Tim Unbehaun
A5040463382- Astrophysics and Cosmic Phenomena
- Gamma-ray bursts and supernovae
- Astrophysical Phenomena and Observations
- Dark Matter and Cosmic Phenomena
- Pulsars and Gravitational Waves Research
- Neutrino Physics Research
- Astro and Planetary Science
- Radiation Detection and Scintillator Technologies
- Astrophysics and Star Formation Studies
- Particle Detector Development and Performance
- Astronomical Observations and Instrumentation
- Nuclear Physics and Applications
- Particle physics theoretical and experimental studies
- 2D Materials and Applications
- Medical Imaging Techniques and Applications
- High-Energy Particle Collisions Research
- MXene and MAX Phase Materials
- Perovskite Materials and Applications
- Galaxies: Formation, Evolution, Phenomena
- Atomic and Subatomic Physics Research
Friedrich-Alexander-Universität Erlangen-Nürnberg
2021-2024
Institut de Recherche sur les Lois Fondamentales de l'Univers
2023
CEA Paris-Saclay
2023
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
2023
ETH Zurich
2023
University of Würzburg
2023
École Polytechnique
2023
Centre National de la Recherche Scientifique
2023
Laboratoire Leprince-Ringuet
2023
Istituto Nazionale di Fisica Nucleare, Sezione di Padova
2023
Context. Traditionally, TeV- γ -ray astronomy has been conducted by experiments employing proprietary data and analysis software. However, the next generation of instruments, such as Cherenkov Telescope Array Observatory (CTAO), will be operated open observatories. Alongside data, they also make associated software tools available to a wider community. This necessity prompted development open, high-level, astronomical customized for high-energy astrophysics. Aims. In this article, we present...
Imaging atmospheric Cherenkov telescopes (IACTs) detect rays by measuring the light emitted secondary particles in air shower when hit atmosphere of Earth. Given usual distances between IACT arrays, at low energies (lesssim 100 GeV), limited amount produced typically implies that event is registered one only. Such events are called monoscopic events, and their analysis particularly difficult. Challenges include reconstruction event's arrival direction, energy, rejection background due to...
Imaging atmospheric Cherenkov telescopes (IACTs) detect gamma rays by measuring the light emitted secondary particles in air shower when hit atmosphere. At low energies, limited amount of produced typically implies that event is registered one IACT only. Such events are called monoscopic events, and their analysis particularly difficult. Challenges include reconstruction event's arrival direction, energy, rejection background events. Here, we present a set improvements, including...
Abstract Multilayers of so-called 2D van der Waals materials have gained considerable attention as active components next-generation electronic and optoelectronic technologies, with semiconducting black phosphorus (BP) regarded one the most promising systems. The applicability performance limits BP in both stand-alone heterostructure-based multilayer devices are determined by individual flake charge transport properties, which synergistically depend on number layers strength interlayer...
Abstract The Cherenkov Telescope Array and the KM3NeT neutrino telescopes are major upcoming facilities in fields of $$\gamma $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>γ</mml:mi> </mml:math> -ray astronomy, respectively. Possible simultaneous production rays neutrinos astrophysical accelerators cosmic-ray nuclei motivates a combination their data. We assess potential combined analysis CTA data to determine contribution hadronic emission processes known Galactic...
In this article, we present Gammapy, an open-source Python package for the analysis of astronomical $\gamma$-ray data, and illustrate functionalities its first long-term-support release, version 1.0. Built on modern scientific ecosystem, Gammapy provides a uniform platform reducing modeling data from different instruments many scenarios. complies with several well-established conventions in high-energy astrophysics, providing serialized products that are interoperable other software...
The Cherenkov Telescope Array and the KM3NeT neutrino telescopes are major upcoming facilities in fields of $\gamma$-ray astronomy, respectively. Possible simultaneous production $\gamma$ rays neutrinos astrophysical accelerators cosmic-ray nuclei motivates a combination their data. We assess potential combined analysis CTA data to determine contribution hadronic emission processes known Galactic emitters, comparing this result cases two separate analyses. In doing so, we demonstrate...