11. Evidence for a mixed mass composition at the ‘ankle’ in the cosmic-ray spectrumMarko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, A. Aab, 2016, original scientific article Found in: ključnih besedah Summary of found: ...ultra-high energy cosmic rays ( UHECR),
UHECR mass composition,
UHECR energy spectrum,
Pierre Auger Observatory,
compositi... Keywords: ultra-high energy cosmic rays (UHECR), UHECR mass composition, UHECR energy spectrum, Pierre Auger Observatory, composition studies at the ‘ankle’ region in the UHECR spectrum Published: 25.11.2016; Views: 3534; Downloads: 156
Fulltext (1,73 MB) |
12. Recent results from the Pierre Auger ObservatorySerguei Vorobiov, published scientific conference contribution abstract (invited lecture) Abstract: Invited lecture at the Workshop on Perspectives on the
Extragalactic Frontier: from Astrophysics to Fundamental
Physics (May 2-6, 2016, ICTP, Trieste, Italy) Found in: ključnih besedah Summary of found: ...Ultra-high energy cosmic rays ( UHECR),
Pierre Auger Observatory,
Auger upgrade AugerPrime,
invited lecture... Keywords: Ultra-high energy cosmic rays (UHECR), Pierre Auger Observatory, Auger upgrade AugerPrime, invited lecture Published: 09.12.2016; Views: 3580; Downloads: 0
Fulltext (7,65 MB) |
13. Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatoryMarko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, A. Aab, 2017, original scientific article Found in: ključnih besedah Summary of found: ...Pierre Auger Observatory, ultra-high energy cosmic rays ( UHECR),
extensive air showers (EAS), EAS muon content,
Auger... Keywords: Pierre Auger Observatory, ultra-high energy cosmic rays (UHECR), extensive air showers (EAS), EAS muon content, Auger Muons and Infill for the Ground Array (AMIGA), scintillation modules for muon counting, silicon photomultipliers (SiPM) Published: 08.03.2017; Views: 3170; Downloads: 1
Fulltext (1,12 MB) |
14. Auger HighlightsMarko Zavrtanik, Danilo Zavrtanik, Darko Veberič, Samo Stanič, Andrej Filipčič, Antonella Castellina, Gašper Kukec Mezek, Ahmed Saleh, Marta Trini, Serguei Vorobiov, Lili Yang, 2014, published scientific conference contribution Found in: ključnih besedah Summary of found: ...Pierre Auger Observatory,
ultra high energy cosmic rays ( UHECR),
UHECR hybrid detection technique,
UHECR energy spectrum,
UHECR mass... Keywords: Pierre Auger Observatory, ultra high energy cosmic rays (UHECR), UHECR hybrid detection technique, UHECR energy spectrum, UHECR mass composition, UHECR arrival directions Published: 20.06.2017; Views: 3384; Downloads: 302
Fulltext (861,47 KB) |
15. Astroparticles at the High Energy Frontier: Results from the Pierre Auger ObservatoryMarko Zavrtanik, Danilo Zavrtanik, Serguei Vorobiov, Darko Veberič, Samo Stanič, Ahmed Saleh, Andrej Filipčič, Gonzalo Parente, 2014, published scientific conference contribution Found in: ključnih besedah Summary of found: ...Pierre Auger Observatory,
ultra-high energy cosmic rays ( UHECR),
UHECR energy spectrum, mass composition, anisotropies... Keywords: Pierre Auger Observatory, ultra-high energy cosmic rays (UHECR), UHECR energy spectrum, mass composition, anisotropies Published: 20.06.2017; Views: 3412; Downloads: 0
Fulltext (1,06 MB) |
16. Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger ObservatoryMarko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, A. Aab, 2017, original scientific article Found in: ključnih besedah Summary of found: ...Pierre Auger Observatory,
ultra-high energy cosmic rays ( UHECR),
UHECR anisotropies,
angular power spectrum, needlet wavelet analysis... Keywords: Pierre Auger Observatory, ultra-high energy cosmic rays (UHECR), UHECR anisotropies, angular power spectrum, needlet wavelet analysis Published: 23.06.2017; Views: 2979; Downloads: 0
Fulltext (1,12 MB) |
