roache; H. J. Rose; A. C. Rovero; M. Schroedter; G. H. Sembroski; G. Demet Senturk; D. Steele; S. P. Swordy; M. Theiling; S. Thibadeau; A. Varlotta; V. V. Vassiliev; S. Vincent; R. G. Wagner; S. P. Wakely; J. E. Ward; T. C. Weekes; A. Weinstein; T. Weisgarber; D. A. Williams; S. Wissel; M. Wood; B. Zitzer; A. Garson; K. Lee; A. C. Sadun; M. Carini; D. Barnaby; K. Cook; J. Maune; A. Pease; S. Smith; R. Walters; A. Berdyugin; E. Lindfors; K. Nilsson; M. Pasanen; J. Sainio; A. Sillanpaa; L. O. Takalo; C. Villforth; T. Montaruli; M. Baker; A. Lahteenmaki; M. Tornikoski; T. Hovatta; E. Nieppola; H. D. Aller; M. F. Aller

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We report on TeV gamma-ray observations of the blazar Mrk 421 (redshift of 0.031) with the VERITAS observatory and the Whipple 10m Cherenkov telescope. The excellent sensitivity of VERITAS allowed us to sample the TeV gamma-ray fluxes and energy spectra with unprecedented accuracy where Mrk 421 was detected in each of the pointings. A total of 47.3 hrs of VERITAS and 96 hrs of Whipple 10m data were acquired between January 2006 and June 2008. We present the results of a study of the TeV...
Source: http://arxiv.org/abs/1106.1210v2

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Multiwavelength Observations of Markarian 421 in 2005 - 2006

Sep 21, 2013 09/13

by D. Horan; V. A. Acciari; S. M. Bradbury; J. H. Buckley; V. Bugaev; K. L. Byrum; A. Cannon; O. Celik; A. Cesarini; Y. C. K. Chow; L. Ciupik; P. Cogan; A. D. Falcone; S. J. Fegan; J. P. Finley; P. Fortin; L. F. Fortson; D. Gall; G. H. Gillanders; J. Grube; G. Gyuk; D. Hanna; E. Hays; M. Kertzman; J. Kildea; A. Konopelko; H. Krawczynski; F.; M. J. Lang; K. Lee; P. Moriarty; T. Nagai; J. Niemiec; R. A. Ong; J. S. Perkins; M. Pohl; J. Quinn; P. T. Reynolds; H. J. Rose; G. H. Sembroski; A. W. Smith; D. Steele; S. P. Swordy; J. A. Toner; V. V. Vassiliev; S. P. Wakely; T. C. Weekes; R. J. White; D. A. Williams; M. D. Wood; B. Zitzer; H. D. Aller; M. F. Aller; M. Baker; D. Barnaby; M. T. Carini; P. Charlot; J. P. Dumm; N. E. Fields; T. Hovatta; B. Jordan; Y. A. Kovalev; Y. Y. Kovalev; H. A. Krimm; O. M. Kurtanidze; A. Lahteenmaki; J. F. Le Campion; J. Maune; T. Montaruli; A. C. Sadun; S. Smith; M. Tornikoski; M. Turunen; R. Walters

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Since September 2005, the Whipple 10m Gamma-ray Telescope has been operated primarily as a blazar monitor. The five Northern Hemisphere blazars that have already been detected at the Whipple Observatory, Markarian 421, H1426+428, Markarian 501, 1ES 1959+650 and 1ES 2344+514, are monitored routinely each night that they are visible. We report on the Markarian 421 observations taken from November 2005 to June 2006 in the gamma-ray, X-ray, optical and radio bands. During this time, Markarian 421...
Source: http://arxiv.org/abs/0901.1225v1

102 102

A Fast Algorithm for Muon Track Reconstruction and its Application to the ANTARES Neutrino Telescope

Sep 23, 2013 09/13

by ANTARES collaboration; J. A. Aguilar; I. Al Samarai; A. Albert; M. Andre; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; R. Auer; B. Baret; S. Basa; M. Bazzotti; V. Bertin; S. Biagi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; M. C. Bouwhuis; A. M. Brown; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Ph. Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; N. Cottini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; J-P. Ernenwein; S. Escoffier; F. Fehr; V. Flaminio; U. Fritsch; J-L. Fuda; S. Galata; P. Gay; G. Giacomelli; J. P. Gomez-Gonzalez; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernandez-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; N. Kalantar-Nayestanaki; O. Kalekin; A. Kappes; U. Katz; P. Kooijman; C. Kopper; A. Kouchner; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lefevre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Lucarelli; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; A. Mazure; A. Meli; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; C. Naumann; M. Neff; D. Palioselitis; G. E. Pavalas; P. Payre; J. Petrovic; N. Picot-Clemente; C. Picq; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; R. Richter; A. Rostovtsev; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J-P. Schuller; R. Shanidze; F. Simeone; A. Spiess; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; M. Taiuti; C. Tamburini; L. Tasca; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; G. Wijnker; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zuniga

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An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. It is particularly well-suited for real time applications such as online monitoring and fast...
Source: http://arxiv.org/abs/1105.4116v1

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Search for a diffuse flux of high-energy $ν_μ$ with the ANTARES neutrino telescope

Sep 21, 2013 09/13

by ANTARES Collaboration; J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; R. Auer; B. Baret; S. Basa; M. Bazzotti; V. Bertin; S. Biagi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; M. C. Bouwhuis; A. M. Brown; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Ph. Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; N. Cottini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; J-P. Ernenwein; S. Escoffier; F. Fehr; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galata; P. Gay; G. Giacomelli; J. P. Gomez-Gonzalez; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernandez-Rey; B. Herold; J. Hossl; C. C. Hsu; M. de Jong; M. Kadler; N. Kalantar-Nayestanaki; O. Kalekin; A. Kappes; U. Katz; P. Kooijman; C. Kopper; A. Kouchner; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Lucarelli; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; A. Mazure; A. Meli; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; C. Naumann; M. Neff; D. Palioselitis; G. E. Pavalas; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; C. Picq; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; K. Roensch; A. Rostovtsev; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schock; J-P. Schuller; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; M. Taiuti; C. Tamburini; L. Tasca; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; G. Wijnker; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zuniga

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A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A $(0.83\times 2\pi)$ sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an $E^{-2}$ flux spectrum, a 90% c.l. upper...
Source: http://arxiv.org/abs/1011.3772v1

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Time Calibration of the ANTARES Neutrino Telescope

