Francesco Vissani
(INFN - LNGS)
14/09/2015, 09:40
IceCube has changed the rules of the game and it continues to progress. Remarkably, the observations are compatible with the known neutrino oscillations. Moreover, the topologies of the events have been used to probe exotic physics. Still, we need independent confirmations; the connections of IceCube's neutrinos with astronomical/astrophysical facts heavily rely on speculations--excepting...
Tyce DeYoung
(Michigan State University)
14/09/2015, 11:00
Data from the IceCube Neutrino Observatory has revealed the existence of a flux of high energy neutrinos of extraterrestrial origin, which is observed in a number of analyses spanning different energy ranges, fields of view, and neutrino flavors. The current data are consistent with an isotropic, equal-flavor flux described by a simple power law spectrum, but deviations from this simple model...
maurizio spurio
(University of Bologna (Italy))
14/09/2015, 11:20
The ANTARES experiment has been running in its final configuration since 2008. It is the largest neutrino telescope in the Northern hemisphere. After the discovery of a cosmic neutrino diffuse flux by the IceCube detector, the search for its origin has become a key mission in high-energy astrophysics.
The ANTARES sensitivity is large enough to constrain the origin of the IceCube excess from...
Prof.
Kael Hanson
(University of Wisconsin - Madison)
14/09/2015, 12:10
New groups from the astroparticle physics community have joined an enlarged IceCube Collaboration to pursue construction of a next-generation very large volume neutrino telescope at the South Pole site. This new collaboration, called the IceCube-Gen2 collaboration, hopes to bring forth an instrument that will further push the recently expanded frontiers of knowledge in the field of neutrino...
Alexander Kappes
(Friedrich-Alexander-Univ. Erlangen (DE))
14/09/2015, 14:50
IceCube-Gen2 is the planned next generation neutrino telescope at the South Pole incorporating a high-energy array for neutrino astronomy and a dense array (PINGU) aimed at the determination of the neutrino mass hierarchy. The contribution presents alternatives to IceCube-Gen2’s single-PMT baseline design which are currently being developed. These designs feature up to 24 smaller...
Vladimir Aynutdinov
(INR RAS, Moscow)
14/09/2015, 15:00
The first stage of the Baikal-GVD neutrino telescope will be composed of more than two thousand light sensors, Optical Modules (OMs), installed deep underwater in Lake Baikal. We describe developed calibration methods which use OM LEDs, atmospheric muons and discuss the performance of these methods.
Matteo Sanguineti
(INFN Genova - Università di Genova)
14/09/2015, 15:20
The ANTARES detector is the largest neutrino telescope currently in operation in the North Hemisphere, while KM3NeT
is a future new generation neutrino telescope with a volume of a cubic-kilometres that will be located at the bottom of the Mediterranean Sea.
The point-like neutrino search is one of the main goal of the neutrino telescopes, therefore the evaluation of the pointing performance...
Vladimir Kulikovskiy
(LNS)
14/09/2015, 15:40
The detector of the KM3NeT telescope composed of several thousands digital optical modules is in the process of its realization in the Mediterranean Sea. Each optical module contains 31 3-inch pre-calibrated photomultipliers. Readout of the optical modules and other detector components is synchronized at the level of sub-nanoseconds. The position of the module is measured by acoustic piezo...
Gerard Kieft
(Nikhef National institute for subatomic physics (NL))
14/09/2015, 16:00
The construction of the KM3NeT neutrino telescope in the abyss of the Mediterranean Sea has started. Installation of in total 30 vertical detection units, each supporting 18 optical modules with 31 photomultipliers is foreseen in the first construction phase of the telescope. The KM3NeT timing calibration uses the optical system to send and fan-out an onshore clock signal, derived from a GPS...
Carlos Maximiliano Mollo
(INFN)
14/09/2015, 16:40
Since almost a century photomultipliers have been the main sensors for photon detection in nuclear and astro-particle physics experiments.
In recent years the search for cosmic neutrinos gave birth to enormous size experiments (Kamiokande, Super-Kamiokande, etc.) and even kilometric scale experiments as ICECUBE, Antares, and the future KM3NeT.
A very large volume neutrino telescope requires...
Antoine David Kouchner
(Universite de Paris VII (FR)),
Bruny Baret
(CNRS)
14/09/2015, 17:00
As has been demonstrated by the first generation of neutrino telescopes Antares and IceCube, precise knowledge of the photon detection efficiency of optical modules is of fundamental importance for the understanding of the instrument and accurate event reconstruction. Dedicated test benches have been developped to measure all related quantities for the Digital Optical Modules of the KM3NeT...
