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VLVnT 2018

1–4 Oct 2018
International Conference Center
Europe/Moscow timezone

Contribution List

143 / 143
8. Opening
02/10/2018, 08:00
9. GNN Diss Prize & Talk
02/10/2018, 08:10
10. Overview IceCube Physics Results
Ignacio Taboada
02/10/2018, 08:25
11. TXS (1)
Anna Franckowiak (DESY)
02/10/2018, 08:48
12. TXS (2)
Chad Finley (Stockholm University)
02/10/2018, 09:06
13. Overview Antares Physics Results
Prof. Antoine Kouchner (APC)
02/10/2018, 09:25
14. Phenomenology of blazars and neutrinos and the 0922 event
Anatoli Fedynitch (DESY)
02/10/2018, 10:20
15. Candidates for Galactic HE neutrino sources
Michael Kachelriess (NTNU)
02/10/2018, 10:50
16. Gravitational Waves and neutrinos
Chad Finley (Stockholm University)
02/10/2018, 11:20
22. Antares TXS results
Giulia Illuminati (Instituto de Física Corpuscular)
02/10/2018, 13:30
32. Investigation of ν properties with the νGEN spectrometer
Dr Alexey Lubashevskiy (JINR)
02/10/2018, 13:30
27. KM3NeT technology transfer
Kostas Pikounis
02/10/2018, 13:30
33. Direct Dark Matter searches: overview
Dr Evgeny Yakushev (JINR)
02/10/2018, 13:50
23. Dissection of the area around IceCube - 170922A
Mr Theo Glauch (Technical University of Munich)
02/10/2018, 13:50
28. GVD optical module and other mechanics: experience and progress
Alexandr Doroshenko (INR RAS)
02/10/2018, 13:50
24. Blazar flare analysis using light curves IceCube
Christoph Raab (ULB)
02/10/2018, 14:10
29. Test of 3.5’’ PMTs from Hama & HZC
Lew Classen (University of Muenster)
02/10/2018, 14:10
34. Indirect dark matter searches
Juan Aguilar Sánchez (Université Libre de Bruxelles (ULB))
02/10/2018, 14:15
25. HESE results IceCube
Juliana Stachurska (DESY Zeuthen)
02/10/2018, 14:30
30. MELTS program for PMTs
MELTS speaker
02/10/2018, 14:30
35. Combined dark matter Antares/IceCube
Sara Rebecca Gozzini (IFIC)
02/10/2018, 14:40
26. HESE with ARCA
Konstantinos Pikounis (NCSR Demokritos)
02/10/2018, 14:50
31. Talk on the GVD cable
Company speaker
02/10/2018, 14:50
36. Monopole searches: overview
Christian Spiering
02/10/2018, 14:55
37. Search for particles beyond the Standard Model with the proposed SHiP experiment at CERN
Prof. Roumen Tsenov (LHEP JINR)
02/10/2018, 15:05
45. KM3NeT DOM
Dr Ronald Bruijn (University of Amsterdam and Nikhef)
02/10/2018, 15:50
50. NMO: Status and JUNO plans
Prof. Alexander Olshevskiy (JINR)
02/10/2018, 15:50
38. Tau analysis IceCube
Prof. Donglian Xu (Shanghai Jiao Tong University)
02/10/2018, 15:50
40. Neutrino / UHECR correlation analysis
Ms Lisa Schumacher (RWTH Aachen)
02/10/2018, 16:08
51. Particle Physics with ORCA (oscill./steriles/DM)
Ms Alba Domi (Università degli Studi di Genova, INFN-Genova, CPPM-Marseille)
02/10/2018, 16:10
46. The new Central Logic Board for KM3NeT
Mr David Calvo (IFIC)
02/10/2018, 16:10
41. Constraints on UHECR sources with 9 years of IceCube EHE data
Prof. Aya Ishihara (Chiba University)
02/10/2018, 16:26
47. mDOM for IceCube
Alexander Kappes (University Muenster)
02/10/2018, 16:30
52. Oscillations with IceCube upgrade
Dr Joshua Hignight (Dr.)
