249 citations · 1.1k across the 19 of their papers we have counts for
19 papers
GW170817 implications on the frequency and damping time of f-mode oscillations of neutron stars
De-Hua Wen, Bao-An Li, Hou-Yuan Chen +1
Within a minimum model for neutron stars consisting of nucleons, electrons and muons at -equilibrium using about a dozen Equation of States (EOSs) from microscopic nuclear many-…
Observation of TeV Gamma Rays from the Fermi Bright Galactic Sources with the Tibet Air Shower Array
M. Amenomori, X. J. Bi, D. Chen +81
Using the Tibet-III air shower array, we search for TeV gamma-rays from 27 potential Galactic sources in the early list of bright sources obtained by the Fermi Large Area Telescope…
Large-scale sidereal anisotropy of multi-TeV galactic cosmic rays and the heliosphere
M. Amenomori, X. J. Bi, D. Chen +83
We develop a model anisotropy best-fitting to the two-dimensional sky-map of multi-TeV galactic cosmic ray (GCR) intensity observed with the Tibet III air shower (AS) array. By inc…
The all-particle spectrum of primary cosmic rays in the wide energy range from 10^14 eV to 10^17 eV observed with the Tibet-III air-shower array
M. Amenomori
We present an updated all-particle energy spectrum of primary cosmic rays in a wide range from 10^14 eV to 10^17 eV using 5.5 times 10^7 events collected in the period from 2000 No…
New estimation of the spectral index of high-energy cosmic rays as determined by the Compton-Getting anisotropy
M. Amenomori, X. J. Bi, D. Chen +82
The amplitude of the Compton-Getting (CG) anisotropy contains the power-law index of the cosmic-ray energy spectrum. Based on this relation and using the Tibet air-shower array dat…
Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : physics goal and overview
M. Amenomori, X. J. Bi, D. Chen +82
The Tibet air shower array, which has an effective area of 37,000 square meters and is located at 4300 m in altitude, has been observing air showers induced by cosmic rays with ene…