Sep 23, 2013 09/13

by The ANTARES Collaboration; J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J. J. Aubert; R. Auer; B. Baret; S. Basa; M. Bazzotti; V. Bertin; S. Biagi; C. Bigongiari; M. Bou-Cabo; M. C. Bouwhuis; A. M. Brown; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Ph. Charvis; T. Chiarusi; M. Circella; H. Costantini; N. Cottini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; D. Drouhin; T. Eberl; U. Emanuele; J. P. Ernenwein; S. Escoffier; F. Fehr; V. Flaminio; U. Fritsch; J. L. Fuda; S. Galata; P. Gay; G. Giacomelli; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hössl; C. C. Hsu; M. de Jong; M. Kadler; N. Kalantar-Nayestanaki; O. Kalekin; A. Kappes; U. Katz; P. Kooijman; C. Kopper; A. Kouchner; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Lucarelli; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; A. Mazure; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; C. Naumann; M. Neff; D. Palioselitis; G. E. Pavalas; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; C. Picq; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J. P. Schuller; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; M. Taiuti; C. Tamburini; L. Tasca; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; G. Wijnker; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a...
Source: http://arxiv.org/abs/1012.2204v1

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A Search for Time Dependent Neutrino Emission from Microquasars with the ANTARES Telescope

Jun 30, 2018 06/18

by S. Adrián-Martínez; A. Albert; M. André; M. Anghinolfi; G. Anton; M. Ardid; T. Astraatmadja; J. -J. Aubert; B. Baret; J. Barrios; S. Basa; E. Nezri; D. Palioselitis; G. E. Păvălaş; C. Perrina; P. Piattelli; V. Popa; T. Pradier; C. Racca; G. Riccobene; R. Richter; V. Bertin; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; M. Saldaña; D. F. E. Samtleben; A. Sánchez-Losa; M. Sanguineti; P. Sapienza; J. Schmid; S. Biagi; J. Schnabel; S. Schulte; F. Schüssler; T. Seitz; C. Sieger; A. Spies; M. Spurio; J. J. M. Steijger; T. Stolarczyk; M. Taiuti; C. Bigongiari; C. Tamburini; Y. Tayalati; A. Trovato; B. Vallage; C. Vallée; V. Van Elewyck; P. Vernin; E. Visser; D. Vivolo; S. Wagner; C. Bogazzi; J. Wilms; E. de Wolf; K. Yatkin; H. Yepes; J. D. Zornoza; J. Zúñiga; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; A. Capone; L. Caramete; C. Cârloganu; J. Carr; S. Cecchini; Z. Charif; P. Charvis; T. Chiarusi; M. Circella; R. Coniglione; L. Core; H. Costantini; P. Coyle; A. Creusot; G. De Rosa; I. Dekeyser; A. Deschamps; G. De Bonis; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; A. Dumas; T. Eberl; D. Elsässer; U. Emanuele; A. Enzenhöfer; J. -P. Ernenwein; S. Escoffier; K. Fehn; I. Felis; P. Fermani; F. Folger; L. A. Fusco; S. Galatà; P. Gay; S. Geißelsöder; K. Geyer; V. Giordano; A. Gleixner; J. P. Gómez-González; K. Graf; G. Guillard; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; J. Hofestädt; C. W. James; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; P. Kooijman; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; E. Lambard; G. Lambard; G. Larosa; D. Lattuada; D. Lefèvre; E. Leonora; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; S. Martini; A. Mathieu; T. Michael; P. Migliozzi; T. Montaruli; C. Müller; M. Neff

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Results are presented on a search for neutrino emission from a sample of six microquasars, based on the data collected by the ANTARES neutrino telescope between 2007 and 2010. By means of appropriate time cuts, the neutrino search has been restricted to the periods when the acceleration of relativistic jets was taking place at the microquasars under study. The time cuts have been chosen using the information from the X-ray telescopes RXTE/ASM and Swift/BAT, and, in one case, the gamma-ray...
Topics: High Energy Astrophysical Phenomena, Astrophysics
Source: http://arxiv.org/abs/1402.1600

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First Search for Dark Matter Annihilation in the Sun Using the ANTARES Neutrino Telescope

Sep 22, 2013 09/13

by ANTARES Collaboration; S. Adrián-Martinez; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; L. Anton; S. Anvar; M. Ardid; T. Astraatmadjaote; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; C. Bigongiari; C. Bogazzi; B. Bouhou; M. C. Bouwhuis; J. Brünner; J. Busto; A. Capone; C. Cârloganu; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; F. Classen; R. Coniglione; L. Core; H. Costantini; P. Coyle; A. Creusot; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; A. Dumas; T. Eberl; U. Emanuele; A. Enzenhöfer; J-P. Ernenwein; S. Escoffier; K. Fehn; P. Fermani; S. Ferry; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatà; P. Gay; S. Geisselsöder; K. Geyer; G. Giacomelli; V. Giordano; A. Gleixner; J. P. Gómez-González; K. Graf; G. Guillard; G. Hallewell; M. Hamal; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hössl; C. C. Hsu; C. James; M. de Jong; M. Kadler; O. Kalekin; A. Kappesote; U. Katz; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; G. Lambardote; G. Larosa; D. Lattuada; D. Lefèvre; E. Leonora; D. Lo Presti; H. Loehner; S. Loucatos; F. Louis; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; S. Martini; T. Montaruli; M. Morgantiote; H. Motz; C. Mueller; M. Neff; E. Nezri; D. Palioselitis; G. E. Pavalas; J. Petrovic; P. Piattelli; V. Popa; T. Pradier; C. Racca; C. Reed; G. Riccobene; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; M. Rujoiu; D. F. E. Samtleben; A. Sánchez-Losa; P. Sapienza; J. Schmid; J. Schnabel; S. Schulte; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; M. Taiuti; C. Tamburini; A. Trovato; B. Vallage; C. Vallée; V. Van Elewyck; P. Vernin; E. Visser; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; K. Yatkin; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was...
Source: http://arxiv.org/abs/1302.6516v1

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Search for Cosmic Neutrino Point Sources with Four Years of Data from the ANTARES Telescope

Sep 20, 2013 09/13

by ANTARES Collaboration; S. Adrián-Martínez; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; T. Astraatmadja; J. -J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; A. Capone; C. Carloganu; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; R. Coniglione; L. Core; H. Costantini; P. Coyle; A. Creusot; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J. -P. Ernenwein; S. Escoffier; K. Fehn; P. Fermani; M. Ferri; S. Ferry; V. Flaminio; F. Folger; U. Fritsch; J. -L. Fuda; S. Galatà; P. Gay; K. Geyer; G. Giacomelli; V. Giordano; A. Gleixner; J. P. Gómez-González; K. Graf; G. Guillard; G. Hallewell; M. Hamal; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; G. Lambard; G. Larosa; D. Lattuada; E. Leonora; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Louis; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; A. Meli; T. Montaruli; M. Morganti; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Păvălaş; K. Payet; J. Petrovic; P. Piattelli; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; D. F. E. Samtleben; P. Sapienza; J. Schmid; J. Schnabel; J. -P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; A. Trovato; B. Vallage; C. Vallée; V. Van Elewyck; M. Vecchi; P. Vernin; E. Visser; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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In this paper, a time integrated search for point sources of cosmic neutrinos is presented using the data collected from 2007 to 2010 by the ANTARES neutrino telescope. No statistically significant signal has been found and upper limits on the neutrino flux have been obtained. Assuming an $E_{\nu}^{-2}$ spectrum, these flux limits are at $1-10\times10^{-8}$ GeV cm$^{-2}$ s$^{-1}$ for declinations ranging from $-90^{\circ}$ to 40$^{\circ}$. Limits for specific models of RX J1713.7-3946 and Vela...
Source: http://arxiv.org/abs/1207.3105v2

