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Felix Aharonian (DIAS and MPIK)04/07/2016, 14:30The key role of high energy gamma-ray observations is described in the context of the origin of galactic and extragalactic cosmic rays. The achievements of recent years regarding both the experimental and theoretical activities are highlighted, and the prospects of the field are discussed.Go to contribution page
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Francesca Romana Spada (PI)04/07/2016, 15:20The Fermi mission is operating in low Earth orbit since June 2008, and has collected more than one billion photons from the whole sky in the 100 MeV - 100 GeV band. Thanks to the large acceptance of the Large Area Telescope, a pair-conversion telescope for high-energy electromagnetic radiation, Fermi also provided the largest high-energy cosmic-ray electron sample to date, with about 10k...Go to contribution page
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Dario Grasso (PI)04/07/2016, 15:50Several independent analyzes of Fermi-LAT results found evidences of a spatial dependence of the cosmic ray (CR) proton spectral index which is not accounted for in conventional models of CR transport in the Galaxy. Moreover, several CR experiments have established the presence of a CR spectral hardening above few hundred GeV. We show that these results may have a relevant impact on the...Go to contribution page
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Leonardo Di Venere (BA)04/07/2016, 16:10In about eight years of data taking, the Large Area Telescope (LAT) onboard the Fermi satellite proved to be an excellent instrument to detect and observe Supernova Remnants (SNRs) in the gamma ray energy band, from one hundred MeV to a few hundred GeV. This energy range is crucial to provide information on the physical processes occurring at the source, which involve both accelerated leptons...Go to contribution page
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Alessandro De Angelis (INFN)04/07/2016, 17:00The present generation of Imaging Air Cherenkov Telescopes (IACTs) has greatly improved our knowledge on the Very High Energy side of the Universe. The MAGIC IACTs operate in stereoscopic configuration since 2009 in La Palma, Canary Islands. This talk will present a few of MAGIC latest and most relevant results, in particular related to the physics of extragalactic objects and...Go to contribution page
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Dr Johannes Knapp (DESY Zeuthen)04/07/2016, 17:30The Cherenkov Telescope Array (CTA) will be the global, next-generation instrument for high-energy gamma-ray astronomy, with unprecedented performance in every respect. It will be an observatory with telescopes in the South and North, and will gradually become an open observatory. CTA is rapidly approaching its realisation. Construction of pre-production telescopes has commenced and data...Go to contribution page
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Dr Markus Garczarczyk (DESY)04/07/2016, 18:00The Cherenkov Telescope Array (CTA), is an international project for the next generation ground-based observatory for gamma-ray astronomy in the energy range from 20 GeV to 300 TeV. The sensitivity in the core energy range will be dominated by up to 40 Medium Size Telescopes (MSTs) distributed over the northern and southern observatory sites. The MST has a modified Davies-Cotton reflector...Go to contribution page
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Nepomuk Otte (Georgia Institute of Technology)05/07/2016, 09:00VERITAS is an array of four 12-m imaging Cherenkov telescopes, sensitive to very-high energy (VHE; >100 GeV) gamma-ray photons. The science program of VERITAS includes the characterization of the VHE gamma-ray sky, the study of cosmic ray accelerators (both within and outside of the Galaxy), and other topics in astrophysics, cosmology and fundamental physics. Collaboration with...Go to contribution page
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Prof. Miguel Mostafa (Penn State Univ.)05/07/2016, 09:30The High Altitude Water Cherenkov (HAWC) experiment is a large field of view, continuously operated TeV gamma ray observatory located at 4,100 meters above sea level inside the Pico de Orizaba national park in Mexico. It consists of an array of 300 water Cherenkov detectors densely-spaced over an area of 22,000 square meters. The high altitude, the large active area, and the optical isolation...Go to contribution page
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Aldo Morselli (ROMA2)05/07/2016, 10:00Detection of gamma rays and cosmic rays from the annihilation or decay of dark matter particles is a promising method for identifying dark matter, understanding its intrinsic properties, and mapping its distribution in the universe. I will review recent results from the Fermi Gamma-ray Space Telescope and other space-based experiments, and highlight the constraints these currently place on...Go to contribution page
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Dr Carmela Bonavolontà05/07/2016, 10:20
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Dr Melania Del Santo (INAF/IASF-Palermo)05/07/2016, 10:22
