1. A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger ObservatoryMarko Zavrtanik, Lukas Zehrer, Danilo Zavrtanik, Serguei Vorobiov, Marta Trini, Samo Stanič, Gašper Kukec Mezek, Andrej Filipčič, A. Aab, 2020, original scientific article Found in: ključnih besedah
Keywords: ultra-high energy neutrinos, blazar TXS 0506+056, the Pierre Auger Observatory, high-energy astrophysics, neutrino astronomy, blazars, transient sources, active galaxies
Published: 20.10.2020; Views: 2310; Downloads: 0
 Fulltext (696,03 KB) |
2. Update of the neutrino and photon limits from the Pierre Auger ObservatoryMarko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, Carla Bleve, 2015, published scientific conference contribution Abstract: Ultra-high energy neutrinos and photons, with energies above
1 EeV and 10 EeV respectively, can be detected with the Surface
Detector array (SD) of the Pierre Auger Observatory. Downward-
going neutrinos of all flavours interacting in the atmosphere
at zenith angles θ > 60◦, upward-going tau neutrinos (“Earth-
skimming”), as well as photons in the zenith range 30◦ − 60◦
can be identified through the broad time-structure of the
signals expected to be induced in the SD stations. An
additional signature for photon-induced air showers is the
steeper lateral distribution of secondary particles at ground
with respect to the nucleonic showers. Stringent limits are set
to the diffuse flux of ultra-high energy (UHE) neutrinos and
photons, using data collected between 2004 and mid-2013, under
the hypothesis of an E[sup]−2 spectrum for signal primaries.
Found in: ključnih besedah
Summary of found: ...Ultra-high energy neutrinos and photons, with energies above
1 EeV...
Keywords: ultra-high energy neutrinos, ultra-high energy photons, cosmic rays, elemental composition, Pierre Auger Observatory
Published: 03.03.2016; Views: 4066; Downloads: 223
Fulltext (398,21 KB) |
3. Search for a correlation between the UHECRs measured by the Pierre Auger Observatory and the Telescope Array and the neutrino candidate events from IceCubeMarko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, Asen Christov, 2015, published scientific conference contribution Abstract: We have conducted three searches for correlations between
ultra-high energy cosmic rays detected by the Telescope Array
and the Pierre Auger Observatory, and high-energy neutrino
candidate events from IceCube. Two cross-correlation analyses
with UHECRs are done: one with 39 cascades from the IceCube
‘high-energy starting events’ sample and the other with 16
high-energy ‘track events’. The angular separation between the
arrival directions of neutrinos and UHECRs is scanned over.
The same events are also used in a separate search using a
maximum likelihood approach, after the neutrino arrival
directions are stacked. To estimate the significance we assume
UHECR magnetic deflections to be inversely proportional to
their energy, with values 3◦, 6◦ and 9◦ at 100 EeV to allow for
the uncertainties on the magnetic field strength and UHECR
charge. A similar analysis is performed on stacked UHECR
arrival directions and the IceCube sample of through-going
muon track events which were optimized for neutrino point-
source searches.
Found in: ključnih besedah
Summary of found: ...The angular separation between the
arrival directions of neutrinos and UHECRs is scanned over.
The same...
Keywords: ultra-high energy cosmic rays, Pierre Auger Observatory, Telescope Array, high-energy neutrinos, IceCube, correlation search
Published: 08.03.2016; Views: 4157; Downloads: 187
Fulltext (1,11 MB) |
4. Improved limits to point-like sources of ultrahigh energy neutrinos with the Pierre Auger ObservatoryLili Yang, Marta Trini, Pablo Pieroni, Jaime Alvarez-Muniz, 2016, treatise, preliminary study, study Found in: ključnih besedah
Keywords: ultrahigh energy neutrinos, Pierre Auger Observatory, surface detector
Published: 07.04.2016; Views: 4446; Downloads: 0
Fulltext (307,54 KB) |
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6. Neutrino events at IceCube and the Fermi bubblesLili Yang, Cecilia Lunardini, Soebur Razzaque, Kristopher T. Theodoseau, 2014, original scientific article Found in: ključnih besedah
Summary of found: ... neutrinos, Fermi bubbles, IceCube, ...
Keywords: neutrinos, Fermi bubbles, IceCube
Published: 09.05.2017; Views: 3529; Downloads: 102
 Fulltext (0,00 KB) |
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8. Towards a Joint Analysis of Data from the IceCube Neutrino Telescope, the Pierre Auger Observatory and Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Serguei Vorobiov, Darko Veberič, Samo Stanič, Ahmed Saleh, Andrej Filipčič, A. Christov, 2016, published scientific conference contribution Found in: ključnih besedah
Summary of found: ...(UHECR),
Pierre Auger Observatory,
Telescope Array,
very-high energy (VHE) neutrinos,
IceCube Neutrino Telescope,
joint data analysis...
Keywords: ultra-high energy cosmic rays (UHECR), Pierre Auger Observatory, Telescope Array, very-high energy (VHE) neutrinos, IceCube Neutrino Telescope, joint data analysis
Published: 08.11.2016; Views: 4349; Downloads: 0
Fulltext (455,27 KB) |
9. Ultrahigh energy neutrino follow-up of Gravitational Wave Event GW150914 with the Pierre Auger ObservatoryMarta Trini, Pablo Pieroni, Zlatka Zas, Francisco Pedreira, Jaime Alvarez-Muňiz, Lili Yang, treatise, preliminary study, study Found in: ključnih besedah
Summary of found: ...UHE neutrinos, SD detector, Gravitational Waves...
Keywords: UHE neutrinos, SD detector, Gravitational Waves
Published: 29.11.2016; Views: 4588; Downloads: 0
Fulltext (881,65 KB) |
10. Multi-messenger study of the Fermi BubblesLili Yang, invited lecture at foreign university Abstract: The Fermi Bubbles have been imaged in sub-TeV gamma rays at Fermi-LAT, and, if their origin is hadronic, they might have been seen with low statistics in ∼0.1−1 PeV neutrinos at IceCube. I discuss the detectability of these objects at the new High Altitude Water Cherenkov (HAWC). HAWC will view the North Bubble for ∼2−3 hours a day, and will map its spectrum at 0.1-100 TeV. For the hard primary proton spectrum required to explain five events at IceCube, a high significance detection at HAWC will be achieved in less than 30 days. I will discuss how the combination of results at HAWC and IceCube will substantiate the hadronic model, or constrain its spectral parameters and how sensitive Cherenkov Telescope Array(CTA) is to the bubbles.
Found in: ključnih besedah
Summary of found: ...seen with low statistics in ∼0.1−1 PeV neutrinos at IceCube. I discuss the detectability of...
Keywords: Fermi Bubbles, neutrinos, HAWC
Published: 06.12.2016; Views: 4204; Downloads: 0
Fulltext (5,54 MB)
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