Global ETD Search

Search theses and dissertations gathered from participating repositories worldwide. Every result links back to the library that holds it. No account is needed.

Results

Showing 1 to 8 of 8 for “"Imaging atmospheric cherenkov telescopes"”.

  1. A detailed study of the gamma-ray supernova remnant RX J1713.7-3946 with H.E.S.S.

    The H.E.S.S. telescope system -- an array of four imaging atmospheric Cherenkov telescopes situated in Namibia -- aims at exploring non-thermal processes in the universe by means of very-high-energy (VHE) gamma rays. Its large field of view combined with unprecedented sensitivity enables detailed …

    heid-diss Repository record for A detailed study of the gamma-ray supernova remnant RX J1713.7-3946 with H.E.S.S. (opens in a new tab)

  2. Generic FPGA Preprocessing for Astrophysics Instruments in HLS

    … detectors with 1D pixel arrays, and imaging atmospheric Cherenkov telescopes with 2D pixel arrays. In doing so, we also present a novel HLS-based two-pass connected-component labeling (CCL) implementation that can be easily switched between 4-way and 8-way CCL.</p>

    wustl Repository record for Generic FPGA Preprocessing for Astrophysics Instruments in HLS (opens in a new tab)

  3. A hybrid analysis approach to the high energy stereoscopic system phase II mono-analysis

    … Stereoscopic System (H.E.S.S.) is an array of imaging atmospheric Cherenkov telescopes located in the Khomas highlands of Namibia. Their primary purpose is to detect Cherenkov light (CL) produced by particles in extensive air showers which are produced by incident high energy particles (gamma …

    namibia Repository record for A hybrid analysis approach to the high energy stereoscopic system phase II mono-analysis (opens in a new tab)

  4. Investigating Extended Gamma-Ray Sources with ASTRI and CTAO: Observation, Analysis and Modelling

    … Galactic sources with next-generation IACTs (Imaging Atmospheric Cherenkov Telescopes) like the telescopes of the ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array and CTAO (Cherenkov Telescope Array Observatory), with the dual aim of addressing the role of young …

    trento Repository record for Investigating Extended Gamma-Ray Sources with ASTRI and CTAO: Observation, Analysis and Modelling (opens in a new tab)

  5. Investigating Extended Gamma-Ray Sources with ASTRI and CTAO: Observation, Analysis and Modelling

    … Galactic sources with next-generation IACTs (Imaging Atmospheric Cherenkov Telescopes) like the telescopes of the ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array and CTAO (Cherenkov Telescope Array Observatory), with the dual aim of addressing the role of young …

    trento Repository record for Investigating Extended Gamma-Ray Sources with ASTRI and CTAO: Observation, Analysis and Modelling (opens in a new tab)

  6. Decoding Continuous Gravitational Waves from Pulsars: A Multi-Wavelength Approach

    … using data from ground-based GW detectors and Imaging Atmospheric Cherenkov Telescopes (IACTs). In particular, this research integrates very-high-energy (VHE) observations from the High Energy Stereoscopic System (HESS) with data from the second observing run of the Advanced Laser …

    adelaide Repository record for Decoding Continuous Gravitational Waves from Pulsars: A Multi-Wavelength Approach (opens in a new tab)

  7. Search for gamma-ray emission from bow shocks of runaway stars

    … on-board the Fermi satellite and the H.E.S.S. telescopes located in the Khomas Highland in Namibia. The Fermi-LAT was launched in 2008 and is continuously scanning the sky since then. It detects photons with energies from 20MeV to over 300 GeV and has an unprecedented sensitivity. The all-sky …

    potsdam-diss Repository record for Search for gamma-ray emission from bow shocks of runaway stars (opens in a new tab)

  8. The search for dark matter annihilation in galaxy clusters at VERITAS

    <p>Recent data and cosmological models point to a significant fraction of the Universe being comprised of Cold Dark Matter (DM), though little is known about it directly as it does not interact electromagnetically. The most likely explanation for DM is a Weakly Interacting Massive Particle (WIMP) …

    purdue-thes Repository record for The search for dark matter annihilation in galaxy clusters at VERITAS (opens in a new tab)