Zobrazeno 1 - 10
of 18
pro vyhledávání: '"D. E. Alexandreas"'
Autor:
D. D. Weeks, David A. Williams, G. M. Dion, C. Y. Chang, Mike Stark, M. L. Chen, C. Dion, A. L. Shoup, R. L. Burman, J. P. Wu, G. E. Allen, W. Zhang, J. A. Goodman, S. R. Klein, P. Chumney, C. M. Hoffman, T. J. Haines, S. D. Biller, D. E. Dorfan, M. Cavalli-Sforza, G. B. Yodh, D. M. Schmidt, D. G. Coyne, R. Schnee, C. Sinnis, D. E. Nagle, D. Berley, Luke Zoltan Kelley, T. Yang, M. Harmon, D. E. Alexandreas, R. W. Ellsworth
Publikováno v:
Physical Review Letters. 71:2524-2527
Data taken with the CYGNUS detector between 1989 September and 1993 January have been used to search for 1 s bursts of ultrahigh-energy gamma rays from point sources at arbitrary locations in the northern sky. We find no evidence for such bursts. We
Autor:
D. Berley, C. Sinnis, G. B. Yodh, G. M. Dion, J. A. Goodman, D. E. Alexandreas, T. J. Haines, S. D. Biller, X. Q. Lu, E. Horch, W. Zhang, C. M. Hoffman
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 328:570-577
Searches for point astrophysical sources of ultra high energy (UHE) gamma rays are plagued by large numbers of background events from isotropic cosmic rays. Some of the methods that have been used to estimate the expected number of background events
Autor:
C. Sinnis, R. Cady, W. Zhang, P.R. Vishwanath, T. N. Thompson, M. Potter, V. D. Sandberg, C.A. Wilkinson, Todd Haines, G. B. Yodh, D. E. Alexandreas, S. D. Biller, R. L. Burman, C. Y. Chang, R. W. Ellsworth, D. E. Nagle, J. A. Goodman, Brenda Dingus, X. Q. Lu, R. L. Talaga, K. B. Butterfield, J. Lloyd-Evans, R. S. Delay, R. C. Allen, G. M. Dion, S. Stanislaus, C. M. Hoffman, S. Gupta, M. J. Stark, D. A. Krakauer, D. Berley
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 311:350-367
The CYGNUS extensive air-shower experiment is described. The design criteria, construction and operation details, and performance characteristics are presented. A discussion of the data analysis techniques is given. Finally, several enhancements and
Autor:
D. E. Nagle, D. Berley, D. A. Krakauer, P. W. Kwok, P. R. Vishwanath, J. A. Goodman, B. L. Dingus, R. C. Allen, D. R. Cady, W. P. Zhang, J. Lloyd-Evans, D. Dion, X. Q. Lu, G. M. Dion, S. Gupta, R. L. Burman, R. L. Talaga, D. E. Alexandreas, C. M. Hoffman, T. J. Haines, S. D. Biller, V. D. Sandberg, G. B. Yodh, C. Y. Chang, R. W. Ellsworth, M. E. Potter, Presented by D. E. Alexandreas, Mike Stark
Publikováno v:
AIP Conference Proceedings.
We report here the preliminary results of our observations of the sporadic X‐binary system 4U0115+63. The CYGNUS air shower array has been collecting data since April 1986. No significant excess is seen from the direction of this source, nor any co
Autor:
R. L. Talaga, J. Lloyd-Evans, D. E. Alexandreas, P. R. Vishwanath, M. K. Gilra, M. E. Potter, R. L. Burman, G. B. Yodh, C. M. Hoffman, D. A. Krakauer, P. W. Kwok, D. Berley, Mike Stark, S. Gupta, X. Q. Lu, C. Y. Chang, W. Zhang, R. C. Allen, G. M. Dion, D. R. Cady, V. D. Sandberg, R. W. Ellsworth, D. E. Nagle, Brenda Dingus, T. J. Haines, S. D. Biller, J. A. Goodman
Publikováno v:
Physical review. D, Particles and fields. 43(5)
Data from an extensive air shower detector of ultrahigh-energy cosmic rays shows shadowing of the cosmic-ray flux by the Moon and the Sun with significance of 4.9 standard deviations. This is the first observation of such shadowing. The effect has be
Autor:
Mike Stark, D. E. Nagle, J. A. Goodman, D. R. Cady, G. M. Dion, M. E. Potter, D. A. Krakauer, P. W. Kwok, C. M. Hoffman, J. Lloyd-Evans, C. Y. Chang, R. L. Burman, D. Berley, W. P. Zhang, G. B. Yodh, B. L. Dingus, D. E. Alexandreas, C. Dion, V. D. Sandberg, Presented by S. Biller, X. Q. Lu, R. W. Ellsworth, P. R. Vishwanath, T. J. Haines, S. D. Biller
Publikováno v:
AIP Conference Proceedings.
