activity
20032019
most citedTransverse momentum and collision energy dependence of high hadron suppression in Au+Au collisions at ultrarelativistic energies

717 citations · 3.3k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2019★ 280 cited

Measurement of the cosmic-ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

Q. An, R. Asfandiyarov, P. Azzarello +151

The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in th…

astro-ph.IM2019★ 77 cited

The on-orbit calibration of DArk Matter Particle Explorer

G. Ambrosi, Q. An, R. Asfandiyarov +155

The DArk Matter Particle Explorer (DAMPE), a satellite-based cosmic ray and gamma-ray detector, was launched on December 17, 2015, and began its on-orbit operation on December 24,…

hep-ex2019★ 1 cited

Response to Comment on Daya Bay's definition and use of Delta(m^2_ee)

The Day Bay Collaboration, D. Adey, F. P. An +190

The Daya Bay Collaboration responds to comments posted by S. Parke and R. Zukanovich Funchal regarding our use of Delta(m^2_ee).

hep-ex2018★ 44 cited

Improved Measurement of the Reactor Antineutrino Flux at Daya Bay

Daya Bay Collaboration, D. Adey, F. P. An +197

This work reports a precise measurement of the reactor antineutrino flux using 2.2 million inverse beta decay (IBD) events collected with the Daya Bay near detectors in 1230 days.…

astro-ph.HE2017★ 541 cited

Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons

G. Ambrosi, Q. An, R. Asfandiyarov +155

High energy cosmic ray electrons plus positrons (CREs), which lose energy quickly during their propagation, provide an ideal probe of Galactic high-energy processes and may enable…

physics.ins-det2017★ 14 cited

Seasonal Variation of the Underground Cosmic Muon Flux Observed at Daya Bay

F. P. An, A. B. Balantekin, H. R. Band +199

The Daya Bay Experiment consists of eight identically designed detectors located in three underground experimental halls named as EH1, EH2, EH3, with 250, 265 and 860 meters of wat…