02/10/2018, 16:30
42. Combined point source
Giulia Illuminati
02/10/2018, 16:44
48. DEgg for IceCube
Yuya Makino (Chiba University)
02/10/2018, 16:50
54. Sterile neutrinos: Overview
Dr Dmitry Naumov (JINR)
02/10/2018, 16:50
43. Combined Galactic Plane
Mr Christian Haack (RWTH Aachen University)
02/10/2018, 17:02
55. Sterile neutrinos: IceCube results
Dr Joshua Hignight (Dr.)
02/10/2018, 17:10
49. WOM status
Peter Peiffer
02/10/2018, 17:10
44. GVD: results of track reconstruction
Mr Grigory Safronov (JINR)
02/10/2018, 17:20
56. Sterile neutrinos: Latest results from reactors with focus on DANSS results
Viacheslav Egorov (JINR)
02/10/2018, 17:20
57. Dubna program overview
Prof. Dmitry Naumov (DLNP JINR)
03/10/2018, 08:00
58. Results HE Gamma Rays
Elisa Püschel
03/10/2018, 08:20
59. Results Fermi/X - rays
Anna Franckowiak (DESY)
03/10/2018, 08:50
60. UHECR results
Maxim Pshirkov (Lomonosov Moscow State University, SAI)
03/10/2018, 09:20
65. Status GVD
Dr Vladimir Aynutdinov (INR RAS)
03/10/2018, 10:20
66. Status ARCA/ORCA
Paschal Coyle (Centre de Physique des particules de Marseille)
03/10/2018, 10:45
67. Physics ORCA - Protvino
Jürgen Brunner (CPPM)
03/10/2018, 11:10
68. NuProgram Protvino
Prof. Alexandre Zaitsev (IHEP NRC KI)
03/10/2018, 11:35
94. Earth Tomography
Véronique Van Elewyck (APC, Université Paris Diderot)
03/10/2018, 13:20
83. GVD: results of cascade reconstruction
Prof. Zhan-Arys Dzhilkibaev (Institute for nuclear research)
03/10/2018, 13:20
88. Time calibration in KM3NeT
Dr Irene Di Palma (University of Rome Sapienza and INFN)
03/10/2018, 13:20
95. Environmental studies in Lake Baikal - basic facts and perspectives for interdisciplinary research
Nikolai Budnev (Irkutsk State University)
03/10/2018, 13:38
84. Improving the angular reconstruction of muon tracks in ice
Mrs Federica Bradascio (DESY)
03/10/2018, 13:40
89. Nanobeacon: A time calibration device for KM3NeT
Mr David Calvo (IFIC)
03/10/2018, 13:40
85. Improving directional reconstruction of hadronic cascades
Mr Christian Haack (RWTH Aachen University)
03/10/2018, 14:00
90. Time calibration in GVD
Mark Shelepov (INR)
03/10/2018, 14:00
96. GVD results
Rastilav Dvornitsky (JINR)
03/10/2018, 14:01
97. Italian Site
Antonino Capone (Physics Department University “La Sapienza” and INFN, Roma, Italy)
03/10/2018, 14:19
91. Spatial positioning of underwater components for Baikal-GVD
Mr Alexander Avrorin (INR RAS)
03/10/2018, 14:20
86. Supernova MEV neutrinos with KM3NeT
Marta Colomer Molla (APC/IFIC)
03/10/2018, 14:20
98. French site (Albatross, MII)
Dr Dominique Lefevre (CNRS MIO)
03/10/2018, 14:37
87. Carpet results
Prof. Sergey Troitsky (INR, Moscow)
03/10/2018, 14:40
92. Compact solid - state pulsed laser for calibration of the GVD data acquisition system
Alexander Shestyakov
03/10/2018, 14:40
99. Environmental studies at Canadian site
Elisa Resconi (TU Munich)
03/10/2018, 15:00
93. White Rabbit etc. from by “sevensolutions”
Pablo Marín Jímenez
03/10/2018, 15:00
100. AMON report
Mr James DeLaunay (Penn State)
03/10/2018, 15:50
110. KM3NeT: software defined networks for DAQ, data transmission and processing
Dr Tommaso Chiarusi (INFN-Sezione di Bologna)
03/10/2018, 15:50
105. NEVOD as test facility for future neutrino telescopes
Anatoly Petrukhin (MEPhI)
03/10/2018, 15:50
111. KM 3NeT: Readout and triggering