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Search for Neutrino Emission from Gamma-Ray Flaring Blazars with the ANTARES Telescope

Sep 23, 2013 09/13

by S. Adrián-Martínez; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; T. Astraatmadja; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Cârloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; L. Core; H. Costantini; P. Coyle; A. Creusot; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J-P. Ernenwein; S. Escoffier; K. Fehn; P. Fermani; M. Ferri; S. Ferry; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatà; P. Gay; K. Geyer; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; G. Lambard; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Louis; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; A. Meli; T. Montaruli; N. Morganti; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Păvălaş; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; D. F. E. Samtleben; P. Sapienza; F. Schöck; J-P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. M. Steijger; Th. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; C. Vallée; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; E. Visser; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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The ANTARES telescope is well-suited to detect neutrinos produced in astrophysical transient sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. Radio-loud active galactic nuclei with jets pointing almost directly towards the observer, the so-called blazars, are particularly attractive potential neutrino point sources. The all-sky monitor LAT on board the Fermi satellite probes the variability of any given gamma-ray bright blazar in the sky on time scales...
Source: http://arxiv.org/abs/1111.3473v1

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The Positioning System of the ANTARES Neutrino Telescope

Sep 23, 2013 09/13

by S. Adrián-Martínez; M. Ageron; J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J. -J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; P. Coyle; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J. -P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J. -L. Fuda; S. Galatá; P. Gay; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Keller; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefévre; A. Le Van Suu; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; V. Niess; D. Palioselitis; G. E. Păvălaş; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; D. Real; C. Reed; G. Riccobene; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; D. F. E. Samtleben; F. Schöck; J. -P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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The ANTARES neutrino telescope, located 40km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the...
Source: http://arxiv.org/abs/1202.3894v3

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First search for neutrinos in correlation with gamma-ray bursts with the ANTARES neutrino telescope

Sep 22, 2013 09/13

by S. Adrián-Martínez; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. Bouwhuis; J. Brunner; J. Busto; A. Capone; C. Carloganu; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; R. Coniglione; L. Core; H. Costantini; P. Coyle; A. Creusot; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J-P. Ernenwein; S. Escoffier; K. Fehn; P. Fermani; M. Ferri; S. Ferry; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatà; P. Gay; K. Geyer; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Hallewell; M. Hamal; H. van Haren; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; G. Lambard; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Louis; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Pavalas; K. Payet; J. Petrovic; P. Piattelli; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; D. F. E. Samtleben; A. Sánchez-Losa; P. Sapienza; J. Schnabel; F. Schöck; J-P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; M. Taiuti; C. Tamburini; A. Trovato; B. Vallage; C. Vallée; V. Van Elewyck; M. Vecchi; P. Vernin; E. Visser; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúniga

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A search for neutrino-induced muons in correlation with a selection of 40 gamma-ray bursts that occurred in 2007 has been performed with the ANTARES neutrino telescope. During that period, the detector consisted of 5 detection lines. The ANTARES neutrino telescope is sensitive to TeV--PeV neutrinos that are predicted from gamma-ray bursts. No events were found in correlation with the prompt photon emission of the gamma-ray bursts and upper limits have been placed on the flux and fluence of...
Source: http://arxiv.org/abs/1302.6750v1

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On the sensitivity of the HAWC observatory to gamma-ray bursts

Sep 21, 2013 09/13

by HAWC collaboration; A. U. Abeysekara; J. A. Aguilar; S. Aguilar; R. Alfaro; E. Almaraz; C. Álvarez; J. de D. Álvarez-Romero; M. Álvarez; R. Arceo; J. C. Arteaga-Velázquez; C. Badillo; A. Barber; B. M. Baughman; N. Bautista-Elivar; E. Belmont; E. Benítez; S. Y. BenZvi; D. Berley; A. Bernal; E. Bonamente; J. Braun; R. Caballero-Lopez; I. Cabrera; A. Carramiñana; L. Carrasco; M. Castillo; L. Chambers; R. Conde; P. Condreay; U. Cotti; J. Cotzomi; J. C. D'Olivo; E. de la Fuente; C. De León; S. Delay; D. Delepine; T. DeYoung; L. Diaz; L. Diaz-Cruz; B. L. Dingus; M. A. Duvernois; D. Edmunds; R. W. Ellsworth; B. Fick; D. W. Fiorino; A. Flandes; N. I. Fraija; A. Galindo; J. L. García-Luna; G. García-Torales; F. Garfias; L. X. González; M. M. González; J. A. Goodman; V. Grabski; M. Gussert; C. Guzmán-Ceron; Z. Hampel-Arias; T. Harris; E. Hays; L. Hernandez-Cervantes; P. H. Hüntemeyer; A. Imran; A. Iriarte; J. J. Jimenez; P. Karn; N. Kelley-Hoskins; D. Kieda; R. Langarica; A. Lara; R. Lauer; W. H. Lee; E. C. Linares; J. T. Linnemann; M. Longo; R. Luna-García; H. Martínez; J. Martínez; L. A. Martínez; O. Martínez; J. Martínez-Castro; M. Martos; J. Matthews; J. E. McEnery; G. Medina-Tanco; J. E. Mendoza-Torres; P. A. Miranda-Romagnoli; T. Montaruli; E. Moreno; M. Mostafa; M. Napsuciale; J. Nava; L. Nellen; M. Newbold; R. Noriega-Papaqui; T. Oceguera-Becerra; A. Olmos Tapia; V. Orozco; V. Pérez; E. G. Pérez-Pérez; J. S. Perkins; J. Pretz; C. Ramirez; I. Ramírez; D. Rebello; A. Rentería; J. Reyes; D. Rosa-González; A. Rosado; J. M. Ryan; J. R. Sacahui; H. Salazar; F. Salesa; A. Sandoval; E. Santos; M. Schneider; A. Shoup; S. Silich; G. Sinnis; A. J. Smith; K. Sparks; W. Springer; F. Suárez; N. Suarez; I. Taboada; A. F. Tellez; G. Tenorio-Tagle; A. Tepe; P. A. Toale; K. Tollefson; I. Torres; T. N. Ukwatta; J. Valdes-Galicia; P. Vanegas; V. Vasileiou; O. Vázquez; X. Vázquez; L. Villaseñor; W. Wall; J. S. Walters; D. Warner; S. Westerhoff; I. G. Wisher; J. Wood; G. B. Yodh; D. Zaborov; A. Zepeda

