activity
20122019
most citedLong-term Monitoring on Mrk 501 for Its VHE gamma Emission and a Flare in October 2011

55 citations · 203 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE201910 cited

Search for gamma-ray emission from the Sun during solar minimum with the ARGO-YBJ experiment

B. Bartoli, P. Bernardini, X. J. Bi +70

The hadronic interaction of cosmic rays with solar atmosphere can produce high energy gamma rays. The gamma-ray luminosity is correlated both with the flux of primary cosmic rays a…

astro-ph.SR201814 cited

Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun

M. Amenomori, X. J. Bi, D. Chen +80

We analyze the Sun's shadow observed with the Tibet-III air shower array and find that the shadow's center deviates northward (southward) from the optical solar disc center in the…

astro-ph.HE201711 cited

EAS age determination from the study of the lateral distribution of charged particles near the shower axis with the ARGO-YBJ experiment

YBJ Collaboration, B. Bartoli, P. Bernardini +69

The ARGO-YBJ experiment, a full coverage extensive air shower (EAS) detector located at high altitude (4300 m a.s.l.) in Tibet, China, has smoothly taken data, with very high stabi…

astro-ph.IM201527 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…

astro-ph.HE201544 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.HE201512 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…