Dr Ronald Bruijn (University of Amsterdam and Nikhef)
03/10/2018, 16:10
106. POCAM in GVD and STRAW in Canada
Mr Felix Henningsen (TUM)
03/10/2018, 16:10
101. Zwicky Transient Facility ZTF
Dr Ludwig Rauch (DESY)
03/10/2018, 16:10
102. Antares results and plans MM
Bruny Baret (APC-CNRS)
03/10/2018, 16:30
107. Data processing and quality monitoring of Baikal - GVD
Evgeny Khramov (JINR)
03/10/2018, 16:30
112. KM3NeT: Acquisition control
Dr Cristiano Bozza (University of Salerno and INFN Gruppo Collegato di Salerno)
03/10/2018, 16:30
113. Computing in the KM3NeT Research Infrastructure
Jannik Hofestaedt (ECAP, Uni Erlangen-Nürnberg)
03/10/2018, 16:50
103. IceCube results and plans MM
Anna Franckowiak (DESY)
03/10/2018, 16:50
108. Moon shadow in Antares
Dr Tommaso Chiarusi (INFN-Sezione di Bologna)
03/10/2018, 16:50
114. ASTERICS
Dr Bernardino Spisso (INFN)
03/10/2018, 17:10
104. GVD results and plans MM
Prof. Zhan-Arys Dzhilkibaev (Institute for nuclear research)
03/10/2018, 17:10
109. Positioning calibration in KM3NeT
Mr Konstantinos Pikounis (NCSR Demokritos)
03/10/2018, 17:10
74. Antares & GW
Bruny Baret (APC-CNRS)
04/10/2018, 08:00
79. IceCube: Deconvolution
Dr Tim Ruhe (TU Dortmund)
04/10/2018, 08:00
75. TAIGA results and perspectives
Dr Leonid Kuzmichev (SINP)
04/10/2018, 08:20
80. KM3NeT: Machine Learning
Dr Chiara De Sio (INFN)
04/10/2018, 08:25
76. LHHASO plans and capabilities
Yuri Stenkin (INR RAS)
04/10/2018, 08:40
81. IceCube: Machine Learning
Mirco Huennefeld (TU Dortmund)
04/10/2018, 08:50
77. FACT/C - Ring “around the world”
Dr Tim Ruhe (TU Dortmund)
04/10/2018, 09:00
82. BIG DATA IN ASTROPARTICLE PHYSICS: A DISTRIBUTED DATA STORAGE; INTELLECTUAL DATA ANALYSIS
Dr Alexander Kryukov (SINP MSU)
04/10/2018, 09:15
78. Radio detection in the multi-messenger context
Dmitriy Kostunin (Karlsruhe Institute of Technology (KIT))
04/10/2018, 09:20
69. Status IC - Upgrade/Gen2
Marek Kowalski (DESY and Humboldt-University)
04/10/2018, 10:10
70. Summary 1
Alexander Kappes (University Muenster)
04/10/2018, 10:30
71. Bringing things together
Christian Spiering
04/10/2018, 10:45
72. Summary Particle Physics with NTs
Jannik Hofestädt (ECAP, Uni Erlangen-Nürnberg)
04/10/2018, 11:00
73. Round Table and Closeout
Prof. Uli Katz (ECAP / Univ. Erlangen)
04/10/2018, 11:15
126. A Cherenkov Telescope Ring for Monitoring and Follow-Up Observations
Tim Ruhe (TU Dortmund)
The new era of multi-messenger astronomy and the vast discovery potential of future detectors mandate already now the development of capabilities for continuous all-sky observations in the photon channel. For the very high energy gamma-ray regime, this could efficiently be achieved with a globe-spanning network of medium sized imaging air Cherenkov telescopes. In this talk, we present the...
133. Analysis of high energy starting events with the KM3NeT/ARCA detector
Konstantinos Pikounis (NCSR Demokritos)
KM3NeT is a research infrastructure housing the next generation neutrino detectors in the depths of the Mediterranean Sea. The ARCA detector, which is currently under construction, is optimized for searches for neutrinos from astrophysical sources as well as measurements of the diffuse high energy astrophysical flux. The unambiguous detection of neutrinos of extraterrestrial origin by IceCube...