Antoine David Kouchner
(Universite de Paris VII (FR)),
Bruny Baret
(CNRS)
14/09/2015, 17:20
KM3NeT is a network of deep-sea neutrino telescopes to be deployed in the Mediterranean Sea, that will perform neutrino astronomy and oscillation studies. It consists of three-dimensional arrays of thousands of optical modules that detect the Cherenkov light induced by charged particles resulting from the interaction of a neutrino with the surrounding medium.
The performance of the...
Prof.
Albrecht KARLE
(Univ. of Wisconsin-Madison)
14/09/2015, 17:40
The observation of cosmic neutrinos can offer insights into the sources of
highest energy cosmic rays and energetic process that are involved to generate them.
IceCube has reported neutrinos with energies beyond 10 eV.
Much larger detection volumes are needed to fully explore the energy region
beyond 10 or 100 PeV.
The Askaryan Radio Array (ARA) is designed to use the...
Allan Hallgren
(Uppsala University)
14/09/2015, 17:55
Detection of neutrinos in the EeV range by observation of radio pulses from the Askaryan effect is proposed by several collaborations. The ARIANNA collaboration is one of them. ARIANNA investigates the possibility to use the unique conditions of the Ross Ice-shelf. The site is isolated with very low levels of anthropogenic radio noise. Reflection of radio signals on the mirror-like ice-sea...
Martin Rongen
(RWTH Aachen)
14/09/2015, 18:00
The IceCube Neutrino Observatory deployed 5160 digital optical modules (DOMs) in a cubic kilometer of deep ice below the South Pole that record the Cherenkov light of passing charged particles. A good understanding of the ice is crucial to the quality of calibration and event reconstruction. While the optical properties of the undisturbed ice are reasonably well understood, the properties of...
Nikos Maragos
(NATIONAL CENTER FOR SCIENTIFIC RESEARCH "DEMOKRITOS")
14/09/2015, 18:20
The deep-sea neutrino telescope in the Mediterranean Sea, being prepared by the KM3NET
collaboration, will contain thousands of optical sensors to readout. The accurate knowledge of the optical properties of deep-sea water is of great importance for the neutrino event reconstruction process. In this study we describe our progress in designing an experimental setup and studying a method to...
Eligio Lisi
(INFN, Bari, Italy)
15/09/2015, 09:00
We present the status of three-neutrino oscillations from a global data analysis, including a partial 2015 update, with emphasis on the unknown parameters: CP phase, octant, mass hierarchy. We also discuss the unprecedented challenges set by (non)parametric systematic uncertainties in hierarchy-sensitive experiments characterized by very high statistics, such as ORCA and PINGU.
Dorothea Samtleben
(Leiden University)
15/09/2015, 09:30
Neutrinos created in interactions of Cosmic Rays with the atmosphere have already for a long time been exploited for measurements of several of the parameters characterizing neutrino oscillations. At low energies, around a few GeV, matter effects from the transition through the Earth are expected to imprint a distinct but also subtle signature on the oscillation pattern specific to the...
Juan-Pablo Yanez
(DESY)
15/09/2015, 10:00
Very large volume neutrino telescopes observe atmospheric neutrinos over a wide energy range (GeV to TeV), after they travel distances as large as the Earth's diameter. DeepCore, the low energy extension of IceCube, has started making meaningful measurements of the neutrino oscillation parameters and by analyzing this flux. PINGU, a proposed extension to lower...
Dustin Hebecker
15/09/2015, 11:00
Prof.
Kael Hanson
(University of Wisconsin - Madison)
15/09/2015, 11:00
The IceCube Detector Operations group continues to improve reliability and add new functionality to the data acquisition (DAQ) and online system as the science of IceCube expands. Following a brief overview of the baseline design which has been running for nearly a decade and highlights of the operational performance of the implementation, this presentation will go on to describe a recent...
Mr
Stefan Coenders
(Technische Universität München)
15/09/2015, 11:20
The IceCube Neutrino Observatory located at the geographic South Pole was designed
to study and discover high energy neutrinos coming from both galactic and
extragalactic astrophysical sources. Track-like events induced by charged-current
muon-neutrino interactions close to the IceCube detector give an angular resolution
better than 1° above TeV energies.