17. Results from the Pierre Auger ObservatoryMarko Zavrtanik, Danilo Zavrtanik, Darko Veberič, Samo Stanič, Andrej Filipčič, Ivan De Mitri, 2015, published scientific conference contribution Found in: ključnih besedah Summary of found: ...Pierre Auger Observatory,
Ultra High Energy Cosmic Rays ( UHECR),
UHECR energy spectrum, UHECR mass composition... Keywords: Pierre Auger Observatory, Ultra High Energy Cosmic Rays (UHECR), UHECR energy spectrum, UHECR mass composition Published: 27.06.2017; Views: 2868; Downloads: 0
Fulltext (475,69 KB) |
18. Reconstructed properties of the sources of UHECR and their dependence on the extragalactic magnetic fieldMarko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Darko Veberič, Marta Trini, Samo Stanič, Ahmed Saleh, Gašper Kukec Mezek, Andrej Filipčič, David Wittkowski, 2017, published scientific conference contribution Found in: ključnih besedah Keywords: extragalactic magnetic field, Pierre Auger Observatory, sources of UHECR Published: 16.02.2018; Views: 2329; Downloads: 140
Fulltext (356,61 KB) |
19. Eenergy Anisotropies of Proton-like Ultra-High Energy Cosmic RaysJon Paul Lundquist, doctoral dissertation Abstract: Evidence of a number of interrelated energy dependent intermediate-scale anisotropies have been found in the arrival directions of proton-like ultra-high energy cosmic rays (UHECR) using 7 years of Telescope Array (TA) data. These are found using analysis techniques that have been developed for this dissertation. Using surface detector (SD) data the reported TA “Hotspot” excess, E≥10^19.75 eV, is found to correspond to a deficit, or “Coldspot,” of events for 10^19.1≤E<10^19.75 eV at 142◦R.A., 40◦ Dec. The global post-trial significance of this Hot/Coldspot event density asymmetry is found to be 5.1σ (p = 1.56 × 10−7). This Hot/Coldspot feature is the combination, at the same location, of an energy spectrum anisotropy with a 3.74σ significance for energies E≥10^19.2 eV and an energy-distance correlation with a 3.34σ significance for energies E≥1019.3 eV. The UHECR Hotspot alone is analyzed using a new kernel density estimation (KDE) anisotropy method and found to have a 3.65σ significance (E≥1019.75 eV). These features suggest energy dependent magnetic deflection of UHECR. The composition of UHECR primary particles is also studied using a new “Quality Factor Analysis” pattern recognition event selection for fluorescence detectors (FD). This minimizes the energy dependence of the resolution of extensive air shower (EAS) Xmax depth. Also, a new statistical method making use of all higher moments than the mean shower depth distribution is developed – as there is large disagreement in between all EAS simulation models. There is also an uncertainty, just as large, for any particular model, given uncertainties in particle interaction parameters extrapolated to much higher energies from Large Hadron Collider (LHC) data. The TA hybrid FD/SD data is found to be statistically compatible with a pure proton composition, though not incompatible with a light mixed composition, for all models of EAS above E≥10^18.4 eV. There is also no statistically significant evidence of the composition getting heavier at the highest energies. The combined information of a proton-like light composition, and anisotropy evidence suggestive of energy dependent magnetic deflection of UHECR, should be useful for informing future source searches and models of intergalactic propagation through magnetic fields. Found in: ključnih besedah Summary of found: ...directions of proton-like ultra-high energy cosmic rays ( UHECR) using 7 years of Telescope Array (TA)... Keywords: cosmic rays, UHECR, composition, anisotropy Published: 24.04.2020; Views: 1809; Downloads: 0
Fulltext (10,26 MB) |
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