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We present the sensitivity of HAWC to Gamma Ray Bursts (GRBs). HAWC is a very high-energy gamma-ray observatory currently under construction in Mexico at an altitude of 4100 m. It will observe atmospheric air showers via the water Cherenkov method. HAWC will consist of 300 large water tanks instrumented with 4 photomultipliers each. HAWC has two data acquisition (DAQ) systems. The main DAQ system reads out coincident signals in the tanks and reconstructs the direction and energy of individual...
Source: http://arxiv.org/abs/1108.6034v2

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First Search for Point Sources of High Energy Cosmic Neutrinos with the ANTARES Neutrino Telescope

Sep 21, 2013 09/13

by Antares Collaboration; S. Adrián-Martínez; J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J-P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatà; P. Gay; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Pavalas; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; D. F. E. Samtleben; P. Sapienza; F. Schöck; J-P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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Results are presented of a search for cosmic sources of high energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 +/- 0.1 degrees. The neutrino flux sensitivity is 7.5 x 10-8 ~...
Source: http://arxiv.org/abs/1108.0292v1

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The ANTARES Telescope Neutrino Alert System

Sep 22, 2013 09/13

by M. Ageron; J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Cârloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenöfer; J-P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatà; P. Gay; G. Giacomelli; V. Giordano; J. Gòmez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamar; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Păvălaş; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J-P. Schuller; F. Schüssler; R. Shanidze; F. Simeone; A. Spies; M. Spuriol; J. J. M. Steijger; Th. Stolarczyk; A. Sànchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zùñiga

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The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are...
Source: http://arxiv.org/abs/1103.4477v1

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AMADEUS - The Acoustic Neutrino Detection Test System of the ANTARES Deep-Sea Neutrino Telescope

Sep 19, 2013 09/13

by ANTARES collaboration; J. A. Aguilar; I. Al Samarai; A. Albert; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J. -J. Aubert; R. Auer; E. Barbarito; B. Baret; S. Basa; M. Bazzotti; V. Bertin; S. Biagi; C. Bigongiari; M. Bou-Cabo; M. C. Bouwhuis; A. Brown; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Cârloganu; G. Carminati; J. Carr; B. Cassano; E. Castorina; V. Cavasinni; S. Cecchini; A. Ceres; Ph. Charvis; T. Chiarusi; N. Chon Sen; M. Circella; R. Coniglione; H. Costantini; N. Cottini; P. Coyle; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; D. Drouhin; T. Eberl; U. Emanuele; J. -P. Ernenwein; S. Escoffier; F. Fehr; C. Fiorello; V. Flaminio; U. Fritsch; J. -L. Fuda; P. Gay; G. Giacomelli; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; A. J. Heijboer; E. Heine; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; M. de Jong; N. Kalantar-Nayestanaki; O. Kalekin; A. Kappes; U. Katz; P. Keller; P. Kooijman; C. Kopper; A. Kouchner; W. Kretschmer; R. Lahmann; P. Lamare; G. Lambard; G. Larosa; H. Laschinsky; H. Le Provost; D. Lefèvre; G. Lelaizant; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; F. Louis; F. Lucarelli; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; A. Mazure; M. Mongelli; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; C. Naumann; M. Neff; R. Ostasch; D. Palioselitis; G. E. Pavalas; P. Payre; J. Petrovic; N. Picot-Clemente; C. Picq; V. Popa; T. Pradier; E. Presani; C. Racca; A. Radu; C. Reed; G. Riccobene; C. Richardt; M. Rujoiu; M. Ruppi; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J. -P. Schuller; R. Shanidze; F. Simeone; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; M. Taiuti; C. Tamburini; L. Tasca; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; G. Wijnker; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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The AMADEUS (ANTARES Modules for the Acoustic Detection Under the Sea) system which is described in this article aims at the investigation of techniques for acoustic detection of neutrinos in the deep sea. It is integrated into the ANTARES neutrino telescope in the Mediterranean Sea. Its acoustic sensors, installed at water depths between 2050 and 2300 m, employ piezo-electric elements for the broad-band recording of signals with frequencies ranging up to 125 kHz. The typical sensitivity of the...
Source: http://arxiv.org/abs/1009.4179v3

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Measurement of the Group Velocity of Light in Sea Water at the ANTARES Site

Sep 23, 2013 09/13

by S. Adrián-Martínez; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; H. Costantini; P. Coyle; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J-P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatá; P. Gay; K. Geyer; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefévre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; J. E. McMillan; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Păvălaş; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; R. Richter; C. Riviére; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; D. F. E. Samtleben; P. Sapienza; F. Schöck; J-P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; L. F. Thompson; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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The group velocity of light has been measured at eight different wavelengths between 385 nm and 532 nm in the Mediterranean Sea at a depth of about 2.2 km with the ANTARES optical beacon systems. A parametrisation of the dependence of the refractive index on wavelength based on the salinity, pressure and temperature of the sea water at the ANTARES site is in good agreement with these measurements.
Source: http://arxiv.org/abs/1110.5184v2

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Contributions to the 32nd International Cosmic Ray Conference (ICRC 2011) by the ANTARES collaboration

Sep 24, 2013 09/13

by S. Adrián-Martínez; J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; H. Costantini; P. Coyle; A. Creusto; C. Curtil; G. De Bonis; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J-P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatà; P. Gay; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; A. Meli; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Pavalas; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J-P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; C. Vallée; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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The ANTARES detector, completed in 2008, is the largest neutrino telescope in the Northern hemisphere. It is located at a depth of 2.5 km in the Mediterranean Sea, 40 km off the Toulon shore. The scientific scope of the experiment is very broad, being the search for astrophysical neutrinos the main goal. In this paper we collect the 22 contributions of the ANTARES collaboration to the 32nd International Cosmic Ray Conference (ICRC 2011). At this stage of the experiment the scientific output is...
Source: http://arxiv.org/abs/1112.0478v1

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A method for detection of muon induced electromagnetic showers with the ANTARES detector

Sep 21, 2013 09/13

by J. A. Aguilar; I. Al. Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J. J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; A. Bigi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Carloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; P. Charvis; T. Chiarusi; M. Circella; R. Coniglione; H. Costantini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J. P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J. L. Fuda; S. Galatà; P. Gay; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hö\ssl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martinez-Mora; A. Meli; T. Montaruli; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. P\uav\uala\cs; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J. P. Schuller; F. Schüssler; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; T. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earth's atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to...
Source: http://arxiv.org/abs/1106.0426v2

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Search for Relativistic Magnetic Monopoles with the ANTARES Neutrino Telescope