We present here the results of...
Francesco Di Capua
(INFN)
15/09/2015, 11:20
The VSiPMT (Vacuum Silicon PhotoMultiplier Tube) is an innovative design for a revolutionary hybrid photodetector.
The idea, born with the purpose to use a SiPM for large detection volumes, consists in replacing the classical dynode chain with a SiPM.
In this configuration, we match the large sensitive area of a photocathode with the performances of the SiPM technology,
which therefore...
Carmelo Pellegrino
(INFN)
15/09/2015, 11:36
KM3NeT is a large research infrastructure in the Mediterranean Sea that includes a network of deep-sea neutrino telescopes. The telescopes consist of vertical detection units carrying optical modules, whose separation is optimised according to the different ranges of neutrino energy that shall be explored. Two building blocks, each one made of 115 detection units, will be deployed at the...
Mr
Yuji Hotta Hotta
(Hamamatsu)
15/09/2015, 11:40
Hamamatsu has been providing various types of vacuum photon detectors in many fields for many years. We will show the latest developmental status for our PMTs.
Sebastian Euler
(Uppsala University)
15/09/2015, 11:40
Due to the overwhelming background of atmospheric muons, traditional IceCube point source searches in the Southern Hemisphere are sensitive only at neutrino energies above 100 TeV. We will report on a new approach, which focuses on events starting inside the instrumented volume of the IceCube detector. By utilizing different veto techniques we are able to significantly reduce the energy...
Dr
Christian Dille
(Hamamatsu Photonics Deutschland GmbH)
15/09/2015, 12:00
In the year 2014 a new generation of low cross-talk MPPCs has been introduced. Due to further improvements in the manufacturing processes, it is now possible to commercially offer MPPCs, which combine low cross-talk and low after pulse features with a significantly increased photo-detection efficiency (PDE). Besides the capability to manufacture large sized MPPC arrays with high element fill...
Sara Rita Pulvirenti
(INFN - National Institute for Nuclear Physics)
15/09/2015, 12:18
KM3NeT is a future research infrastructure hosting a network of neutrino telescopes in the abyss of the Mediterranean Sea. The whole data transport over an optical network is based on the Dense Wavelength Division Multiplexing technique with optical channels spaced 50 GHz apart and a bit rate of 1.25Gbps. Over the telescope life time, precise temperature control of the laser is required to...
Mr
Barrios-Martí Javier
(IFIC (CSIC-UV))
15/09/2015, 12:20
A search for cosmic neutrino point-like sources using the ANTARES and IceCube neutrino telescopes over the Southern Hemisphere is presented. The ANTARES data was collected between January 2007 and December 2012, whereas the IceCube data ranges from April 2008 to May 2011. Clusters of muon neutrinos over the diffusely distributed background have been looked for by means of an unbinned maximum...
Valentina Giordano
(INFN)
15/09/2015, 12:20
Photomultipliers are widely used in astroparticle physics detectors to measure Cherenkov light in media like water or ice.
KM3NeT neutrino telescope will be the largest underwater neutrino telescope and will be located in the abyss of the Mediterranean Sea.
The detection principle is based on the measurement of the Cherenkov light induced by relativistic charged particles emerging from an...
Cristiano Bozza
(University of Salerno)
15/09/2015, 12:33
KM3NeT is a future research infrastructure hosting a new generation neutrino telescope located at the bottom of the deep seas of the Mediterranean. With the KM3NeT telescope, scientists will search for cosmic neutrinos to study highly energetic objects in the Universe. A new initiative is to extend the research facility with a neutrino detector dedicated to measure the properties of the...
Antoine David Kouchner
(Universite de Paris VII (FR)),
Bruny Baret
(CNRS)
15/09/2015, 12:40
No transient or steady significant signal having been found so far from individual source, we investigate potential collective effects in the spacial or temporal domains in Antares data samples.
On the one hand, we use a two point correlation analysis to look for inhomogeneities in the arrival directions of the high energy muon neutrino candidates detected by the ANTARES neutrino telescope....
Tamas Gal
(University of Erlangen)
15/09/2015, 12:48
KM3NeT is a new generation neutrino telescope in the abyss of the Mediterranean Sea. It will instrument a volume of several cubic kilometres of sea water in its final configuration. Currently, the project is in its first phase with the aim of constructing and installing 31 detection units up to 700m in height, each equipped with 18 digital optical modules. The optical modules are equipped with...
