Moreno Baricevic
YOU?
Author Swipe
View article: Enhancing air-shower observations: Results from an IceCube Surface Array Prototype Station
Enhancing air-shower observations: Results from an IceCube Surface Array Prototype Station Open
The Surface Array Enhancement of the IceCube Neutrino Observatory is set to equip the existing\nsurface cosmic-ray array of ice-Cherenkov detectors, IceTop, with radio antennas and scintillation\ndetectors. This can lower the energy thresh…
View article: Towards the Composition of sub-PeV Cosmic Rays at IceCube
Towards the Composition of sub-PeV Cosmic Rays at IceCube Open
With the implementation of a low-energy trigger, the surface array of the IceCube Neutrino Observatory is able to record cosmic-ray induced air showers with a primary energy of a few hundred TeV. This extension of the energy range closes t…
View article: In situ estimation of ice crystal properties at the South Pole using LED calibration data from the IceCube Neutrino Observatory
In situ estimation of ice crystal properties at the South Pole using LED calibration data from the IceCube Neutrino Observatory Open
The IceCube Neutrino Observatory instruments about 1 km3 of deep, glacial ice at the geographic South Pole. It uses 5160 photomultipliers to detect Cherenkov light emitted by charged relativistic particles. An unexpected light propagation …
View article: Cosmic ray detection with the IceTop Enhancement
Cosmic ray detection with the IceTop Enhancement Open
IceTop is the cosmic-ray detector located on the surface of the IceCube Neutrino Observatory at the South Pole, consisting of 81 pairs of ice-Cherenkov tanks. The rise in the energy threshold of air-shower measurements in IceTop due to acc…
View article: Highlights from the IceCube Neutrino Observatory
Highlights from the IceCube Neutrino Observatory Open
As IceCube surpasses a decade of operation in the full detector configuration, results that drive forward the fields of neutrino astronomy, cosmic ray physics, multi-messenger astronomy, particle physics, and beyond continue to emerge at a…
View article: Measurement of the Cosmic Neutrino Flux from the Southern Sky using 10 years of IceCube Starting Track Events
Measurement of the Cosmic Neutrino Flux from the Southern Sky using 10 years of IceCube Starting Track Events Open
The measurement of a diffuse astrophysical neutrino flux using starting track events marks the first time IceCube has observed and subsequently measured the astrophysical diffuse flux using a dataset composed primarily of starting track ev…
View article: Search for TeV Neutrinos from Seyfert Galaxies in the Southern Sky using Starting Track Events in IceCube
Search for TeV Neutrinos from Seyfert Galaxies in the Southern Sky using Starting Track Events in IceCube Open
Supermassive black holes (SMBHs) power active galactic nuclei (AGN). The vicinity of the SMBH has long been proposed as the potential site of particle acceleration and neutrino production. Recently, IceCube reported evidence of neutrino em…
View article: Joint searches by FACT, H.E.S.S., MAGIC and VERITAS for VHE gamma-ray emission associated with neutrinos detected by IceCube
Joint searches by FACT, H.E.S.S., MAGIC and VERITAS for VHE gamma-ray emission associated with neutrinos detected by IceCube Open
The sources of the astrophysical flux of high-energy neutrinos detected by IceCube are still largely unknown, but searches for temporal and spatial correlation between neutrinos and electromagnetic radiation are a promising approach in thi…
View article: Search for Extremely High Energy Neutrinos with IceCube
Search for Extremely High Energy Neutrinos with IceCube Open
Extremely high energy (EHE) neutrinos (with energies above $10^7$ GeV) are produced in interactions of the highest energy cosmic rays. A primary contribution to the EHE neutrino flux is expected from so-called cosmogenic neutrinos produced…
View article: Cosmic Ray Anisotropy with Eleven Years of IceCube Data
Cosmic Ray Anisotropy with Eleven Years of IceCube Data Open
The IceCube Observatory provides our highest-statistics picture of the cosmic-ray arrival directions in the Southern Hemisphere, with over 700 billion cosmic-ray-induced muon events collected between May 2011 and May 2022. Using the larger…
View article: Search for high-energy neutrinos from magnetars with IceCube
Search for high-energy neutrinos from magnetars with IceCube Open
Neutron stars with very strong magnetic fields are known as magnetars. There are multiple theories that predict magnetars may be able to emit high-energy (HE) neutrinos through hadronic processes by accelerating cosmic rays to high energie…