Sep 23, 2013 09/13

by ANTARES Collaboration; S. Adrián-Martínez; J. A. Aguilar; I. Al Samarai; A. Albert; M. André; M. Anghinolfi; G. Anton; S. Anvar; M. Ardid; A. C. Assis Jesus; T. Astraatmadja; J-J. Aubert; B. Baret; S. Basa; V. Bertin; S. Biagi; C. Bigongiari; C. Bogazzi; M. Bou-Cabo; B. Bouhou; M. C. Bouwhuis; J. Brunner; J. Busto; F. Camarena; A. Capone; C. Cârloganu; G. Carminati; J. Carr; S. Cecchini; Z. Charif; Ph. Charvis; T. Chiarusi; M. Circella; H. Costantini; P. Coyle; C. Curtil; M. P. Decowski; I. Dekeyser; A. Deschamps; C. Distefano; C. Donzaud; D. Dornic; Q. Dorosti; D. Drouhin; T. Eberl; U. Emanuele; A. Enzenhöfer; J-P. Ernenwein; S. Escoffier; P. Fermani; M. Ferri; V. Flaminio; F. Folger; U. Fritsch; J-L. Fuda; S. Galatà; P. Gay; G. Giacomelli; V. Giordano; J. P. Gómez-González; K. Graf; G. Guillard; G. Halladjian; G. Hallewell; H. van Haren; J. Hartman; A. J. Heijboer; Y. Hello; J. J. Hernández-Rey; B. Herold; J. Hößl; C. C. Hsu; M. de Jong; M. Kadler; O. Kalekin; A. Kappes; U. Katz; O. Kavatsyuk; P. Kooijman; C. Kopper; A. Kouchner; I. Kreykenbohm; V. Kulikovskiy; R. Lahmann; P. Lamare; G. Larosa; D. Lattuada; D. Lefèvre; G. Lim; D. Lo Presti; H. Loehner; S. Loucatos; S. Mangano; M. Marcelin; A. Margiotta; J. A. Martínez-Mora; A. Meli; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; M. Neff; E. Nezri; D. Palioselitis; G. E. Păvălaş; K. Payet; P. Payre; J. Petrovic; P. Piattelli; N. Picot-Clemente; V. Popa; T. Pradier; E. Presani; C. Racca; C. Reed; G. Riccobene; C. Richardt; R. Richter; C. Rivière; A. Robert; K. Roensch; A. Rostovtsev; J. Ruiz-Rivas; M. Rujoiu; G. V. Russo; F. Salesa; P. Sapienza; F. Schöck; J-P. Schuller; F. Schüssler; T. Seitz; R. Shanidze; F. Simeone; A. Spies; M. Spurio; J. J. M. Steijger; Th. Stolarczyk; A. Sánchez-Losa; M. Taiuti; C. Tamburini; S. Toscano; B. Vallage; V. Van Elewyck; G. Vannoni; M. Vecchi; P. Vernin; S. Wagner; G. Wijnker; J. Wilms; E. de Wolf; H. Yepes; D. Zaborov; J. D. Zornoza; J. Zúñiga

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Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric...
Source: http://arxiv.org/abs/1110.2656v2

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Use of event-level neutrino telescope data in global fits for theories of new physics

Sep 20, 2013 09/13

by P. Scott; C. Savage; J. Edsjö; the IceCube Collaboration; :; R. Abbasi; Y. Abdou; M. Ackermann; J. Adams; J. A. Aguilar; M. Ahlers; D. Altmann; K. Andeen; J. Auffenberg; X. Bai; M. Baker; S. W. Barwick; V. Baum; R. Bay; K. Beattie; J. J. Beatty; S. Bechet; J. Becker Tjus; K. -H. Becker; M. Bell; M. L. Benabderrahmane; S. BenZvi; J. Berdermann; P. Berghaus; D. Berley; E. Bernardini; D. Bertrand; D. Z. Besson; D. Bindig; M. Bissok; E. Blaufuss; J. Blumenthal; D. J. Boersma; C. Bohm; D. Bose; S. Böser; O. Botner; L. Brayeur; A. M. Brown; R. Bruijn; J. Brunner; S. Buitink; K. S. Caballero-Mora; M. Carson; J. Casey; M. Casier; D. Chirkin; B. Christy; F. Clevermann; S. Cohen; D. F. Cowen; A. H. Cruz Silva; M. Danninger; J. Daughhetee; J. C. Davis; C. De Clercq; F. Descamps; P. Desiati; G. de Vries-Uiterweerd; T. DeYoung; J. C. Díaz-Vélez; J. Dreyer; J. P. Dumm; M. Dunkman; R. Eagan; J. Eisch; R. W. Ellsworth; O. Engdegård; S. Euler; P. A. Evenson; O. Fadiran; A. R. Fazely; A. Fedynitch; J. Feintzeig; T. Feusels; K. Filimonov; C. Finley; T. Fischer-Wasels; S. Flis; A. Franckowiak; R. Franke; K. Frantzen; T. Fuchs; T. K. Gaisser; J. Gallagher; L. Gerhardt; L. Gladstone; T. Glüsenkamp; A. Goldschmidt; J. A. Goodman; D. Góra; D. Grant; A. Groß; S. Grullon; M. Gurtner; C. Ha; A. Haj Ismail; A. Hallgren; F. Halzen; K. Hanson; D. Heereman; P. Heimann; D. Heinen; K. Helbing; R. Hellauer; S. Hickford; G. C. Hill; K. D. Hoffman; R. Hoffmann; A. Homeier; K. Hoshina; W. Huelsnitz; P. O. Hulth; K. Hultqvist; S. Hussain; A. Ishihara; E. Jacobi; J. Jacobsen; G. S. Japaridze; O. Jlelati; H. Johansson; A. Kappes; T. Karg; A. Karle; J. Kiryluk; F. Kislat; J. Kläs; S. R. Klein; J. -H. Köhne; G. Kohnen; H. Kolanoski; L. Köpke; C. Kopper; S. Kopper; D. J. Koskinen; M. Kowalski; M. Krasberg; G. Kroll; J. Kunnen; N. Kurahashi; T. Kuwabara; M. Labare; K. Laihem; H. Landsman; M. J. Larson; R. Lauer; M. Lesiak-Bzdak; J. Lünemann; J. Madsen; R. Maruyama; K. Mase; H. S. Matis; F. McNally; K. Meagher; M. Merck; P. Mészáros; T. Meures; S. Miarecki; E. Middell; N. Milke; J. Miller; L. Mohrmann; T. Montaruli; R. Morse; S. M. Movit; R. Nahnhauer; U. Naumann; S. C. Nowicki; D. R. Nygren; A. Obertacke; S. Odrowski; A. Olivas; M. Olivo; A. O'Murchadha; S. Panknin; L. Paul; J. A. Pepper; C. Pérez de los Heros; D. Pieloth; N. Pirk; J. Posselt; P. B. Price; G. T. Przybylski; L. Rädel; K. Rawlins; P. Redl; E. Resconi; W. Rhode; M. Ribordy; M. Richman; B. Riedel; J. P. Rodrigues; F. Rothmaier; C. Rott; T. Ruhe; D. Rutledge; B. Ruzybayev; D. Ryckbosch; S. M. Saba; T. Salameh; H. -G. Sander; M. Santander; S. Sarkar; K. Schatto; M. Scheel; F. Scheriau; T. Schmidt; M. Schmitz; S. Schoenen; S. Schöneberg; L. Schönherr; A. Schönwald; A. Schukraft; L. Schulte; O. Schulz; D. Seckel; S. H. Seo; Y. Sestayo; S. Seunarine; M. W. E. Smith; M. Soiron; D. Soldin; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; A. Stasik; T. Stezelberger; R. G. Stokstad; A. Stößl; E. A. Strahler; R. Ström; G. W. Sullivan; H. Taavola; I. Taboada; A. Tamburro; S. Ter-Antonyan; S. Tilav; P. A. Toale; S. Toscano; M. Usner; N. van Eijndhoven; D. van der Drift; A. Van Overloop; J. van Santen; M. Vehring; M. Voge; C. Walck; T. Waldenmaier; M. Wallraff; M. Walter; R. Wasserman; Ch. Weaver; C. Wendt; S. Westerhoff; N. Whitehorn; K. Wiebe; C. H. Wiebusch; D. R. Williams; H. Wissing; M. Wolf; T. R. Wood; K. Woschnagg; C. Xu; D. L. Xu; X. W. Xu; J. P. Yanez; G. Yodh; S. Yoshida; P. Zarzhitsky; J. Ziemann; A. Zilles; M. Zoll