Dr
Emanuele Leonora
(INFN-sezione di Catania)
15/09/2015, 14:00
The KM3NeT European project aims to construct a large volume underwater neutrino telescope in the depths of the Mediterranean Sea. Thanks to a dedicated funding by the Italian Ministry of Education, University and Research (MIUR) in its first phase, referred as KM3NeT-Italia, an 8-towers detector is under construction.
The detection element of the telescope, the optical module, is composed by...
Dr
Konstantinos Manolopoulos
(University of Athens)
15/09/2015, 14:00
GRBNeT is a Gamma Ray Burst Neutrino Telescope made of autonomously operated arrays of deep-sea light detectors, anchored to the sea-bed without any cabled connection to the shore. This paper presents the digital and analog electronics that we have designed and developed for the GRBNeT prototype. We describe the requirements for these electronics and present their design and functionality. We...
Antonio Marinelli
(Institute of Physics, Pisa)
15/09/2015, 14:00
The IceCube collaboration recently released the results of an updated measurement of the astrophysical neutrino flux based on four years of observation. The origin of this emission is still unknown due to the large uncertainties related to the poor angular resolution of shower-like events. While the present results are consistent with a isotropic flux a recent maximum-likelihood analysis of...
Matteo Favaro
(INFN - National Institute for Nuclear Physics)
15/09/2015, 14:18
KM3NeT-Italia is an INFN project supported with Italian PON fundings for building the core of the Italian node of the KM3NeT neutrino telescope.
The detector, made of 700 10" optical modules (OMs) lodged along 8 vertical structures called {\em towers}, will be deployed starting from fall 2015 at the KM3NeT-It site, about 100 km off Capo Passero, Italy, 3500 m deep.
The {\em all data to...
Riccardo PAPALEO
(INFN LNS)
15/09/2015, 14:20
The KM3NeT European project aims to construct a large volume underwater neutrino telescope in the depths of the Mediterranean Sea. INFN and KM3NeT collaboration, thanks to a dedicated funding of 21.000.000 (PON 2007-2013), are committed to building and deploying the Phase 1 of the telescope, composed of a network of detection units: 8 towers, equipped with single PMT optical modules, and 24...
Luigi Antonio Fusco
(University of Bologna)
15/09/2015, 14:20
The existence of cosmic neutrinos has been reported by the IceCube Collaboration. Though this measurement is consistent with an isotropic neutrino flux, a sub-dominant galactic component coming from extended region such as the Galactic Plane/Ridge cannot be excluded.
The ANTARES detector, located in the Mediterranean Sea, is currently the largest and longest operated under-water neutrino...
Carlo Alessandro Nicolau
(INFN - National Institute for Nuclear Physics)
15/09/2015, 14:33
The KM3NeT European project has entered the production stage of a large volume neutrino telescope that will be deployed at about 100 km off the Sicily coast. The forthcoming installation includes 24 strings, equipped with multi-PMT optical modules, and 8 towers. The KM3NeT tower design is based on the NEMO Phase-2 prototype tower, deployed in March 2013. In order to optimize production costs,...
Konstantinos Pikounis
(NCSR Demokritos)
15/09/2015, 15:00
GRBNeT is a project aiming at the detection of ultra-high energy neutrinos, for example neutrinos originating from Gamma Ray Bursts. The goal is to design, construct and test-deploy a prototype unit of an autonomous (data/energy-wise) neutrino detector.
Being autonomous is crucial since for the detection of ultra-high energy neutrinos a very large volume of water is required. Large...
Luigi Antonio Fusco
(University of Bologna)
15/09/2015, 15:00
The KM3NeT Collaboration has started the construction of a research infrastructure hosting a network of underwater neutrino observatories in the Mediterranean Sea. Two telescopes based on the same technology are being built: KM3NeT/ORCA to measure the neutrino mass hierarchy and to study atmospheric neutrino oscillations and KM3NeT/ARCA to detect high-energy cosmic neutrinos both in diffuse...
David Schultz
(University of Wisconsin-Madison)
15/09/2015, 15:10
IceCube's simulation production relies largely on dynamic, heterogeneous resources spread around the world. Datasets consist of many thousands of job workflow subsets running in parallel as directed
acyclic graphs (DAGs) and using varying resources. IceProd is a set of python daemons which process job workflow and maintain configuration and status information on jobs before, during, and after...