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Tristano Di Girolamo (NA)05/07/2016, 10:24
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Emanuele Fiandrini (PG)05/07/2016, 10:26
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Francesco Giordano (BA)05/07/2016, 10:28
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Mr Stefano Grazzi (Study and Research Centre “Enrico Fermi” (Rome))05/07/2016, 10:30
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Andrea Lavagno (TO)05/07/2016, 10:32
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Mr Mihai Niculescu-Oglinzanu (HoriaHulubei National Institute for R&D in Physics)05/07/2016, 10:34
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Dr Beatrice Panico (NA)05/07/2016, 10:36
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Julio Arturo Rabanal Reina (LAL/IN2P3/CNRS)05/07/2016, 10:38
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Giuliana Russano (TIFP)05/07/2016, 10:40
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Dr VALENTINA SCOTTI (NA)05/07/2016, 10:42
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Dr VALENTINA SCOTTI (NA)05/07/2016, 10:44
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Daniela Simone (BA)05/07/2016, 10:46
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Dr Gerd Puehlhofer (IAAT, University of Tuebingen)05/07/2016, 11:00The High Energy Stereoscopic System (H.E.S.S.) collaboration runs a system of meanwhile five Imaging Air Cherenkov Telescopes in the Khomas Highlands of Namibia. Observations of the sky in the photon energy range between below 100 GeV and ~100 TeV have revealed a large number of objects that are capable of efficiently accelerating particles to TeV energies. In this contribution, recent...Go to contribution page
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Pierre Brun (CEA Saclay)05/07/2016, 11:30Gamma-ray astronomy is a powerful mean of studying particle physics and cosmology independently of particle colliders and more conventional observatories. In a 50 GeV-50 TeV range, observations of Galactic and extragalactic high-energy sources allow to efficiently search for new particles such as dark matter particles and axions; they probe the UV to infrared backgrounds of the universe whose...Go to contribution page
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Dr Francois Brun (CENBG, CNRS/IN2P3, Bordeaux, France)05/07/2016, 11:50The supernova remnant (SNR) W49B originated from a core-collapse supernova that occurred between one and four thousand years ago, and subsequently evolved into a mixed-morphology remnant, which is interacting with molecular clouds (MC). SNR/MC associations are particularly interesting for probing the acceleration of hadrons in SNRs and consequently the origin of Galactic cosmic rays. The...Go to contribution page
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Nicola Giglietto (Politecnico di BARI e INFN - BARI), Silvia Rainò (Università e INFN-BARI)05/07/2016, 12:10The high energy gamma-ray emission from the Sun is due to the interactions of cosmic ray (CR) protons and electrons with matter and photons in the solar environment. Such interactions lead to two component gamma-ray emission: a disk-like emission due to the nuclear interactions of CR protons and nuclei in the solar atmosphere and a space extended emission due to the inverse Compton (IC)...Go to contribution page
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Bruna Bertucci (PG)05/07/2016, 14:30In the last decade, direct cosmic ray studies entered in a new era of precision. Access to space with long-term running experiments and state of the art detectors has been the key to advance and to unveil unexpected features in the CR composition and energy spectra. A wealth of measurements is now available in a wide energy range, from few MeV to TeV, which provides new constraints to the...Go to contribution page
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Mr Alberto Oliva (CIEMAT (Spain))05/07/2016, 15:20AMS-02 is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and operating continuously since then. With a collection rate of approximately 1.7 × 10^{10} events/year, combined with the particle identification capabilities of 5 independent detectors, AMS is able to accurately measure all the charged cosmic rays (CRs) species separating...Go to contribution page
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Paolo Bernardini (LE)05/07/2016, 16:20The DAMPE (DArk Matter Particle Explorer) satellite was launched on December 17, 2015 and is in smooth data taking since few days after. It was designed in order to work properly for at least three years and, thanks to its large geometric factor (~0.3 m2 sr for protons and nuclei), is integrating one of the largest exposures for galactic cosmic ray (CR) studies in space. Even if primarily...Go to contribution page
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Giovanni Ambrosi (PG)05/07/2016, 16:50The High Energy cosmic-Radiation Detection (HERD) facility is one of several space astronomy payloads of the cosmic lighthouse program onboard China’s Space Station, which is planned for operation starting around 2022 for about 10 years. The main scientific objectives of HERD are indirect dark matter search, precise cosmic ray spectrum and composition measurements up to the knee energy, and...Go to contribution page
