Zobrazeno 1 - 10
of 350
pro vyhledávání: '"de Marco, D"'
Publikováno v:
In Cognition May 2022 222
Autor:
Besson, D. Z., Stockham, J., Sullivan, M., Allison, P., Barwick, S. W., Baughman, B. M., Beatty, J. J., Belov, K., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., De Marco, D., Dowkontt, P. F., DuVernois, M., Goldstein, D., Gorham, P. W., Grashorn, E. W., Hill, B., Hoover, S., Huang, M., Israel, M. H., Javaid, A., Kowalski, J., Learned, J., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Naudet, C. J., Nichol, R. J., Palladino, K., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Shang, R. Y., Stockham, M., Varner, G. S., Vieregg, A. G., Wang, Y.
From an elevation of ~38 km, the balloon-borne ANtarctic Impulsive Transient Antenna (ANITA) is designed to detect the up-coming radio frequency (RF) signal resulting from a sub-surface neutrino-nucleon collision. Although no neutrinos have been disc
Externí odkaz:
http://arxiv.org/abs/1301.4423
Autor:
Vieregg, A. G., Palladino, K., Allison, P., Baughman, B. M., Beatty, J. J., Belov, K., Besson, D. Z., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Detrixhe, M., De Marco, D., Dowkontt, P. F., DuVernois, M., Gorham, P. W., Grashorn, E. W., Hill, B., Hoover, S., Huang, M., Israel, M. H., Javaid, A., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Nichol, R. J., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G. S., Wang, Y.
Publikováno v:
ApJ 736 (2011) 50
We set the first limits on the ultra-high energy (UHE) neutrino fluence at energies greater than 10^9 GeV from gamma-ray bursts (GRBs) based on data from the second flight of the ANtarctic Impulsive Transient Antenna (ANITA). During the 31 day flight
Externí odkaz:
http://arxiv.org/abs/1102.3206
Autor:
Gorham, P. W., Allison, P., Baughman, B. M., Beatty, J. J., Belov, K., Besson, D. Z., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Detrixhe, M., De Marco, D., Dowkontt, P. F., DuVernois, M., Grashorn, E. W., Hill, B., Hoover, S., Huang, M., Israel, M. H., Javaid, A., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Nichol, R. J., Palladino, K., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Shang, R. Y., Varner, G. S., Vieregg, A. G., Wang, Y.
This is an erratum to our paper in Physical Review D82:022004,2010, corresponding to preprint: arXiv:1003.2961 .
Comment: 2 pages, 1 figure, 1 table. Erratum
Comment: 2 pages, 1 figure, 1 table. Erratum
Externí odkaz:
http://arxiv.org/abs/1011.5004
Autor:
The ANITA Collaboration, Gorham, P. W., Allison, P., Baughman, B. M., Beatty, J. J., Belov, K., Besson, D. Z., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Detrixhe, M., De Marco, D., Dowkontt, P. F., DuVernois, M., Grashorn, E. W., Hill, B., Hoover, S., Huang, M., Israel, M. H., Javaid, A., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Nichol, R. J., Palladino, K., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G. S., Vieregg, A. G., Wang, Y.
Publikováno v:
Phys.Rev.D82:022004,2010
The Antarctic Impulsive Transient Antenna (ANITA) completed its second long-duration balloon flight in January 2009, with 31 days aloft (28.5 live days) over Antarctica. ANITA searches for impulsive coherent radio Cherenkov emission from 200 to 1200
Externí odkaz:
http://arxiv.org/abs/1003.2961
Autor:
Berat, C., Bottai, S., De Marco, D., Moreggia, S., Naumov, D., Pallavicini, M., Pesce, R., Petrolini, A., Stutz, A., Taddei, E., Thea, A.
Publikováno v:
Astroparticle Physics Volume 33, Issue 4, May 2010, Pages 221-247
Future detection of Extensive Air Showers (EAS) produced by Ultra High Energy Cosmic Particles (UHECP) by means of space based fluorescence telescopes will open a new window on the universe and allow cosmic ray and neutrino astronomy at a level that
Externí odkaz:
http://arxiv.org/abs/0907.5275
Publikováno v:
Astropart.Phys. 23 (2005) 211-226
If ultra-high energy cosmic rays (UHECRs) are accelerated at astrophysical point sources, the identification of such sources can be achieved if there is some kind of radiation at observable wavelengths that may be associated with the acceleration and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0404352
Autor:
Romero-Wolf, A., Hoover, S., Vieregg, A.G., Gorham, P.W., Allison, P., Barwick, S.W., Baughman, B.M., Beatty, J.J., Belov, K., Besson, D.Z., Bevan, S., Binns, W.R., Chen, C., Chen, P., Clem, J.M., Connolly, A., Detrixhe, M., De Marco, D., Dowkontt, P.F., DuVernois, M., Goldstein, D., Grashorn, E.W., Hill, B., Huang, M., Israel, M.H., Javaid, A., Kowalski, J., Learned, J., Liewer, K.M., Matsuno, S., Mercurio, B.C., Miki, C., Mottram, M., Nam, J., Naudet, C.J., Nichol, R.J., Palladino, K., Ruckman, L., Saltzberg, D., Seckel, D., Shang, R.Y., Stockham, J., Stockham, M., Varner, G.S., Wang, Y.
Publikováno v:
In Astroparticle Physics January 2015 60:72-85
Publikováno v:
Journal of Enterprise Information Management, 2006, Vol. 19, Issue 5, pp. 465-482.
Externí odkaz:
http://www.emeraldinsight.com/doi/10.1108/17410390610703620
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