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We present a fast likelihood method for including event-level neutrino telescope data in parameter explorations of theories for new physics, and announce its public release as part of DarkSUSY 5.0.6. Our construction includes both angular and spectral information about neutrino events, as well as their total number. We also present a corresponding measure for simple model exclusion, which can be used for single models without reference to the rest of a parameter space. We perform a number of...
Source: http://arxiv.org/abs/1207.0810v2

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Search for Galactic PeV Gamma Rays with the IceCube Neutrino Observatory

Sep 22, 2013 09/13

by IceCube collaboration; M. G. Aartsen; R. Abbasi; Y. Abdou; M. Ackermann; J. Adams; J. A. Aguilar; M. Ahlers; D. Altmann; K. Andeen; J. Auffenberg; X. Bai; M. Baker; S. W. Barwick; V. Baum; R. Bay; K. Beattie; J. J. Beatty; S. Bechet; J. Becker Tjus; K. -H. Becker; M. Bell; M. L. Benabderrahmane; S. BenZvi; J. Berdermann; P. Berghaus; D. Berley; E. Bernardini; D. Bertrand; D. Z. Besson; D. Bindig; M. Bissok; E. Blaufuss; J. Blumenthal; D. J. Boersma; S. Bohaichuk; C. Bohm; D. Bose1; S. Böser; O. Botner; L. Brayeur; A. M. Brown; R. Bruijn; J. Brunner; S. Buitink; M. Carson; J. Casey; M. Casier; D. Chirkin; B. Christy; K. Clark; F. Clevermann; S. Cohen; D. F. Cowen; A. H. Cruz Silva; M. Danninger; J. Daughhetee; J. C. Davis; C. De Clercq; S. De Ridder; F. Descamps; P. Desiati; G. de Vries-Uiterweerd; T. DeYoung; J. C. Díaz-Vélez; J. Dreyer; J. P. Dumm; M. Dunkman; R. Eagan; B. Eberhardt; J. Eisch; R. W. Ellsworth; O. Engdegård; S. Euler; P. A. Evenson; O. Fadiran; A. R. Fazely; A. Fedynitch; J. Feintzeig; T. Feusels; K. Filimonov; C. Finley; T. Fischer-Wasels; S. Flis; A. Franckowiak; R. Franke; K. Frantzen; T. Fuchs; T. K. Gaisser; J. Gallagher; L. Gerhardt; L. Gladstone; T. Glüsenkamp; A. Goldschmidt; G. Golup; J. A. Goodman; D. Góra; D. Grant; A. Groß; S. Grullon; M. Gurtner; C. Ha; A. Haj Ismail; A. Hallgren; F. Halzen; K. Hanson; D. Heereman; P. Heimann; D. Heinen; K. Helbing; R. Hellauer; S. Hickford; G. C. Hill; K. D. Hoffman; R. Hoffmann; A. Homeier; K. Hoshina; W. Huelsnitz; P. O. Hulth; K. Hultqvist; S. Hussain; A. Ishihara; E. Jacobi; J. Jacobsen; G. S. Japaridze; O. Jlelati; A. Kappes; T. Karg; A. Karle; J. Kiryluk; F. Kislat; J. Kläs; S. R. Klein; J. -H. Köhne; G. Kohnen; H. Kolanoski; L. Köpke; C. Kopper; S. Kopper; D. J. Koskinen; M. Kowalski; M. Krasberg; G. Kroll; J. Kunnen; N. Kurahashi; T. Kuwabara; M. Labare; H. Landsman; M. J. Larson; R. Lauer; M. Lesiak-Bzdak; J. Lünemann; J. Madsen; R. Maruyama; K. Mase; H. S. Matis; F. McNally; K. Meagher; M. Merck; P. Mészáros; T. Meures; S. Miarecki; E. Middell; N. Milke; J. Miller; L. Mohrmann; T. Montaruli; R. Morse; R. Nahnhauer; U. Naumann; S. C. Nowicki; D. R. Nygren; A. Obertacke; S. Odrowski; A. Olivas; M. Olivo; A. O'Murchadha; S. Panknin; L. Paul; J. A. Pepper; C. Pérez de los Heros; D. Pieloth; N. Pirk; J. Posselt; P. B. Price; G. T. Przybylski; L. Rädel; K. Rawlins; P. Redl; E. Resconi; W. Rhode; M. Ribordy; M. Richman; B. Riedel; J. P. Rodrigues; C. Rott; T. Ruhe; B. Ruzybayev; D. Ryckbosch; S. M. Saba; T. Salameh; H. -G. Sander; M. Santander; S. Sarkar; K. Schatto; M. Scheel; F. Scheriau; T. Schmidt; M. Schmitz; S. Schoenen; S. Schöneberg; L. Schönherr; A. Schönwald; A. Schukraft; L. Schulte; O. Schulz; D. Seckel; S. H. Seo; Y. Sestayo; S. Seunarine; C. Sheremata; M. W. E. Smith; M. Soiron; D. Soldin; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; A. Stasik; T. Stezelberger; R. G. Stokstad; A. Stöß; E. A. Strahler; R. Ström; G. W. Sullivan; H. Taavola; I. Taboada; A. Tamburro; S. Ter-Antonyan; S. Tilav; P. A. Toale; S. Toscano; M. Usner; D. van der Drift; N. van Eijndhoven; A. Van Overloop; J. van Santen; M. Vehring; M. Voge1; M. Vraeghe; C. Walck; T. Waldenmaier; M. Wallraff; M. Walter; R. Wasserman; Ch. Weaver; C. Wendt; S. Westerhoff; N. Whitehorn; K. Wiebe; C. H. Wiebusch; D. R. Williams; H. Wissing; M. Wolf; T. R. Wood; K. Woschnagg; C. Xu; D. L. Xu; X. W. Xu; J. P. Yanez; G. Yodh; S. Yoshida; P. Zarzhitsky; J. Ziemann; S. Zierke; A. Zilles; M. Zoll

