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V. Verguilov

Researcher at University of Geneva

Publications -  20
Citations -  6594

V. Verguilov is an academic researcher from University of Geneva. The author has contributed to research in topics: Fermi Gamma-ray Space Telescope & Blazar. The author has an hindex of 3, co-authored 5 publications receiving 5986 citations. Previous affiliations of V. Verguilov include Sofia University.

Papers
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The CMS experiment at the CERN LHC

S. Chatrchyan, +3175 more
TL;DR: The Compact Muon Solenoid (CMS) detector at the Large Hadron Collider (LHC) at CERN as mentioned in this paper was designed to study proton-proton (and lead-lead) collisions at a centre-of-mass energy of 14 TeV (5.5 TeV nucleon-nucleon) and at luminosities up to 10(34)cm(-2)s(-1)
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CMS physics technical design report, volume II: Physics performance

G. L. Bayatian, +2063 more
- 01 Jun 2007 - 
TL;DR: In this article, the authors present a detailed analysis of the performance of the Large Hadron Collider (CMS) at 14 TeV and compare it with the state-of-the-art analytical tools.
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CMS physics technical design report: Addendum on high density QCD with heavy ions

David D'Enterria, +2188 more
- 01 Nov 2007 - 
TL;DR: In this paper, the capabilities of the CERN Large Hadron Collider (LHC) experiment to explore the rich heavy-ion physics program offered by the LHC are presented, and the potential of the CMS experiment to carry out a series of representative Pb-Pb measurements.
Journal ArticleDOI

Author Correction: Proton acceleration in thermonuclear nova explosions revealed by gamma rays

V. A. Acciari, +208 more
- 15 Feb 2022 - 
TL;DR: In this article , the MAGIC telescopes were used to detect gamma-ray emission from RS Ophiuchi, a recurrent nova with a red giant companion, which allowed them to accurately characterize the emission from a nova in the 60 GeV to 250 GeV energy range.
Journal ArticleDOI

Proton acceleration in thermonuclear nova explosions revealed by gamma rays

V. A. Acciari, +208 more
- 14 Apr 2022 - 
TL;DR: In this article , the MAGIC telescopes were used to detect gamma-ray emission from RS Ophiuchi, a recurrent nova with a red giant companion, which allowed them to accurately characterize the emission from a nova in the 60 GeV to 250 GeV energy range.