The 11 ‘‘in‐phase’’ source events from the 1986 muon‐rich bursts associated with Hercules X‐1 (previously reported by this group) have been studied for indications of further anomalous behavior. The most significant effect observed resu
Autor:
G. M. Dion, R. C. Allen, W. P. Zhang, D. Berley, P. R. Vishwanath, R. L. Talaga, J. Lloyd-Evans, Mike Stark, B. L. Dingus, X. Q. Lu, R. L. Burman, T. J. Haines, S. D. Biller, P. W. Kwok, G. B. Yodh, M. E. Potter, J. A. Goodman, R. Cady, D. E. Alexandreas, M. K. Gilra, V. D. Sandberg, D. E. Nagle, R. W. Ellsworth, C. M. Hoffman, C. Y. Chang
Publikováno v:
AIP Conference Proceedings.
A new method of searching for UHE point source has been developed. With a data sample of 150 million events, we have surveyed the sky for point sources over 3314 locations (1.4°
Autor:
D. A. Krakauer, P. W. Kwok, J. Lloyd-Evans, V. D. Sandberg, C. Y. Chang, Mike Stark, B. L. Dingus, D. Berley, G. M. Dion, P.R. Vishwanath, D. R. Cady, Presented by G. Dion, X. Q. Lu, D. E. Alexandreas, E. W. Ellsworth, M. E. Potter, R. L. Burman, T. J. Haines, S. D. Biller, G. B. Yodh, D. A. Nagle, J. A. Goodman, C. Dion, C. M. Hoffman, W. P. Zhang
Publikováno v:
AIP Conference Proceedings.
A preliminary search is made for continuously pulsed, and burst, emission from the Crab pulsar or its nebula at ultra‐high energies using the CYGNUS air shower experiment. No evidence is found for pulsed emission over the entire data set of 1,075 d
Autor:
J. A. Goodman, R. Cady, J. Lloyd-Evans, D. E. Nagle, R. L. Burman, D. Berley, P. R. Vishwanath, B. L. Dingus, G. B. Yodh, Mike Stark, R. C. Allen, R. L. Talaga, D. E. Alexandreas, G. M. Dion, T. J. Haines, S. D. Biller, X. Q. Lu, C. M. Hoffman, V. D. Sandberg, W. P. Zhang, C. Y. Chang, R. W. Ellsworth, M. E. Potter, D. A. Krakauer, P. W. Kwok
Publikováno v:
AIP Conference Proceedings.
Data from the CYGNUS extensive air shower experiment at Los Alamos, NM has been analyzed to study the angular resolution of the array, and to search for point sources in the galaxy. Results on searches for steady emission from Cyg X‐3, Her X‐1 an
Autor:
M. E. Potter, R. L. Talaga, R. L. Burman, S. D. Biller, X. Q. Lu, R. Cady, J. A. Goodman, P. R. Vishwanath, C. M. Hoffman, V. D. Sandberg, Mike Stark, J. Lloyd-Evans, G. M. Dion, R. W. Ellsworth, W. Zhang, C. Y. Chang, G. B. Yodh, R. C. Allen, D. E. Nagle, Brenda Dingus, D. Berley, D. E. Alexandreas, Todd Haines
Publikováno v:
Physical review letters. 64(25)
A unique feature of Cygnus X-3 is that occasionally it has large radio outbursts that begin very abruptly and last for several days. Several experiments in the past have claimed to observe signals above 1 TeV correlated with these radio bursts; the m