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researcher

G. Bashindzhagyan

4 papers hereh-index 9364 citations26 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph1
  • hep-ex1
same name
  • G. Bashindzhagyan — 9 papers, h 24
  • G. Bashindzhagyan — 2 papers, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19952011
collaborators

4 papers

astro-ph.HE2011

Possible structure in the cosmic ray electron spectrum measured by the ATIC-2 and ATIC-4 experiments

A. D. Panov, V. I. Zatsepin, N. V. Sokolskaya +15

A strong excess in a form of a wide peak in the energy range of 300-800 GeV was discovered in the first measurements of the electron spectrum in the energy range from 20 GeV to 3 T…

astro-ph.HE2009

Energy dependence of Ti/Fe ratio in the Galactic cosmic rays measured by the ATIC-2 experiment

V. I. Zatsepin, A. D. Panov, N. V. Sokolskaya +15

Titanium is a rare, secondary nucleus among Galactic cosmic rays. Using the Silicon matrix in the ATIC experiment, Titanium has been separated. The energy dependence of the Ti to F…

astro-ph2007

Relative abundances of cosmic ray nuclei B-C-N-O in the energy region from 10 GeV/n to 300 GeV/n. Results from ATIC-2 (the science flight of ATIC)

A. D. Panov, N. V. Sokolskaya, J. H. Adams +19

The ATIC balloon-borne experiment measures the energy spectra of elements from H to Fe in primary cosmic rays from about 100 GeV to 100 TeV. ATIC is comprised of a fully active bis…

hep-ex1995

Measurement of multiplicity and momentum spectra in the current fragmentation region of the Breit frame at HERA

ZEUS Collaboration

Charged particle production has been measured in Deep Inelastic Scattering (DIS) events using the ZEUS detector over a large range of Q2 from 10 to 1280 GeV2. The evol…

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