7 citations · 10 across the 7 of their papers we have counts for
7 papers
LHAASO-WCDA observed a 5 days TeV-delayed flaring event in blazar 1ES 1959+650
Zhen Cao, F. Aharonian, Y. X. Bai +339
We report a day-scale hard lag between GeV and TeV -ray emission from the HBL 1ES~1959+650 in early 2024. Since the LHAASO-WCDA real-time monitoring system began operation in la…
Anisotropic Particle Transport from a Pulsar Wind Nebula Revealed by Einstein Probe and LHAASO
Zhen Cao, F. Aharonian, Y. X. Bai +339
Pulsar wind nebulae (PWNe) are major cosmic ray accelerators, yet the mechanisms transporting high-energy particles into the interstellar medium remain elusive. Building on the LHA…
Observation of the Exotic State in
BESIII Collaboration, M. Ablikim, M. N. Achasov +750
A partial wave analysis of the process is performed using events collected with t…
First Observation of \boldmath{ and } in \boldmath{ and } Decays
BESIII Collaboration, M. Ablikim, M. N. Achasov +756
We perform the first amplitude analysis of the singly Cabibbo-suppressed decays , using collision data collected with the BESIII detector…
Measurement of the branching fractions of via
BESIII Collaboration, M. Ablikim, M. N. Achasov +762
Using events collected with the BESIII detector operating at BEPCII, the branching fractions of () are mea…
An extreme particle accelerator powered by pulsar PSR J1849-0001
The LHAASO Collaboration
Pulsar wind nebulae (PWNe) are bubbles of relativistic particles, powered by the rotational energy loss of the central pulsars. The Crab Nebula, powered by the Milky Way's most ene…
Improved measurement of the branching fraction of
BESIII Collaboration, M. Ablikim, M. N. Achasov +608
Using collision data with an integrated luminosity of collected at center-of-mass energies between 4.128 and 4.226 GeV with the BESIII detector ope…