activity
20092016
most citedMeasurement of the in-medium phi-meson width in proton-nucleus collisions

78 citations · 160 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2016★ 5 cited

Very Hight Energy Observationa of Shell-Type Supernova Remnants with SHALON Mirror Cherenkov Telescopes

Vera G. Sinitsyna, Vera Y. Sinitsyna

The investigation of VHE gamma-ray sources by any methods, including mirror Cherenkov telescopes, touches on the problem of the cosmic ray origin and, accordingly, the role of the…

nucl-ex2015★ 6 cited

Kaon pair production in proton-nucleus collisions at 2.83 GeV kinetic energy

Yu. T. Kiselev, M. Hartmann, A. Polyanskiy +23

The production of non-phi K+K- pairs by protons of 2.83 GeV kinetic energy on C, Cu, Ag, and Au targets has been investigated using the COSY-ANKE magnetic spectrometer. The K- mome…

astro-ph.HE2014★ 27 cited

Emission from the Galaxy NGC 1275 at High and Very High Energies and its Origin

V. G. Sinitsyna, V. Yu. Sinitsyna

The Seyfert galaxy NGC 1275 is the central, dominant galaxy in the Perseus cluster of galaxies. NGC1275 is known as a powerful source of radio and X-ray emission. The well-known ex…

nucl-ex2012★ 44 cited

Momentum dependence of the phi-meson nuclear transparency

M. Hartmann, Yu. T. Kiselev, A. Polyanskiy +29

The production of phi mesons in proton collisions with C, Cu, Ag, and Au targets has been studied via the phi -> K+K- decay at an incident beam energy of 2.83 GeV using the ANKE de…

nucl-ex2010★ 78 cited

Measurement of the in-medium phi-meson width in proton-nucleus collisions

A. Polyanskiy, M. Hartmann, Yu. T. Kiselev +25

The production of phi mesons in the collisions of 2.83 GeV protons with C, Cu, Ag, and Au at forward angles has been measured via the phi -> K+K- decay using the COSY-ANKE magnetic…

hep-ph2009

Heavy neutrino decay at SHALON

V. G. Sinitsyna, M. Masip, S. I. Nikolsky +1

The SHALON Cherenkov telescope has recorded over 2x10^6 extensive air showers during the past 17 years. The analysis of the signal at different zenith angles (θ) has included obser…