Wang, Y., Bi, X. J., Cui, S. W., Ding, L. K., 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...
Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., 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...
Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., 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...
Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., 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...
The Solar Flare of the 14th of July 2000 (L3+C detector results) (2007)
Achard, P, Adriani, O, Aguilar-Benítez, M, Alcaraz, J, Alemanni, G, ...
Several experiments have reported observations on possible correlations between the flux of high energy muons and intense solar flares. If confirmed, these observations would have significant...
The solar flare of the 14th of July 2000 : L3+C detector results (2007)
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
Aims.Several experiments have reported observations on possible correlations between the flux of high energy muons and intense solar flares. If confirmed, these observations would have significant...
The solar flare of the 14th of July 2000 : L3+C detector results (2007)
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
Aims.Several experiments have reported observations on possible correlations between the flux of high energy muons and intense solar flares. If confirmed, these observations would have significant...
The solar flare of the 14th of July 2000 : L3+C detector results (2007)
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
Aims.Several experiments have reported observations on possible correlations between the flux of high energy muons and intense solar flares. If confirmed, these observations would have significant...
A search for flaring Very-High-Energy cosmic-ray sources with the L3+C muon spectrometer (2006)
Achard, P, Adriani, O, Aguilar-Benítez, M, Alcaraz, J, Alemanni, G, ...
The L3+C muon detector at the Cern electron-position collider, LEP, is used for the detection of very-high-energy cosmic \gamma-ray sources through the observation of muons of energies above 20, 30,...
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
The L3+C muon detector at the CERN electron-positron collider, LEP, is used for the detection of very-high-energy cosmic gamma-ray sources through the observation of muons of energies above 20, 30,...
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
The L3+C muon detector at the CERN electron-positron collider, LEP, is used for the detection of very-high-energy cosmic gamma-ray sources through the observation of muons of energies above 20, 30,...
Measurement of the atmospheric muon spectrum from 20 to 300 GeV (2005)
Achard, P., Adriani, O., Aguilar-Benitez, M., Vanden Akker, M., Alcaraz, J., Alemanni, G., ...
The absolute muon flux between 20 GeV and 300 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 degree to 58 degrees. Due to the large exposure of about 150 m2...
Measurement of the atmospheric muon spectrum from 20 to 300 GeV (2005)
Achard, P., Adriani, O., Aguilar-Benitez, M., Vanden Akker, M., Alcaraz, J., Alemanni, G., ...
The absolute muon flux between 20 GeV and 300 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 degree to 58 degrees. Due to the large exposure of about 150 m2...
Measurement of the atmospheric muon spectrum from 20 to 300 GeV (2005)
Achard, P., Adriani, O., Aguilar-Benitez, M., Vanden Akker, M., Alcaraz, J., Alemanni, G., ...
The absolute muon flux between 20 GeV and 300 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 degree to 58 degrees. Due to the large exposure of about 150 m2...
Search for antihelium in cosmic rays (2005)
Alcaraz, J., Alvisi, D., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., ...
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km. A total of 2.86 * 10^6 helium nuclei...
Search for antihelium in cosmic rays (2005)
Alcaraz, J., Alvisi, D., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., ...
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km. A total of 2.86 * 10^6 helium nuclei...
Search for antihelium in cosmic rays (2005)
Alcaraz, J., Alvisi, D., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., ...
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km. A total of 2.86 * 10^6 helium nuclei...
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth...
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth...
Measurement of the Atmospheric Muon Spectrum from 20 to 3000 GeV (2004)
Achard, P, Adriani, O, Aguilar-Benítez, M, Van Den Ancker, M E, Alcaraz, J, Alemanni, G, ...
The absolute muon flux between 20 GeV and 300 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 degree to 58 degrees. Due to the large exposure of about 150 m2...
Measurement of the atmospheric muon spectrum from 20 to 3000 GeV (2004)
Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., ...
The absolute muon flux between 20 and 3000 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0degrees to 58degrees. Due to the large exposure of about 150 m(2) sr...
Measurement of the atmospheric muon spectrum from 20 to 300 GeV (2004)
Achard, P., Adriani, O., Aguilar-Benitez, M., Vanden Akker, M., Alcaraz, J., Alemanni, G., ...
