نتایج جستجو برای: cherenkov array

تعداد نتایج: 135478  

2017
Petr Janeček Jan Ebr Jiří Blažek Michael Prouza Martin Mašek

The Cherenkov Telescope Array (CTA) is a project to build a new generation ground-based gammaray observatory. The FRAM – F(/Ph)otometric Robotic Atmospheric Monitor – is a device, which can provide it with the Vertical Aerosol Optical Depth (VAOD) maps in the field of view of the CTA in almost real time (delay in minutes). The FRAM is a small fast robotic astronomical telescope with a large fie...

2017
F. De Palma M. Del Santo C. Delgado D. della Volpe T. Di Girolamo

We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX J1713.7−3946, a young supernova remnant (SNR) and one of the brightest sources ever discovered in very-high-energy (VHE) gamma rays. Special attention is paid to explore possible spatial (anti-)correlations of gamma rays with emission at other wavelengths, in particular X-rays and CO/Hi emission. We present a s...

Journal: :Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 2018

Journal: :Journal of physics 2023

Abstract In the last decades an incredible amount of evidence for existence dark matter (DM) has been accumulating. At same time, many efforts have undertaken to try identify what is made of. Indirect searches look at places in Universe where known be abundant and seek possible annihilation or decay signatures. with Fermi Gamma ray Space Telescope Imaging Atmospheric Cherenkov Telescopes (IACTs...

Journal: :Journal of physics 2023

Abstract The Large-Sized Telescopes (LSTs) of the Cherenkov Telescope Array (CTA) are designed for gamma-ray studies focusing on low energy threshold, high flux sensitivity and rapid telescope repositioning. LST has a tessellated parabolic mirror 23 m diameter weight about 100 tons, with capability pointing to any position in sky 20 seconds or less catch transients. A 2 ton 3x3 camera, placed f...

2009
Wystan Benbow

The VERITAS array of 12-m atmospheric-Cherenkov telescopes in southern Arizona is currently the world’s most-sensitive detector of astrophysical very high energy (VHE; E>100 GeV) γ-rays. Approximately 25 blazars are known to emit VHE photons, and observations of blazars are one of the VERITAS collaboration’s key science projects (KSP). More than 50 of these objects have been observed with the a...

2008
H. KRAWCZYNSKI

The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is an array of four 12m diameter Imaging Atmospheric Cherenkov Technique (IACT) telescopes operated at the base of Mt. Hopkins in southern Arizona. The four-telescope experiment started operation in April, 2007. GeV and TeV gamma-ray observations of blazars can be used to probe the structure and composition of their jets, and...

Journal: :Physics in medicine and biology 2017
S E Brunner D R Schaart

Due to detector developments in the last decade, the time-of-flight (TOF) method is now commonly used to improve the quality of positron emission tomography (PET) images. Clinical TOF-PET systems based on L(Y)SO:Ce crystals and silicon photomultipliers (SiPMs) with coincidence resolving times (CRT) between 325 ps and 400 ps FWHM have recently been developed. Before the introduction of L(Y)SO:Ce...

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