Javier Gonzalez
(Bartol Research Institute, Univ Delaware)
15/09/2015, 15:20
Motivated by the discovery of high-energy astrophysical neutrinos with IceCube, we study the prospects for improved measurements of neutrinos of astrophysical origin with a surface detector array combined with IceCube or a next generation neutrino detector at the South Pole. The background in astrophysical neutrino searches is reduced by tagging muons and neutrinos of atmospheric origin...
Christos Filippidis
(Nat. Cent. for Sci. Res. Demokritos (GR))
15/09/2015, 15:30
KM3NeT is a future European deep-sea research infrastructure hosting a new generation neutrino telescope with a volume of several cubic kilometres that -located at the bottom of the Mediterranean Sea - will open a new window on the universe. International collaborative scientific experiments, like KM3NeT, are generating datasets which are increasing exponentially in both complexity and volume,...
Mr
Christophe Tardy
(POWERSEA)
15/09/2015, 15:40
PowerSea is a spin-off company based on research done by the french CNRS on the wet-mateable underwater connectors.
The reliability and the cost of subsea connections are a key issue for deep sea projects.
The company has already developed a wet-mate connector adapted to marine renewable energies, featuring a high power (24 kV-300A on 3 phases) and a cost adapted to the return of...
Christos Filippidis
(Nat. Cent. for Sci. Res. Demokritos (GR))
15/09/2015, 15:45
International collaborative scientific experiments are generating datasets which are increasing exponentially in both complexity and volume, making their analysis, archival, and sharing one of the grand challenges of the 21st century. These experiments, in their majority, adopt computing models consisting of different Tiers (each Tier is made up of several computing centres and provides a...
Mohamed Rameez
(Universite de Geneve (CH))
15/09/2015, 16:30
Placeholder. The actual abstract will be submitted later.
Dr
Carla Distefano
(LNS-INFN)
15/09/2015, 16:30
The gSeaGen code simulates neutrino-induced events detectable by an underwater neutrino detector. The code is an application based on GENIE (Generates Events for Neutrino Interaction Experiments), a set of libraries developed with the purpose to have a "canonical" Monte Carlo for neutrino interaction physics. The gSeaGen code is able to generate events induced by all neutrino flavours, taking...
Cristiano Bozza
(University of Salerno)
15/09/2015, 16:30
KM3NeT is a new generation neutrino telescope in the Mediterranean Sea. For the operation of the telescope a relational database is designed and implemented for several purposes, like the centralised management of accounts, the storage of all documentation on components and on the status of the detector, of the slow control and calibration data. It also contains information useful during the...
Christos Filippidis
(Nat. Cent. for Sci. Res. Demokritos (GR))
15/09/2015, 17:10
Aim of this work is the development of a multithreaded version of the SIRENE detector simulation software for high energy neutrinos. This approach allows utilization of multiple CPU cores and GPUs, leading to a potentially significant decrease in the required execution time compared to the sequential code. We are making use of MPI, OpenMP frameworks for the production of multithreaded code...
Joakim Sandroos
(Universität Mainz, IceCube)
15/09/2015, 17:10
Next generation atmospheric low-energy neutrino detectors, will be able to measure neutrinos with energies of a few GeV. In this energy range the primary signal below the horizon is neutrino secondaries from cosmic ray interactions in the atmosphere. The measured event rate will depend on the neutrino mass hierarchy, allowing determination of the Neutrino mass hierarchy to a significance level...
Dr
Askhat Gazizov
(GSSI/DESY)
15/09/2015, 17:30
We present an updated set of (anti)neutrino-nucleon charged and neutral current scattering cross-sections with an emphasis on intermediate energies between ~ 3 GeV and ~ 100 GeV. These cross-sections can be used for reconstruction and analysis of events in the future PINGU, ORCA and Hyper-Kamiokande experiments and for detector parameters optimization. Dynamic effects due to the finite...
Luigi Antonio Fusco
(University of Bologna)
15/09/2015, 17:30
The data acquisition conditions in a marine environment are not stable and constant in time. Some biological and physical phenomena follow a seasonal evolution producing a periodical change of the rates registered in a neutrino telescope. Also variations in the sea current velocity affects the measured baseline value and the burst fraction on short time scales.
Monte Carlo simulations of...
Kyle Jero
(University of Wisconsin - Madison)
15/09/2015, 17:46
CORSIKA is a simulation program for extensive air showers initiated by high energy cosmic particles. These air showers create the majority of the muons and neutrinos that neutrino telescopes detect and are considered a background signature in searches for astrophysical neutrinos. This contribution will discuss changes to CORSIKA which allow for faster high energy background simulation. The...
