activity
20092023
most citedThe Knee of the Cosmic Hydrogen and Helium Spectrum below 1 PeV Measured by ARGO-YBJ and a Cherenkov Telescope of LHAASO

127 citations · 1.2k across the 28 of their papers we have counts for

collaborators
Showing 2015Show all

7 papers · 1 filter

astro-ph.IM2015★ 40 cited

Detection of thermal neutrons with the PRISMA-YBJ array in Extensive Air Showers selected by the ARGO-YBJ experiment

B. Bartoli, P. Bernardini, X. J. Bi +79

We report on a measurement of thermal neutrons, generated by the hadronic component of extensive air showers (EAS), by means of a small array of EN-detectors developed for the PRIS…

astro-ph.HE2015★ 63 cited

4.5 years multi-wavelength observations of Mrk 421 during the ARGO-YBJ and Fermi common operation time

B. Bartoli, P. Bernardini, X. J. Bi +68

We report on the extensive multi-wavelength observations of the blazar Markarian 421 (Mrk 421) covering radio to gamma-rays, during the 4.5 year period of ARGO-YBJ and Fermi common…

astro-ph.IM2015★ 27 cited

The analog Resistive Plate Chamber detector of the ARGO-YBJ experiment

B. Bartoli, P. Bernardini, X. J. Bi +68

The ARGO-YBJ experiment has been in stable data taking from November 2007 till February 2013 at the YangBaJing Cosmic Ray Observatory (4300 m a.s.l.). The detector consists of a si…

hep-ex2015★ 41 cited

The cosmic ray proton plus helium energy spectrum measured by the ARGO-YBJ experiment in the energy range 3-300 TeV

YBJ Collaboration, B. Bartoli, P. Bernardini +70

The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray Observatory (Tibet, People's Republic of China, 4300 m a.s.l.). The high altitud…

astro-ph.HE2015★ 44 cited

Crab Nebula: five-year observation with ARGO-YBJ

YBJ Collaboration

The ARGO-YBJ air shower detector monitored the Crab Nebula gamma ray emission from 2007 November to 2013 February. The integrated signal, consisting of 3.3 10 ev…

astro-ph.HE2015★ 12 cited

Search for GeV Gamma Ray Bursts with the ARGO-YBJ Detector: Summary of Eight Years of Observations

B. Bartoli, P. Bernardini, X. J. Bi +78

The search for Gamma Ray Burst (GRB) emission in the energy range 1-100 GeV in coincidence with the satellite detection has been carried out using the Astrophysical Radiation with…