Zobrazeno 1 - 5
of 5
pro vyhledávání: '"P. H. Hüntemeyer"'
Autor:
C. P. Lansdell, James M. Ryan, B. E. Kolterman, D. Noyes, T. Aune, Brenda Dingus, David Berley, Peter Nemethy, J. T. Linnemann, C. M. Hoffman, G. W. Sullivan, B. T. Allen, R. W. Ellsworth, J. A. Goodman, R. Fleysher, P. H. Hüntemeyer, A. L. Shoup, A. J. Smith, M. M. Gonzalez, L. Fleysher, Allen Mincer, Sabrina Casanova, David A. Williams, A. A. Abdo, V. Vasileiou, B. Hopper, Julie McEnery, P. M. Saz Parkinson, G. P. Walker, Chang-Hsiao Chen, G. B. Yodh, J. Pretz, G. Sinnis
Publikováno v:
The Astrophysical Journal. 698:2121-2130
Results are presented of a harmonic analysis of the large scale cosmic-ray anisotropy as observed by the Milagro observatory. We show a two-dimensional display of the sidereal anisotropy pro jections in right ascension generated by the fitting of thr
Autor:
A. A. Abdo, U. Abeysekara, B. T. Allen, T. Aune, D. Berley, E. Bonamente, G. E. Christopher, T. DeYoung, B. L. Dingus, R. W. Ellsworth, J. G. Galbraith-Frew, M. M. Gonzalez, J. A. Goodman, C. M. Hoffman, P. H. Hüntemeyer, C. M. Hui, B. E. Kolterman, J. T. Linnemann, J. E. McEnery, A. I. Mincer, T. Morgan, P. Nemethy, J. Pretz, J. M. Ryan, P. M. Saz Parkinson, A. Shoup, G. Sinnis, A. J. Smith, V. Vasileiou, G. P. Walker, D. A. Williams, G. B. Yodh
The Cygnus region is a very bright and complex portion of the TeV sky, host to unidentified sources and a diffuse excess with respect to conventional cosmic-ray propagation models. Two of the brightest TeV sources, MGRO J2019+37 and MGRO J2031+41, ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63df1b8338bdd0680ea3e5a95d42b79a
http://arxiv.org/abs/1202.0846
http://arxiv.org/abs/1202.0846
Autor:
James M. Ryan, Peter Nemethy, R. Fleysher, C. M. Hoffman, E. Blaufuss, J. Pretz, P. M. Saz Parkinson, A. Shoup, G. P. Walker, L. Fleysher, R. W. Ellsworth, C. P. Lansdell, G. B. Yodh, B. E. Kolterman, A. A. Abdo, Benjamin William Allen, G. Sinnis, Maria Magdalena González, Julie McEnery, C. Chen, David A. Williams, D. Berley, P. H. Hüntemeyer, D. Noyes, Allen Mincer, A. J. Smith, J. T. Linnemann, Sabrina Casanova, T. Aune, J. A. Goodman, V. Vasileiou, Brenda Dingus, G. W. Sullivan
Publikováno v:
Physical Review Letters. 101
An analysis of 7 years of Milagro data performed on a 10-degree angular scale has found two localized regions of excess of unknown origin with greater than 12 sigma significance. Both regions are inconsistent with gamma-ray emission with high confide
Autor:
A. A. Abdo, J. T. Linnemann, D. Noyes, B. Hopper, G. W. Sullivan, Peter Nemethy, A. J. Smith, David A. Williams, James M. Ryan, G. Sinnis, Sabrina Casanova, X. W. Xu, B. E. Kolterman, J. A. Goodman, R. W. Ellsworth, C. P. Lansdell, R. Fleysher, P. M. Saz Parkinson, P. H. Hüntemeyer, G. B. Yodh, G. P. Walker, Benjamin William Allen, A. L. Shoup, E. Hays, D. G. Coyne, Allen Mincer, L. Fleysher, Brenda Dingus, M. M. Gonzalez, V. Vasileiou, C. Chen, J. E. McEnery, D. Berley, C. M. Hoffman
A survey of Galactic gamma-ray sources at a median energy of ~20 TeV has been performed using the Milagro Gamma Ray Observatory. Eight candidate sources of TeV emission are detected with pre-trials significance $>4.5\sigma$ in the region of Galactic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::590b4f57381843e61f27ecfb0f3c85ec
Autor:
A. A. Abdo, B. T. Allen, R. Atkins, T. Aune, W. Benbow, D. Berley, E. Blaufuss, E. Bonamente, J. Bussons, C. Chen, G. E. Christopher, D. G. Coyne, T. DeYoung, B. L. Dingus, D. E. Dorfan, R. W. Ellsworth, A. Falcone, L. Fleysher, R. Fleysher, J. Galbraith-Frew, M. M. Gonzalez, J. A. Goodman, T. J. Haines, E. Hays, C. M. Hoffman, P. H. Hüntemeyer, L. A. Kelley, B. E. Kolterman, C. P. Lansdell, J. T. Linnemann, J. McCullough, J. E. McEnery, T. Morgan, A. I. Mincer, M. F. Morales, P. Nemethy, D. Noyes, J. Pretz, J. M. Ryan, F. W. Samuelson, P. M. Saz Parkinson, A. Shoup, G. Sinnis, A. J. Smith, G. W. Sullivan, V. Vasileiou, G. P. Walker, M. Wascko, D. A. Williams, S. Westerhoff, G. B. Yodh
Publikováno v:
The Astrophysical Journal. 750:63
The Crab Nebula was detected with the Milagro experiment at a statistical significance of 17 standard deviations over the lifetime of the experiment. The experiment was sensitive to approximately 100 GeV - 100 TeV gamma ray air showers by observing t