Jon Dumm
(Stockholm University)
15/09/2015, 17:50
The origins of the flux of high-energy astrophysical neutrinos observed by the IceCube Neutrino Observatory continue to elude us. These neutrinos most likely originate in hadronic interactions taking place in or near the sources of cosmic-ray acceleration, causing associated gamma-ray production. We use the VERITAS Imaging Air Cherenkov Telescope to search for these gamma rays from the...
Kyle Jero
(University of Wisconsin - Madison)
15/09/2015, 18:02
We introduce the SQuIDS framework, which was designed to solve quantum mechanical evolution in the density matrix formalism in an efficient way. A specialization of this package for neutrino propagation, called -SQuIDS, is showcased. Finally, we show how this new propagation scheme is being integrated into the IceCube MC software to add flexibility for analyzers.
Ms
EVANGELIA DRAKOPOULOU
(N.C.S.R. Demokritos)
15/09/2015, 18:18
KM3NeT will be a European deep-sea infrastructure of neutrino telescopes covering a volume of several cubic kilometers at the Mediterranean Sea aiming to search for high energy neutrinos from galactic and extragalactic sources. This analysis focuses on muon neutrinos and muons coming from charged-current interactions. In large water Cherenkov detectors the reconstructed muon is used to...
Douglas Cowen
(Pennsylvania State University)
15/09/2015, 18:30
The Astrophysical Multimessenger Observatory Network (AMON) will link the world’s leading high-energy neutrino, cosmic-ray, gamma-ray and gravitational wave observatories by performing real-time coincidence searches for multimessenger sources from observatory subthreshold data streams. The resulting coincidences will be distributed to interested parties in the form of electronic alerts for...
Anatoli Fedynitch
(KIT - Karlsruhe Institute of Technology (DE))
16/09/2015, 09:00
The detection of astrophysical neutrinos, certainly a break-through result, introduced new experimental challenges and fundamental questions about acceleration mechanisms of cosmic rays. On one hand IceCube succeeded in finding an unambiguous proof for the existence of a diffuse astrophysical neutrino flux, on the other hand the precise determination of its spectral index and normalization...
Juan M Nieves
(IFIC (CSIC-UV))
16/09/2015, 09:30
New and more precise measurements of neutrino cross sections have renewed the interest in a better understanding of electroweak interactions on nucleons and nuclei. This effort is crucial to achieve the precision goals of the neutrino oscillation program, making new discoveries, like the CP violation in the leptonic sector, possible. We review the recent progress in the physics of neutrino...
Alfons Weber
(STFC/RAL & Uni Oxford)
16/09/2015, 10:00
Some of the most precise measurements of neutrino oscillation parameters have been made using accelerator based muon neutrino beams. By studying how the flavour composition of a beam of muon neutrinos changes and they become electron and tau neutrinos, one can not only measure several mixing angles of the PMNS matrix, but also their mass differences squared. After a short introduction into the...
Christopher van Eldik
(University of Erlangen-Nuremberg)
16/09/2015, 11:00
Since about a decade, ground-based gamma-ray telescopes are key instruments to investigate the high-energy universe at photon energies above ~100 GeV. Mainly devoted to searching for and characterizing cosmic particle acceleration and transport, the instruments HESS, MAGIC, VERITAS and HAWC have so far discovered more than 100 Galactic and extragalactic sources of very-high-energy (VHE) gamma...
Alessandro De Angelis
(Universita degli Studi di Udine (IT))
16/09/2015, 11:40
Several projects planned or proposed can significantly expand our knowledge of the high-energy Universe. Construction of the Cherenkov telescope array CTA is going to start in October, and other detectors are planned which will use the reconstruction of extensive air showers. This talk describes the physics potential of this exploration, with particular attention to possible discoveries on...
Rob van der Meer
(ASTRON)
16/09/2015, 12:20
ASTERICS (Astronomy ESFRI and Research Infrastructure Cluster) brings together astronomers and astroparticle physicists of 22 institutes in Europe to help Europe’s world-leading observatories work together to find common solutions to their Big Data challenges, their interoperability and scheduling, and their data access, searching for cross-cutting solutions with mutual and wide-ranging...
Antonio Capone
(Universita e INFN, Roma I (IT))
16/09/2015, 14:30