X. J. Bi

An Updated Search of Steady TeV $\gamma-$Ray Point Sources in Northern Hemisphere Using the Tibet Air Shower Array (2008)

Wang, Y., Bi, X. J., Cui, S. W., Ding, L. K., Danzengluobu, Ding, X. H., ...

Using the data taken from Tibet II High Density (HD) Array (1997 February-1999 September) and Tibet-III array (1999 November-2005 November), our previous northern sky survey for TeV $\gamma-$ray...

The diffuse GeV-TeV $\gamma$-ray emission of the Cygnus region (2008)

Bi, X. J., Chen, T. L., Wang, Y., Yuan, Q.

The Milagro's observation shows that there is a strong diffuse multi-TeV $\gamma$-ray excess in the Cygnus region compared with the background estimated by GALPROP. While the GeV observation by EGRET...

New estimation of the spectral index of high-energy cosmic rays as determined by the Compton-Getting anisotropy (2007)

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., ...

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 data, we measure the...

Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : simulation and sensitivity (2007)

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., ...

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 energies above a few...

Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : physics goal and overview (2007)

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., ...

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 energies above a few...