5. Candidates for Galactic HE neutrino sources
Michael Kachelriess
123. Cherenkov water detector NEVOD as a facility for calibration of various OMs
Anatoly Petrukhin (MEPhI)
NEVOD is the first in the world Cherenkov water detector (CWD) at the Earth’s surface equipped with a spatial lattice of quasi-spherical measuring modules for the investigations of all basic components of cosmic rays including neutrinos. A large dynamic diapason and close location of quasispherical modules allows use this detector as a Cherenkov water calorimeter for cascade shower...
120. D-Egg: The next-generation optical module for the deep in-ice neutrino detector
Yuya Makino (Chiba University)
The next-generation optical module for such detector extension is expected to have improved detection efficiency for Cherenkov photons over the current IceCube optical module. Furthermore, it is also anticipated that additional information possibly provided by new sensors, such as positions of the Cherenkov photons at each optical sensors, will lead to advances in event reconstructions. The...
125. Dark matter searches with IceCube
Juan Antonio Aguilar Sanchez (Université Libre de Bruxelles (ULB))
The nature of dark matter remains one of the most enduring unsolved questions in modern cosmology. In order to decipher the mystery of dark matter and understand its properties different experimental avenues are explored. Indirect searches make use of the annihilation or decay products of dark matter as traces to prove its existence. This strategy is complementary of direct detection as...
141. Deconvolution Algorithms in IceCube
Tim Ruhe (TU Dortmund)
Since the energy of an incident neutrino is inherently unknown, it has to be inferred from energy-dependent quantities, e.g. the energy loss of secondary particles. The production of secondary particles, however, is a stochastic process, which poses certain challenges for the reconstruction of neutrino energy spectra, which is further made difficult by a limited acceptance and smearing effects...
18. Direct Dark Matter searches: overview
Evgeny Yakushev Yakushev
127. Galactic neutrinos
Michael Kachelriess (NTNU)
I review possible Galactic neutrino sources and the resulting signatures. In particular, I discuss options leading to neutrino arrival directions which are extended over a much larger solid angle than the Galactic plane. Finally, I argue that the photons accompanying the Galactic neutrino signal are already seen in the Fermi-LAT data.
139. Gamma-ray lightcurve correlation searches for IceCube neutrinos from blazar flares
Christoph Raab (Université libre de Bruxelles)
Blazars have long been considered as accelerator candidates for cosmic rays. In such a scenario, hadronic interactions in their jet would produce neutrinos and gamma-rays. Correlating the astrophysical neutrinos detected by IceCube, a cubic-kilometre neutrino telescope at the South Pole, with the gamma-ray emission from blazars could therefore reveal the origin of cosmic rays. In our method we...
6. Gravitational Waves and neutrinos
Imre Bartos
137. IceCube high energy starting events at 7.5 years - new measurements of flux and flavor
Juliana Stachurska (DESY Zeuthen)
The IceCube Neutrino Observatory at the South Pole, which detects Cherenkov light from charged particles produced in neutrino interactions, firmly established the existence of an astrophysical high-energy neutrino component. In this talk I will present IceCube\'s High-Energy Starting Event sample, the updates made and the new results obtained with a livetime of 7 years. I will focus on...
136. Improving the directional reconstruction of PeV hadronic cascades in IceCube
Mr Christian Haack (RWTH Aachen University)
Many neutrino interactions measured by the IceCube Neutrino Observatory produce only hadronic showers, which appear as almost point-like light emission due to the large detector spacing (~125m). At PeV energies these showers often saturate the PMTs closest to the interaction vertex - thus the reconstruction has to rely on more diffused photons which requires precise understanding of the...
138. Improving the muon track reconstruction of IceCube and IceCube-Gen2
Federica Bradascio (DESY Zeuthen)
IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. It aims at detecting astrophysical neutrinos and identifying their sources. High-energy muon neutrinos are identified through the muons produced in the interactions with the ice. The muon tracks are reconstructed using a maximum likelihood method, which models the arrival times of Cherenkov photons registered by the...
19. Indirect dark matter searches
Juanan Aguilar
17. Investigation of ν properties with the νGEN spectrometer
Alexey Lubashevskiy
130. KM3NeT Acquisition Control
Dr Cristiano Bozza (University of Salerno and INFN Gruppo Collegato di Salerno)
The multi-site nature of the KM3NeT collaboration has influenced the development and evolution of its Acquisition Control software. It is flexible and portable to the extent that the same programs are used in data-taking shore station of neutrino telescopes as well as in the test and qualification sites for performance and quality assessment of detector components at different stages of the...