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Roberta Sparvoli (ROMA2)05/07/2016, 17:20It was the 15th of June of 2006 when the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome in Kazakhstan. Since then, PAMELA has been making high-precision measurements of the charged component of the cosmic radiation opening a new era of precision studies in cosmic rays. The measured antiparticle component of the cosmic radiation shows features that can be...Go to contribution page
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Alan Watson (University of Leeds)06/07/2016, 09:00Measurements relevant to the arrival direction distribution, the energy spectrum and the mass composition of cosmic rays above 1 PeV will be reviewed. Interpretation of raw data is affected, to a greater or lesser extent, by our lack of knowledge of key parameters of hadronic interactions: the limitations will be emphasised. Work at the Auger Observatory leads to the view that there is a...Go to contribution page
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Martina Bohacova (Institute of Physics, Prague)06/07/2016, 09:50The Pierre Auger Observatory, based in Mendoza province, Argentina, represents the largest Ultrahigh Energy Cosmic Ray observatory ever built. After twelve years of operation the exposure reached almost 60 000 km2 sr yr and the unprecedented quality data set spans three orders of magnitude in energy. The status and performance of the detectors and their enhancements will be described. The...Go to contribution page
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Mr Benedikt Zimmermann (Karlsruhe Institute of Technology (KIT))06/07/2016, 10:20The Auger Engineering Radio Array (AERA) consists of 153 autonomous radio stations at the site of the Pierre Auger Observatory in Malargüe, Prov. of Mendoza, Argentina. With an area of 17 km^2 covered, AERA is the largest radio-detector worldwide for UHECR physics. The radio stations are sensitive in the 30 to 80 MHz band to the coherent radio signal emitted by the electromagnetic air shower...Go to contribution page
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Gabriella Cataldi (LE)06/07/2016, 10:40The Pierre Auger Observatory has begun a major Upgrade (AugerPrime), with an emphasis on improved mass composition determination using the surface detectors of the Observatory. AugerPrime will include new 4 m2 plastic scintillator detectors on top of all 1660 water-Cherenkov detectors, a faster and more powerful electronics, a large array of buried muon detectors, and an extended dynamic...Go to contribution page
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Dr Daisuke Ikeda (Institute for Cosmic Ray Research, University of Tokyo)06/07/2016, 11:30The Telescope Array (TA) experiment, located in Utah, US, is the largest ultra-high energy cosmic ray (UHECR) observatory in the northern hemisphere. TA observes the UHECR using the hybrid technique which consists of 507 surface detectors (SD) on a 1.2km grid covering about 700 km^2 area and three fluorescence detector (FD) stations surrounding the SD array. Specification of the detectors,...Go to contribution page
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Mr Philippe Gorodetzky (APC-Paris 7)06/07/2016, 12:00Jem-Euso is a project to set-up a large fiel of view UV telescope in space to detect HECR. The surface on ground is about 200 000 km^2. The air mass seen by the instrument makes it very good to detect high energy neutrinos. Very luminous atmospheric events will also be studied through special electronics. The pathfinders are: - Timmins balloon (CNES), launched in 2014, was able during the 5...Go to contribution page
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Mr Philippe Gorodetzky (APC-Paris 7)06/07/2016, 12:20The EUSO-SPB (Extreme Universe Space Observatory - Super Pressure Balloon) is a fluorescence telescope at a stratospheric balloon with the main goal of detecting UV- light from Extensive Air Showers for the first time from (near) space. For this purpose it will employ a UV telescope consisting of three 1 m2 Fresnel lenses focusing light on 2304 channels of multi-anode photomultipliers. The...Go to contribution page
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Enrico Calloni (INFN Napoli)07/07/2016, 09:00
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Massimiliano Razzano (PISA)07/07/2016, 09:50Since 2011 the Virgo collaboration has undertaken a major detector upgrade towards a second generation detector with the aim of increasing the number of observable galaxies (and thus the detection rate) by three orders of magnitude. The installation and integration of Advanced Virgo was recently completed and the commissioning phase has begun with the objective of joining the two Advanced LIGO...Go to contribution page