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Gamma-ray induced air showers are notable for their lack of muons, compared to hadronic showers. Hence, air shower arrays with large underground muon detectors can select a sample greatly enriched in photon showers by rejecting showers containing muons. IceCube is sensitive to muons with energies above ~500 GeV at the surface, which provides an efficient veto system for hadronic air showers with energies above 1 PeV. One year of data from the 40-string IceCube configuration was used to perform...
Source: http://arxiv.org/abs/1210.7992v1

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Measurement of the Atmospheric $ν_e$ flux in IceCube

Sep 23, 2013 09/13

by IceCube Collaboration; M. G. Aartsen; R. Abbasi; Y. Abdou; M. Ackermann; J. Adams; J. A. Aguilar; M. Ahlers; D. Altmann; K. Andeen; J. Auffenberg; X. Bai; M. Baker; S. W. Barwick; V. Baum; R. Bay; K. Beattie; J. J. Beatty; S. Bechet; J. Becker Tjus; K. -H. Becker; M. Bell; M. L. Benabderrahmane; S. BenZvi; J. Berdermann; P. Berghaus; D. Berley; E. Bernardini; D. Bertrand; D. Z. Besson; D. Bindig; M. Bissok; E. Blaufuss; J. Blumenthal; D. J. Boersma; S. Bohaichuk; C. Bohm; D. Bose1; S. Boser; O. Botner; L. Brayeur; A. M. Brown; R. Bruijn; J. Brunner; S. Buitink; M. Carson; J. Casey; M. Casier; D. Chirkin; B. Christy; K. Clark; F. Clevermann; S. Cohen; D. F. Cowen; A. H. Cruz Silva; M. Danninger; J. Daughhetee; J. C. Davis; C. De Clercq; S. De Ridder; F. Descamps; P. Desiati; G. de Vries-Uiterweerd; T. DeYoung; J. C. Diaz-Velez; J. Dreyer; J. P. Dumm; M. Dunkman; R. Eagan; B. Eberhardt; J. Eisch; R. W. Ellsworth; O. Engdegard; S. Euler; P. A. Evenson; O. Fadiran; A. R. Fazely; A. Fedynitch; J. Feintzeig; T. Feusels; K. Filimonov; C. Finley; T. Fischer-Wasels; S. Flis; A. Franckowiak; R. Franke; K. Frantzen; T. Fuchs; T. K. Gaisser; J. Gallagher; L. Gerhardt; L. Gladstone; T. Glusenkamp; A. Goldschmidt; G. Golup; J. A. Goodman; D. Gora; D. Grant; A. Gross; S. Grullon; M. Gurtner; C. Ha; A. Haj Ismail; A. Hallgren; F. Halzen; K. Hanson; D. Heereman; P. Heimann; D. Heinen; K. Helbing; R. Hellauer; S. Hickford; G. C. Hill; K. D. Hoffman; R. Hoffmann; A. Homeier; K. Hoshina; W. Huelsnitz; P. O. Hulth; K. Hultqvist; S. Hussain; A. Ishihara; E. Jacobi; J. Jacobsen; G. S. Japaridze; O. Jlelati; A. Kappes; T. Karg; A. Karle; J. Kiryluk; F. Kislat; J. Klas; S. R. Klein; J. -H. Kohne; G. Kohnen; H. Kolanoski; L. Kopke; C. Kopper; S. Kopper; D. J. Koskinen; M. Kowalski; M. Krasberg; G. Kroll; J. Kunnen; N. Kurahashi; T. Kuwabara; M. Labare; H. Landsman; M. J. Larson; R. Lauer; M. Lesiak-Bzdak; J. Lunemann; J. Madsen; R. Maruyama; K. Mase; H. S. Matis; F. McNally; K. Meagher; M. Merck; P. Meszaros; T. Meures; S. Miarecki; E. Middell; N. Milke; J. Miller; L. Mohrmann; T. Montaruli; R. Morse; R. Nahnhauer; U. Naumann; S. C. Nowicki; D. R. Nygren; A. Obertacke; S. Odrowski; A. Olivas; M. Olivo; A. O'Murchadha; S. Panknin; L. Paul; J. A. Pepper; C. Perez de los Heros; D. Pieloth; N. Pirk; J. Posselt; P. B. Price; G. T. Przybylski; L. Radel; K. Rawlins; P. Redl; E. Resconi; W. Rhode; M. Ribordy; M. Richman; B. Riedel; J. P. Rodrigues; C. Rott; T. Ruhe; B. Ruzybayev; D. Ryckbosch; S. M. Saba; T. Salameh; H. -G. Sander; M. Santander; S. Sarkar; K. Schatto; M. Scheel; F. Scheriau; T. Schmidt; M. Schmitz; S. Schoenen; S. Schoneberg; L. Schonherr; A. Schonwald; A. Schukraft; L. Schulte; O. Schulz; D. Seckel; S. H. Seo; Y. Sestayo; S. Seunarine; C. Sheremata; M. W. E. Smith; M. Soiron; D. Soldin; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; A. Stasik; T. Stezelberger; R. G. Stokstad; A. Stoss; E. A. Strahler; R. Strom; G. W. Sullivan; H. Taavola; I. Taboada; A. Tamburro; S. Ter-Antonyan; S. Tilav; P. A. Toale; S. Toscano; M. Usner; D. van der Drift; N. van Eijndhoven; A. Van Overloop; J. van Santen; M. Vehring; M. Voge1; M. Vraeghe; C. Walck; T. Waldenmaier; M. Wallraff; M. Walter; R. Wasserman; Ch. Weaver; C. Wendt; S. Westerhoff; N. Whitehorn; K. Wiebe; C. H. Wiebusch; D. R. Williams; H. Wissing; M. Wolf; T. R. Wood; K. Woschnagg; C. Xu; D. L. Xu; X. W. Xu; J. P. Yanez; G. Yodh; S. Yoshida; P. Zarzhitsky; J. Ziemann; S. Zierke; A. Zilles; M. Zoll