143. KM3NeT Acquisition Control
Dr Cristiano Bozza (University of Salerno and INFN Gruppo Collegato di Salerno)
The multi-site nature of the KM3NeT project has influenced the development and evolution of its acquisition control software so that it doesn’t stick to a single detector site or configuration. It is flexible and portable to the extent that the same programs are used in data-taking shore station of neutrino telescopes as well as in testing sites for detector components at...
134. KM3NeT Technology Transfer
Konstantinos Pikounis (NCSR Demokritos)
The status of the construction of the KM3NeT detector components and the experience gained from the detector units deployed underpin the presentation of technological solutions developed or modified by KM3NeT to industry, Institutions and other stakeholders with potential interest. KM3NeT has now entered a phase during which the design of the detector elements is finalized and the methods...
142. KM3NeT: Machine Learning
Dr Chiara De Sio (INFN)
The KM3NeT Collaboration is building a network of underwater Cherenkov telescopes at two sites in the Mediterranean sea, with the main goal of investigating astrophysical sources of high-energy neutrinos (ARCA) and of determining the neutrino mass hierarchy (ORCA). Various Machine Learning techniques, such as Random Forests, BDTs, Shallow and Deep Networks are being used for diverse tasks,...
122. LHAASO Status and Perspectives
Yuri Stenkin (INR RAS)
LHAASO physics and current status will be presented
20. Monopole searches: overview
Christian Spiering
135. Multimessenger Astrophysics with AMON: Current and Future Alerts
James DeLaunay (Penn State)
The Astrophysical Multimessenger Observatory Network (AMON) is connecting observatories around the world in order to enable real-time coincidence searches across all four astrophysical messengers: neutrinos, cosmic rays, photons, and gravitational waves. AMON analyses deliberately extend into the \"sub-threshold\" regimes of these experiments, and are conceived so as to enable near...
39. Neutrino / UHECR correlation analysis
Lisa Schumacher
119. Neutrino astrophysics and IceCube
Ignacio Taboada (Georgia Institute of Technology)
Cosmic rays and neutrinos are intimately related. And though TeV-PeV astrophysical neutrinos have been observed, their sources and their relation to potential sources of cosmic rays remain largely unknown. IceCube has conducted numerous searches for potential neutrino sources. This talk is an overview that complements other presentations at this conference. I will describe the...
64. NuProgram Protvino
Alexandre Zaitsev
118. Oscillation Physics with Deepcore and the IceCube Upgrade
Dr Joshua Hignight (Dr.)
The IceCube neutrino observitory is a cubic km neutrino telescope located at the South Pole. DeepCore is an infill array of the IceCube Neutrino Observatory and enables observations of atmospheric neutrinos with energies as low as 5 GeV. Atmospheric neutrinos from 5-50 GeV allow for a broad range of particle physics, from measuring standard neutrino oscillations to probing BSM physics. In...
3. Overview Antares Physics Results
Antoine Kouchner
0. Overview IceCube Physics Results
Ignacio Taboada
4. Phenomenology of blazars and neutrinos and the 0922 event
Anatoly Fedynitch
63. Physics ORCA - Protvino
Jürgen Brunner
140. PMT characterization for the multi-PMT Digital Optical Module
Lew Classen (University of Muenster)
Optical modules are the \"eyes\" of neutrino telescopes, detecting the Cherenkov light from charged particles created in neutrino interactions in the surrounding medium. In the framework of a planned upgrade of the current IceCube Neutrino Observatory as well as a future next-generation neutrino telescope at the South Pole, new optical modules are being developed which are expected...
129. Prospectes on CCSN neutrino detection with KM3NeT
Marta Colomer Molla (APC/IFIC)
Core Collapse Supernovae (CCSN) are explosive phenomena that may occur at the end of the life of massive stars, releasing over 99% of the energy through emission of neutrinos with energies on the 10 MeV scale. While the explosion mechanics is not fully understood, neutrinos are believed to play an important role in it. The only detection as of today, marking the beginning of extrasolar...