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Luciano Di Fiore (INFN Napoli)07/07/2016, 10:20A torsion pendulum with 2 soft degrees of freedom (DOF), realized by off-axis cascading two torsion fibers, has been built and operated. This instrument allows simultaneous measurement, of force and torque acting on the suspended test mass, approaching free-fall condition down to a few mHz. It was developed for ground testing on two DOFs, before the launch, of the Gravitational Reference...Go to contribution page
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Dr ik siong heng (University of Glasgow)07/07/2016, 11:10The detection of gravitational waves from binary black hole coalescence and merger was a major highlight of Advanced LIGO's first observing run (O1). These detections of gravitational wave heralded the dawn of gravitational wave astronomy. The Advanced LIGO detectors, though significantly more sensitive than any other gravitational wave detector before, were not operating at design sensitivity...Go to contribution page
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Rita Dolesi (TIFP)07/07/2016, 11:40
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Massimiliano Razzano (on behalf of the LIGO Scientific Collaboration and Virgo Collaboration)07/07/2016, 12:10The direct detection of gravitational waves from the merger of binary black holes marked the birth of gravitational wave astronomy and opened a new chapter in the multimessenger study of the cosmos. Among gravitational wave sources, mergers of compact objects containing at least one neutron star are thought to be associated with electromagnetic transient phenomena, such as short Gamma Ray...Go to contribution page
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Dr Lorenzo Natalucci (INAF/IAPS)07/07/2016, 12:40The detection of the first gravitational waves from GW150914 by the LIGO-Virgo collaboration has triggered many multi-wavelength campaigns using space and ground observatories. Large field-of-view gamma-ray telescopes, such as those onboard INTEGRAL have the capability of detecting relatively faint transient events (>~ a few 10^-8 erg cm-2) and are unique for the study of the prompt emission....Go to contribution page
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Angela Dora Vittoria Di Virgilio (PI)07/07/2016, 13:00GINGER (Gyroscopes IN General Relativity) is a proposal aiming at measuring the Lense-Thirring effect with an experiment based on Earth. It is an array of ringlasers, which are the most sensitive inertial sensors to measure the rotation rate of the Earth. After reviewing the importance of light as a probe for testing the structure of space-time, we describe the GINGER project. GINGER is based...Go to contribution page
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Delia Tosi (DESY)07/07/2016, 14:30The IceCube Neutrino Observatory features a cubic-kilometer volume of instrumented ice at the geographic South Pole. A high energy astrophysical neutrino flux has been confirmed since 2013 as an excess of neutrinos above 10 TeV compared to the expectation from atmospheric neutrino background. This excess, nowadays significant at >6 sigma level, has been observed both in neutrino interactions...Go to contribution page
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Shigeru Yoshida (Chba University)07/07/2016, 15:00The IceCube neutrino observatory has detected the bulk of cosmic neutrinos with energies from TeV to PeV together with the stringent limits on the EeV-energy neutrino flux. It has already contained rich informative implications to the yet-unknown origin of ultra-high energy cosmic rays. In this talk we discuss what the neutrino observations have revealed the characteristics of cosmic accelerators.Go to contribution page
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Maurizio Spurio (BO)07/07/2016, 16:20A primary goal of a deep-sea neutrino telescopes as ANTARES is the search for astrophysical neutrinos in the TeV-PeV range. ANTARES has been running in its final configuration since 2008; it comprise an array of 885 photomultipliers tubes housed in optical modules, detecting the Cherenkov light induced by charged particles produced by neutrino interactions in and around the instrumented...Go to contribution page
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Piera Sapienza (Laboratorio Nazionale del Sud INFN)07/07/2016, 16:50The KM3NeT Collaboration aims at the discovery and subsequent observation of high neutrino sources in the Universe (ARCA) and at the determination of the neutrino mass hierarchy (ORCA). The KM3NeT technologies, current status and expected performances are reported. In particular the ARCA detector is described and its perspectives for detection of high energy neutrinos signals from different...Go to contribution page
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Alberto Guglielmi (PD)07/07/2016, 17:20The ICARUS-T600 is the biggest LAr-TPC detector ever realized. The ICARUS Collaboration concluded a very successful, long duration run with the T600 detector at the LNGS underground laboratory, taking data both with the CNGS neutrino beam and with cosmic rays. It performed a sensitive search for anomalous nue appearance as suggested by LSND signal and experimental neutrino anomalies at...Go to contribution page
