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CERN Document Server 14 записей найдено  1 - 10следующий  перейти к записи: Поиск длился 1.12 секунд. 
1.
Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring Episode / Event Horizon Telescope Multi-wavelength Science Collaboration
The nearby elliptical galaxy M87 contains one of the only two supermassive black holes whose emission surrounding the event horizon has been imaged by the Event Horizon Telescope (EHT). [...]
arXiv:2404.17623 ; FERMILAB-PUB-24-0804-PPD. - 46.
Fermilab Library Server - Fulltext - Fulltext
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2.
Searches for gamma-ray lines and `pure WIMP' spectra from Dark Matter annihilations in dwarf galaxies with H.E.S.S / H.E.S.S. Collaboration
Dwarf spheroidal galaxies are among the most promising targets for detecting signals of Dark Matter (DM) annihilations. The H.E.S.S. [...]
arXiv:1810.00995; DESY 18-157; DESY-18-157; CERN-TH-2018-201.- 2018-11-23 - 23 p. - Published in : JCAP 11 (2018) 037 Fulltext: PDF;
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3.
Science with the Cherenkov Telescope Array / Cherenkov Telescope Array Consortium Collaboration
The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. [...]
arXiv:1709.07997. - 2017. - 211 p.
Preprint
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4.
The cosmic ray proton, helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOP / Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the National Gran Sasso Laboratories by means of EAS-TOP (Campo Imperatore, 2005 m a.s.l.) and MACRO (deep underground, 3100 m w.e., the surface energy threshold for a muon reaching the detector being E/sub mu //sup th/ approximately=1.3 TeV). The measurement is based on: (a) the selection of primaries based on their energy/nucleon (i.e., with energy/nucleon sufficient to produce a muon with energy larger than 1.3 TeV) and the reconstruction of the shower geometry by means of the muons recorded by MACRO in the deep underground laboratories; (b) the detection of the associated atmospheric Cherenkov light (C.l.) signals by means of the C.l. [...]
2004 - Published in : Astropart. Phys. 21 (2004) 223-40
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5.
Calibrations of CR39 and Makrofol nuclear track detectors and search for exotic particles / MACRO Collaboration
We present the final results of the search for exotic massive particles in the cosmic radiation performed with the MACRO underground experiment. Magnetic monopoles and nuclearites flux upper limits obtained with the CR39 nuclear track subdetector, the scintillation and streamer tube subdetectors are given. [...]
2003 - Published in : Nucl. Phys. B, Proc. Suppl. 125 (2003) 217-21
In : 8th Topical Seminar on Innovative Particle and Radiation Detectors, Sienna, Italy, 21 - 24 Oct 2002, pp.217-21 (vol. 125)
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6.
Search for GUT magnetic monopoles and nuclearites with the MACRO experiment / MACRO Collaboration
We present the final results obtained by the MACRO experiment in the search for GUT magnetic monopoles and nuclearites. Several searches were performed with different subdetectors, i.e. [...]
2003 - Published in : Radiat. Meas. 36 (2003) 301-5
In : 21st International Conference on Nuclear Tracks in Solids, New Delhi, India, 21 - 25 Oct 2002, pp.301-5 (vol. 36)
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7.
Time correlations of high energy muons in an underground detector / Becherini, Y ; Cecchini, S ; Chiarusi, T ; Cozzi, M ; Dekhissi, H ; Derkaoui, J ; Esposito, L S ; Giacomelli, G ; Giglietto, N ; Giorgini, M et al.
We present the result of a search for correlations in the arrival times of high energy muons collected from 1995 till 2000 with the streamer tube system of the complete MACRO detector at the underground Gran Sasso Lab. Large samples of single muons (8.6 million), double muons (0.46 million) and multiple muons with multiplicities from 3 to 6 (0.08 million) were selected. [...]
2005 - Published in : Astropart. Phys. 23 (2005) 341-348
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8.
The cosmic ray primary composition between $10^{15}$ and $10^{16}$ ev from Extensive Air Showers electromagnetic and TeV muon data / Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The cosmic ray primary composition in the energy range between 10/sup 15/ and 10/sup 16/ eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurements of the EAS-TOP air shower array (2005 m a.s.l., 10/sup 5/ m/sup 2/ collecting area) and the MACRO underground detector (963 m a.s.l., 3100 m w.e. of minimum rock overburden, 920 m/sup 2/ effective area) at the National Gran Sasso Laboratories. [...]
2004 - Published in : Astropart. Phys. 20 (2004) 641-52
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9.
Transmission of light in deep sea water at this site of the ANTARES neutrino telescope / ANTARES Collaboration
DAPNIA-2004-090. - 2004. - 40 p.
Fulltext
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10.
Neutrino energy estimates from multiple Coulomb scattering of upthroughgoing muons in MACRO / Bakari, D ; Becherini, Y ; Giorgini, M ; Spurio, M /MACRO Collaboration
Summary form only given. Estimates of the energies of neutrino induced muons in MACRO were made by measuring the multiple Coulomb scattering (MCS) in the rock absorbers in the lower part of the MACRO detector. [...]
2002
In : 6th ICTP School on Non-Accelerator Astroparticle Physics, Trieste, Italy, 9 - 20 Jul 2001, pp.355-6
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CERN Document Server : 14 записей найдено   1 - 10следующий  перейти к записи:
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116 Becherini, Y
2 Becherini, Yvonne
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