121. Recent highlights from very-high-energy gamma-ray instruments
Elisa Pueschel (Deutsches Elektronen-Synchrotron)
The very-high-energy gamma-ray sky grows ever more populated, with over 200 sources. The current-generation imaging atmospheric Cherenkov telescope arrays, VERITAS, H.E.S.S. and MAGIC, have collected over a decade of observations covering an energy range from tens of GeV to tens of TeV, while HAWC has collected several years of survey observations in the TeV to 100 TeV energy range. These...
128. Recent results from the ANTARES neutrino telescope
Antoine Kouchner (University Paris Diderot -- APC)
ANTARES, the largest underwater neutrino telescope, has been continuously operating since 2007 in the Mediterranean Sea. The transparency of the water allows for a very good angular resolution in the reconstruction of neutrino events of all flavors. This results in an unmatched sensitivity for neutrino source searches, in a large fraction of the Southern Sky at TeV energies. As a consequence,...
132. Reconstruction Techniques in IceCube using Convolutional and Generative Neural Networks
Mirco Huennefeld (TU Dortmund)
A key challenge to the success of high-energy physics experiments such as IceCube is the reliable and accurate reconstruction of events. In IceCube, further challenges arise as the detector is situated at the geographic South Pole where resources are limited. However, to perform real-time analyses and to issue alerts to telescopes around the world, powerful reconstruction methods are desired....
115. Report on the Asterics projects CORELib and ROAst
Dr Bernardino Spisso (INFN)
In this talk will be introduced the Asteriscs program and presented the status of two Asterics projects: CORElib and ROAst. CORELib (Cosmic Ray Event Library) is a collection of simulations based on CORSIKA featuring a common set of physical parameters in order to achieve a common high statistics production. Will be discussed the pilot production, the framework used to achieve this...
131. Search for correlations of high-energy neutrinos and ultra-high-energy cosmic rays
Ms Lisa Schumacher (RWTH Aachen)
The IceCube Neutrino Observatory has recently found compelling evidence for a particular blazar producing high-energy neutrinos and PeV cosmic rays, however the sources of cosmic rays above several EeV remain unidentified. It is believed that the same environments that accelerate ultra-high-energy cosmic rays (UHECRs) also produce high-energy neutrinos via hadronic interactions of lower-energy...
21. Search for particles beyond the Standard Model with the proposed SHiP experiment at CERN
Roumen Tsenov
62. Status ARCA/ORCA
Paschal Coyle
61. Status GVD
Vladimir Aynutdinov
124. The blazar TXS 0506+056 as possible neutrino counterpart
Anna Franckowiak (DESY)
On September 22, 2017, the IceCube Neutrino Observatory observed for the first time ever an extremely high-energy neutrino IceCube-170922A in spatial and temporal coincidence with a gamma-ray flaring blazar, TXS 0506+056. Following the original IceCube alert, the source has been observed by several telescopes in a broad wavelength band. Most notably the Fermi Large Area Telescope has reported...
144. The KM3NeT Multi-PMT DOM and Detection Unit
Ronald Bruijn (University of Amsterdam and Nikhef)
The KM3NeT Collaboration is constructing new-generation neutrino detectors in the Mediterranean Sea. The main goals are the study of the high-energy neutrino flux (KM3NeT/ARCA, off-shore Capo-Passero, Italy) and the determination of the neutrino mass ordering (KM3NeT/ORCA, off-shore Toulon, France). The basic detection element, the Digital Optical Module (DOM), houses 31 three-inch PMT’s...
117. The multi-PMT optical module for the IceCube-Upgrade
Alexander Kappes (University Muenster)
Following the first observation of an astrophysical high-energy neutrino flux with the IceCube Neutrino Observatory in 2013, planning for an upgrade of the detector are progressing, which will expand the capabilities of the detector at low neutrino energies and allow to determine IceCube detector systematics with significantly improved precision. A substantial contribution to the improved...
116. The new CLBv4 for the KM3NeT neutrino telescope
David Calvo (IFIC)
The KM3NeT collaboration aims at the construction of a multi-km3 high-energy neutrino telescope in the Mediterranean Sea consisting of thousands of glass spheres, the so called Digital Optical Module (DOM), each of them containing 31 photomultipliers of small photocathode area for the detection of the Cherenkov light induced by charged particles produced by the interaction of neutrinos with...
1. TXS (1)
Anna Franckowiak
2. TXS (2)
Chad Finley
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