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Daniele Fargion (Università Roma 1)07/07/2016, 17:50The recent UHECR events by AUGER and TA offered wide clustering as the North and South Hot Spot possibly related to near AGN as M82 and Cen A, as well as rare narrow clustering along SS433 and in opposite side of the galactic plane multiplet events: we tag them, with a very few other sky regions, a couple of years ago. Last year highest UHE tens-hundreds TeV neutrino events did...Go to contribution page
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Dr Ralph Engel (Karlsruhe Institute of Technology (KIT))08/07/2016, 09:00Thanks to new data from LHC and fixed-target experiments and an improved understanding of the phenomenology of extensive air showers, significant progress has been made in predicting composition-relevant observables. The current status of predictions for air showers is reviewed and discussed on the basis of general features of hadronic multiparticle production. Implications for the...Go to contribution page
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Dr Anatoli Fedynitch (DESY Zeutehn)08/07/2016, 09:50
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Dr Juan Carlos Arteaga Velazquez (Universidad Michoacana)08/07/2016, 10:20KASCADE-Grande was an air-shower experiment aimed to investigate cosmic rays between 10^16 and and 10^18 eV. The instrument was located at the site of the Karlsruhe Institute of Technology, Germany at an altitude of 110 m a.s.l. and covered an area of 0.5 km^2 . KASCADE-Grande consisted of several detector systems dedicated to measure different components of the cosmic ray induced air showers,...Go to contribution page
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Mr Francisco Diogo (LIP)08/07/2016, 11:20The most energetic particles in the universe - ultra-high energy cosmic rays – interact with the atmosphere creating air showers whose charactristics are sensitive to the primary mass composition and hadronic interaction properties. Currently, these showers are our only window to test the properties of collisions at energies beyond the reach of human-made accelerators. The Pierre Auger...Go to contribution page
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Alessia Rita Tricomi (CT)08/07/2016, 11:40The goal of the LHCf experiment is to provide precise measurements of the spectra of neutral particles produced in the very forward region at LHC. These measurements are of fundamental importance since provide a calibration tool to tune the hadronic interaction models used by ground-based cosmic rays experiments up to the highest energy currently available at accelerator facilities. In order...Go to contribution page
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Dr Melania Del Santo (INAF/IASF-Palermo)Among the considerable number of studies that can be carried out using muons, we pay specific attention to the radiography of volcanoes based on the same principle of the X-ray radiography of human body. Thanks to their high penetration capability, cosmic-ray muons can be used to reconstruct the density distribution of the interior of huge structures by measuring the attenuation induced by...Go to contribution page
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Dr Giuliana Russano (University of Trento)The LISA Pathfinder geodesic explorer mission for gravitational wave astronomy has demonstrated a residual acceleration between two free falling test masses at femto-m/s^2Hz^1/2 level in the frequency range 0.7 - 20 mHz. The relative acceleration between these two objects is perturbed by the presence of a large and constant relative acceleration that must be actively compensated in order to...Go to contribution page
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emanuele fiandrini (University&Infn erugia)The Cherenkov Telescope Array (CTA) will be the next generation of ground-based observatory of very high energy gamma ray sources. The Italian Institute of Nuclear Physics (INFN) is involved in the R&D effort for the development of a possible solution for one of the Cherenkov photon camera designs, working on replacing the Hamamatsu MPPC S12642- 0404PA-50 with more UV sensitive ones from...Go to contribution page
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Dr Carmela Bonavolonta (INFN-Napoli)The development of a new camera based on the use of Silicon Photomultipliers (SiPM) proposed for the Cherenkov Telescope Array (CTA), which represents a new generation of ground based very high energy gamma ray observatory, is one of the main items of the Italian Institute of Nuclear Physics (INFN). In the R&D framework a single channel electronic charge preamplifier has been developed to...Go to contribution page
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Daniela Simone (BA)The Italian Institute of Nuclear Physics (INFN) is involved in the development of a prototype for a SiPM-based camera for the Cherenkov Telescope Array (CTA), a new generation of telescopes for ground – based gamma ray astronomy. In this framework, an R&D program within the ‘Progetto Premiale TElescopi CHErenkov made in Italy (TECHE.it)’ for the development of SiPMs suitable for Cherenkov...Go to contribution page