The absolute muon flux between 20 GeV and 300 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 degree to 58 degrees. Due to the large exposure of about 150 m2...
Measurement of the atmospheric muon spectrum from 20 to 300 GeV (2004)
Achard, P., Adriani, O., Aguilar-Benitez, M., Vanden Akker, M., Alcaraz, J., Alemanni, G., ...
The absolute muon flux between 20 GeV and 300 GeV is measured with the L3 magnetic muon spectrometer for zenith angles ranging from 0 degree to 58 degrees. Due to the large exposure of about 150 m2...
Performances of the $\simeq 100$ kg NaI (Tl) set-up of the DAMA experiment at Gran Sasso (2000)
Bernabei, R, Belli, P, Montecchia, F, Di Nicolantonio, W, Ignesti, G, Incicchitti, A, ...
On a further search for a yearly modulation of the rate in particle Dark Matter direct search (1999)
Bernabei, R, Belli, P, Montecchia, F, Di Nicolantonio, W, Ignesti, G, Incicchitti, A, ...
Search for antihelium in cosmic rays (1999)
Alcaraz, J., Alvisi, D., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., ...
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km. A total of 2.86 * 10^6 helium nuclei...
Search for antihelium in cosmic rays (1999)
Alcaraz, J., Alvisi, D., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., ...
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 in a 51.7 degree orbit at altitudes between 320 and 390 km. A total of 2.86 * 10^6 helium nuclei...
Bernabei, R., Belli, P., Montecchia, F., Di Nicolantonio, W., Incicchitti, A., Prosperi, D., ...
The DAMA experiments are running deep underground in the Gran Sasso National Laboratory. Several interesting results have been achieved so far. Here a maximum likelihood method to search for the WIMP...
Shadowing of cosmic rays by the sun near maximum or at the declining phase of solar activity (1996)
Amenomori, M, Dai, B Z, Ding, L K, Feng, Z Y, Hibino, K, Hotta, N, ...
Progress on wimp search with low activity scintillators (1996)
Belli, P., Bacci, C., Bernabei, R., Dai, C.J., Di Nicolantonio, W., Ding, L.K., ...
On the possibility to measure neutrino magnetic moment to $10^11$ $\mu_B$ (1996)
Barabanov, I. R., Belli, P., Bernabei, R., Besida, O., Cherehovsky, V.I., Dai, C. J., ...
Progress on wimp search with low activity scintillators (1996)
Belli, P., Bacci, C., Bernabei, R., Dai, C.J., Di Nicolantonio, W., Ding, L.K., ...
On the possibility to measure neutrino magnetic moment to $10^11$ $\mu_B$ (1996)
Barabanov, I. R., Belli, P., Bernabei, R., Besida, O., Cherehovsky, V.I., Dai, C. J., ...
Particle dark matter search with low activity scintillators: status report (1994)
Bacci, Cesare, Belli, P, Bernabei, R, Dai Chang Jiang, Di Nicolantonio, W, Ding, L K, ...
New limits on axial coupled WIMPs with scintillators (1994)
Belli, P., Bacci, C., Bernabei, R., Dai, C J., Di Nicolantonio, W., Ding, L K., ...
Status report on dark matter search with low activity scintillators (1994)
Bacci, C., Belli, P., Bernabei, R., Dai, C., Di Nicolantonio, W., Ding, L.K., ...
Particle dark matter search with low activity scintillators: status report (1994)
Bacci, C., Belli, P., Bernabei, R., Dai, C J., Di Nicolantonio, W., Ding, L K., ...
Pas de résumé
Dark matter search with calcium fluoride crystals (1994)
Bacci, C., Belli, P., Bernabei, R., Dai, C.J., Di Nicolantonio, W., Ding, L.K., ...
New limits on axial coupled WIMPs with scintillators (1994)
Belli, P., Bacci, C., Bernabei, R., Dai, C J., Di Nicolantonio, W., Ding, L K., ...
Status report on dark matter search with low activity scintillators (1994)
Bacci, C., Belli, P., Bernabei, R., Dai, C., Di Nicolantonio, W., Ding, L.K., ...