about
Black hole lightning due to particle acceleration at subhorizon scalesMAGIC detection of short-term variability of the high-peaked BL Lac object 1ES 0806+524Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010Optimized dark matter searches in deep observations of Segue 1 with MAGICThe major upgrade of the MAGIC telescopes, Part II: A performance study using observations of the Crab NebulaThe major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the systemVery high energy {gamma}-rays from the universe's middle age: detection of the z = 0.940 blazar PKS 1441+25 with MAGICFIRST NuSTAR OBSERVATIONS OF MRK 501 WITHIN A RADIO TO TeV MULTI-INSTRUMENT CAMPAIGNDiscovery of Very High Energy Gamma Radiation from IC 443 with the MAGIC TelescopeRadio imaging of the very-high-energy gamma-ray emission region in the central engine of a radio galaxy.Very-high-energy gamma rays from a distant quasar: how transparent is the universe?Observation of pulsed gamma-rays above 25 GeV from the Crab pulsar with MAGIC.Upper Limit for γ‐Ray Emission above 140 GeV from the Dwarf Spheroidal Galaxy DracoVery High Energy Gamma-Ray Radiation from the Stellar Mass Black Hole Binary Cygnus X-1Limits on the flux of tau neutrinos from 1 PeV to 3 EeV with the MAGIC telescopesIndirect dark matter searches in the dwarf satellite galaxy Ursa Major II with the MAGIC telescopesMAGIC gamma-ray telescope observation of the Perseus cluster of galaxies: implications for cosmic rays, dark matter, and NGC 1275Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomyChanges in the annihilation delay time distribution of stopped antiprotons in helium gas, due to contaminants. — IIExotic trapping of antiprotons in4He: dependence on pressureExperimental antiproton nuclear stopping power inH2andD2p̄p annihilation cross section at very low energyAntiproton Slowing Down inH2and He and Evidence of Nuclear Stopping PowerPerformances of the OBELIX time of flight systemφπ0 and φη production in antiproton annihilation at rest in a hydrogen gas target at NTPA study of pontecorvo reactions in antiproton deuterium annihilations at restAnnihilation cross-sections of antineutrons on C, Al, Cu, Sn and Pb at low momenta (180–280 MeV/c) with the OBELIX spectrometerChanges in the Annihilation’s delay time distribution of stopped antiprotons in helium gas, due to contaminants.—IEvidence of a new state at ∼ 1660 MeV/c2 observed in $$\bar np$$ annihilationsannihilationsFirst results from OBELIX on reactions with detected neutral poins in the final stateMeasurement of the frequency of the annihilation reaction at rest in a NTP hydrogen targetMeasurement of the annihilation frequencies in a 5 mb hydrogen gas targetMeson spectroscopy withS- andP-wave-dominant initial-state selection in $$\bar pp$$ annihilationannihilationThe φπ+/ωπ+ ratio from $$\bar np$$ annihilationsannihilationsφ and ω meson production in annihilation and the OZI ruleA new measurement of the Pontecorvo reaction with the OBELIX spectrometer at LEARAntiproton stopping power in hydrogen below 120 keV and the Barkas effectFirst results on nuclear physics with antineutrons by the OBELIX spectrometerNew results on meson spectroscopy from ObelixNuclear physics with OBELIX
P50
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P50
description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Petar Temnikov
@ast
Petar Temnikov
@en
Petar Temnikov
@es
Petar Temnikov
@nl
type
label
Petar Temnikov
@ast
Petar Temnikov
@en
Petar Temnikov
@es
Petar Temnikov
@nl
prefLabel
Petar Temnikov
@ast
Petar Temnikov
@en
Petar Temnikov
@es
Petar Temnikov
@nl
P1053
L-6999-2016
P106
P1153
7003612798
P31
P496
0000-0002-9559-3384