View article: Search for Cosmic-Ray Events Using Radio Signals and CNNs in Data from the IceTop Enhancement Prototype Station
Search for Cosmic-Ray Events Using Radio Signals and CNNs in Data from the IceTop Enhancement Prototype Station Open
Cosmic-ray air showers emit radio waves that can be used to measure the properties of cosmic-ray primary particles. The radio detection technique presents several advantages, such as low cost and year-round duty cycle as well as the abilit…
View article: The Surface Array of IceCube-Gen2
The Surface Array of IceCube-Gen2 Open
The science goals of IceCube-Gen2 include multi-messenger astronomy, astroparticle and particle physics. To this end, the observatory will include several detection methods, including a surface array and in-ice optical sensors. The array w…
View article: Search for high-energy neutrino emission from hard X-ray AGN with IceCube
Search for high-energy neutrino emission from hard X-ray AGN with IceCube Open
Active Galactic Nuclei (AGN) are powerful astronomical objects with very high luminosities. Theoretical arguments suggest that these objects are capable of accelerating particles to energies of 1020 eV. In environments with matter or photo…
View article: A multi-detector EAS reconstruction framework for IceCube
A multi-detector EAS reconstruction framework for IceCube Open
The IceCube Neutrino Observatory is also a very unique extensive air shower (EAS) detector, that simultaneously measures the EAS footprint on the surface and the high-energy muons in deep ice. The surface array - IceTop, comprising of ice-…
View article: Searches for IceCube Neutrinos Coincident with Gravitational Wave Events
Searches for IceCube Neutrinos Coincident with Gravitational Wave Events Open
Searches for neutrinos from gravitational wave events have been performed utilizing the wide energy range of the IceCube Neutrino Observatory. We discuss results from these searches during the third observing run (O3) of the advanced LIGO …
View article: Sensitivity of the IceCube-Gen2 Surface Array for Cosmic-Ray Anisotropy Studies
Sensitivity of the IceCube-Gen2 Surface Array for Cosmic-Ray Anisotropy Studies Open
The energy of the transition from Galactic to extra-galactic origin of cosmic rays is one of the major unresolved issues of cosmic-ray physics. However, strong constraints can be obtained from studying the anisotropy in the arrival directi…
View article: Exploring the Galactic neutrino flux origins using IceCube datasets
Exploring the Galactic neutrino flux origins using IceCube datasets Open
Astrophysical neutrinos detected by the IceCube observatory can be of Galactic or extragalactic origin. The collective contribution of all the detected neutrinos allows us to measure the total diffuse neutrino Galactic and extragalactic si…
View article: Estimating the coincidence rate between the optical and radio array of IceCube-Gen2
Estimating the coincidence rate between the optical and radio array of IceCube-Gen2 Open
The IceCube-Gen2 Neutrino Observatory is proposed to extend the all-flavour energy range of IceCube beyond PeV energies. It will comprise two key components: I) An enlarged 8km3 in-ice optical Cherenkov array to measure the continuation of…
View article: Summary of IceCube tau neutrino searches and flavor composition measurements of the diffuse astrophysical neutrino flux
Summary of IceCube tau neutrino searches and flavor composition measurements of the diffuse astrophysical neutrino flux Open
We present a summary of the flavor composition measurements for the diffuse astrophysical neutrino flux using data from the IceCube Neutrino Observatory at the South Pole. IceCube has identified candidate astrophysical tau neutrinos throug…
View article: A Two-Component Lateral Distribution Function for the Reconstruction of Air-Shower Events in IceTop
A Two-Component Lateral Distribution Function for the Reconstruction of Air-Shower Events in IceTop Open
The surface component of the IceCube Neutrino Observatory, IceTop, consists of an array of ice-Cherenkov tanks measuring the electromagnetic signal as well as low-energy (∼ GeV) muons from cosmic-ray air showers. In addition, accompanying …
View article: 2D Convolutional Neural Network for Event Reconstruction in IceCube DeepCore
2D Convolutional Neural Network for Event Reconstruction in IceCube DeepCore Open
IceCube DeepCore is an extension of the IceCube Neutrino Observatory designed to measure GeV scale atmospheric neutrino interactions for the purpose of neutrino oscillation studies. Distinguishing muon neutrinos from other flavors and reco…