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Dr Stefano Grazzi (Study and Research Centre “Enrico Fermi” (Rome))The Extreme Energy Events Project is an extended array for Cosmic Rays survey, conceived by Antonino Zichichi and supported by the Study and Research Centre “Enrico Fermi” (Rome) with the collaboration of the European Organization for Nuclear Research (CERN), of the Italian National Institute of Nuclear Physics (INFN) and of the Italian Ministry of Education, University and Research (MIUR)....Go to contribution page
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Dr VALENTINA SCOTTI (ROMA2)EUSO-TA is one of the prototypes of the JEM-EUSO space telescope, realized in the framework of the EUSO project. Its aims are to calibrate the detector response, test its performance in air and space, raise the technological readiness level of some of the components and improve our knowledge of the various detector systems. EUSO-TA is located at the Telescope Array (TA) site in Black Rock...Go to contribution page
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Roberta Sparvoli (ROMA2)CSES (China Seismo-Electromagnetic Satellite) is a space scientific mission dedicated to monitoring electromagnetic field, plasma and particles perturbations in the atmosphere, ionosphere and magnetosphere induced by natural sources and anthropocentric emitters. CSES, made by a Chinese-Italian collaboration, is scheduled to be launched in the first half of 2017 and has an expected lifetime...Go to contribution page
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Francesco Giordano (BA)In recent years, Silicon Photomultipliers (SiPMs) have proven to be very performing devices, especially for those applications where high sentivity to low intensity light and fast responses are required. A SiPM consists of a system of hundreds or even thousands of p-n junctions connected in parallel and operating in Geiger mode. We performed a very detailed modeling of several devices from...Go to contribution page
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Andrea Lavagno (TO)We study the spectrum of high energy cosmic rays as an ultra-relativistic multicomponent quasi-ideal plasma. Such a quasi-ideal plasma reflects a power-law behavior reproducing the knee-ankle structure of the high and ultra high energy spectrum. The presence of nonextensive statistical effects are discussed in the light of the recent data and in connection with anomalous sub-diffusive...Go to contribution page
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Dr Tristano Di Girolamo (Universita` di Napoli "Federico II")The Large Area Telescope (LAT) on the Fermi gamma-ray satellite telescope observes Gamma-Ray Bursts (GRBs) at energies above 100 MeV. Thanks to a new detection algorithm and a new event reconstruction, it is expected to publish a catalogue with more than 100 GRBs. This work aims at revising the prospects for GRB alerts with the Cherenkov Telescope Array (CTA) based on the new LAT results. We...Go to contribution page
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Dr Beatrice Panico (NA)The High-Energy Particle Detector (HEPD) is one of the payloads of the CSES space mission. The CSES (China Seismo-Electromagnetic Satellite) mission will investigate the structure and the dynamic of the topside ionosphere, will monitor electric and magnetic field and high energy particle fluctuations, searching for their correlations with the geophysical activity, in order to contribute to the...Go to contribution page
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Dr VALENTINA SCOTTI (ROMA2)The China Seismo Electromagnetic Satellite (CSES) aims to contribute to the monitoring of earthquakes from space. This space mission, lead by a Chinese-Italian collaboration, will study phenomena of electromagnetic nature and their correlation with the geophysical activity. The satellite will be launched in 2016 and will host several instruments onboard: two magnetometers, an electrical field...Go to contribution page
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Mr Mihai Niculescu-Oglinzanu (IFIN-HH)The measurements of the flux and the trajectory of cosmic muons are performed using a detector based on plastic scintillators, optical fibers (wavelength shifters) and readout by SiPM(MPPC-Multi Pixel Photon Counter) devices. The Detector is consisting of a stack of 6 active modules, grouped in 3 layers for determining the muon trajectories through 3 planes. One module has 24 plastic...Go to contribution page
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Julio Arturo Rabanal Reina (LAL/IN2P3/CNRS)The JEM-EUSO (Extreme Universe Space Observatory on Japanese Experiment Module) experiment is about a space telescope that will be installed on the ISS in 2020. The UHECR study aims to improve by a factor of 100 the current measures of Pierre-Auger observatory. The telescope EUSO-Balloon, which was technologically validated in 2014 was the first prototype with the whole chain of...Go to contribution page
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