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We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of operation of IceCube's DeepCore low energy extension. Techniques to identify neutrinos interacting within the DeepCore volume and veto muons originating outside the detector are demonstrated. A sample of 1029 events is observed in 281 days of data, of which 496 $\pm$ 66(stat.) $\pm$ 88(syst.) are estimated to be...
Source: http://arxiv.org/abs/1212.4760v2

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Neutrino analysis of the September 2010 Crab Nebula flare and time-integrated constraints on neutrino emission from the Crab using IceCube

Sep 21, 2013 09/13

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

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We present the results for a search of high-energy muon neutrinos with the IceCube detector in coincidence with the Crab nebula flare reported on September 2010 by various experiments. Due to the unusual flaring state of the otherwise steady source we performed a prompt analysis of the 79-string configuration data to search for neutrinos that might be emitted along with the observed gamma-rays. We performed two different and complementary data selections of neutrino events in the time window of...
Source: http://arxiv.org/abs/1106.3484v2

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All-particle cosmic ray energy spectrum measured with 26 IceTop stations

Sep 23, 2013 09/13

by IceCube Collaboration; R. Abbasi; Y. Abdou; T. Abu-Zayyad; M. Ackermann; J. Adams; J. A. Aguilar; M. Ahlers; D. Altmann; K. Andeen; J. Auffenberg; X. Bai; M. Baker; S. W. Barwick; V. Baum; R. Bay; J. L. Bazo Alba; K. Beattie; J. J. Beatty; S. Bechet; J. K. Becker; K. -H. Becker; M. Bell; M. L. Benabderrahmane; S. BenZvi; J. Berdermann; P. Berghaus; D. Berley; E. Bernardini; D. Bertrand; D. Z. Besson; D. Bindig; M. Bissok; E. Blaufuss; J. Blumenthal; D. J. Boersma; C. Bohm; D. Bose; S. Böser; O. Botner; L. Brayeur; A. M. Brown; S. Buitink; K. S. Caballero-Mora; M. Carson; M. Casier; D. Chirkin; B. Christy; F. Clevermann; S. Cohen; D. F. Cowen; A. H. Cruz Silva; M. V. D'Agostino; M. Danninger; J. Daughhetee; J. C. Davis; C. De Clercq; T. Degner; F. Descamps; P. Desiati; G. de Vries-Uiterweerd; T. DeYoung; J. C. Díaz-Vélez; J. Dreyer; J. P. Dumm; M. Dunkman; J. Eisch; R. W. Ellsworth; O. Engdegård; S. Euler; P. A. Evenson; O. Fadiran; A. R. Fazely; A. Fedynitch; J. Feintzeig; T. Feusels; K. Filimonov; C. Finley; T. Fischer-Wasels; S. Flis; A. Franckowiak; R. Franke; T. K. Gaisser; J. Gallagher; L. Gerhardt; L. Gladstone; T. Glüsenkamp; A. Goldschmidt; J. A. Goodman; D. Góra; D. Grant; A. Groß; S. Grullon; M. Gurtner; C. Ha; A. Haj Ismail; A. Hallgren; F. Halzen; K. Han; K. Hanson; P. Heimann; D. Heinen; K. Helbing; R. Hellauer; S. Hickford; G. C. Hill; K. D. Hoffman; B. Hoffmann; A. Homeier; K. Hoshina; W. Huelsnitz; P. O. Hulth; K. Hultqvist; S. Hussain; A. Ishihara; E. Jacobi; J. Jacobsen; G. S. Japaridze; H. Johansson; A. Kappes; T. Karg; A. Karle; J. Kiryluk; F. Kislat; S. R. Klein; S. Klepser; J. -H. Köhne; G. Kohnen; H. Kolanoski; L. Köpke; S. Kopper; D. J. Koskinen; M. Kowalski; M. Krasberg; G. Kroll; J. Kunnen; N. Kurahashi; T. Kuwabara; M. Labare; K. Laihem; H. Landsman; M. J. Larson; R. Lauer; J. Lünemann; J. Madsen; R. Maruyama; K. Mase; H. S. Matis; K. Meagher; M. Merck; P. Mészáros; T. Meures; S. Miarecki; E. Middell; N. Milke; J. Miller; T. Montaruli; R. Morse; S. M. Movit; R. Nahnhauer; J. W. Nam; U. Naumann; S. C. Nowicki; D. R. Nygren; S. Odrowski; A. Olivas; M. Olivo; A. O'Murchadha; S. Panknin; L. Paul; C. Pérez de los Heros; D. Pieloth; J. Posselt; P. B. Price; G. T. Przybylski; K. Rawlins; P. Redl; E. Resconi; W. Rhode; M. Ribordy; M. Richman; B. Riedel; J. P. Rodrigues; F. Rothmaier; C. Rott; T. Ruhe; D. Rutledge; B. Ruzybayev; D. Ryckbosch; H. -G. Sander; M. Santander; S. Sarkar; K. Schatto; M. Scheel; T. Schmidt; S. Schöneberg; A. Schönwald; A. Schukraft; L. Schulte; A. Schultes; O. Schulz; M. Schunck; D. Seckel; B. Semburg; S. H. Seo; Y. Sestayo; S. Seunarine; A. Silvestri; M. W. E. Smith; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; T. Stezelberger; R. G. Stokstad; A. Stößl; E. A. Strahler; R. Ström; M. Stüer; G. W. Sullivan; H. Taavola; I. Taboada; A. Tamburro; S. Ter-Antonyan; S. Tilav; P. A. Toale; S. Toscano; D. Tosi; N. van Eijndhoven; A. Van Overloop; J. van Santen; M. Vehring; M. Voge; C. Walck; T. Waldenmaier; M. Wallraff; M. Walter; R. Wasserman; Ch. Weaver; C. Wendt; S. Westerhoff; N. Whitehorn; K. Wiebe; C. H. Wiebusch; D. R. Williams; R. Wischnewski; H. Wissing; M. Wolf; T. R. Wood; K. Woschnagg; C. Xu; D. L. Xu; X. W. Xu; J. P. Yanez; G. Yodh; S. Yoshida; P. Zarzhitsky; M. Zoll

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We report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, the surface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysis were taken between June and October, 2007, with 26 surface stations operational at that time, corresponding to about one third of the final array. The fiducial area used in this analysis was 0.122 km^2. The analysis investigated the energy spectrum from 1 to 100 PeV measured for three different...
Source: http://arxiv.org/abs/1202.3039v1

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Constraints on high-energy neutrino emission from SN 2008D

Sep 22, 2013 09/13

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

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SN 2008D, a core collapse supernova at a distance of 27 Mpc, was serendipitously discovered by the Swift satellite through an associated X-ray flash. Core collapse supernovae have been observed in association with long gamma-ray bursts and X-ray flashes and a physical connection is widely assumed. This connection could imply that some core collapse supernovae possess mildly relativistic jets in which high-energy neutrinos are produced through proton-proton collisions. The predicted neutrino...
Source: http://arxiv.org/abs/1101.3942v1

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