Zobrazeno 1 - 10
of 858
pro vyhledávání: '"Lu, M.-Y."'
Autor:
Allison, P., Archambault, S., Beatty, J. J., Besson, D. Z., Bishop, A., Chen, C. C., Chen, C. H., Chen, P., Chen, Y. C., Clark, B. A., Clay, W., Connolly, A., Cremonesi, L., Dasgupta, P., Davies, J., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Flaherty, J., Friedman, E., Gaior, R., Hanson, J., Harty, N., Hendricks, B., Hoffman, K. D., Hong, E., Hsu, S. Y., Hu, L., Huang, J. J., Huang, M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Kim, K. -C., Kim, M. -C., Kravchenko, I., Krebs, R., Ku, Y., Kuo, C. Y., Kurusu, K., Landsman, H., Latif, U. A., Li, C. -J., Liu, T. -C., Lu, M. -Y., Madison, B., Madison, K., Mase, K., Meures, T., Nam, J., Nichol, R. J., Nir, G., Novikov, A., Nozdrina, A., Oberla, E., Osborn, J., Pan, Y., Pfendner, C., Punsuebsay, N., Roth, J., Seckel, D., Seikh, M. F. H., Shiao, Y. -S., Shultz, A., Smith, D., Toscano, S., Torres, J., Touart, J., van Eijndhoven, N., Varner, G. S., Vieregg, A., Wang, M. -Z., Wang, S. -H., Wang, Y. H., Wissel, S. A., Xie, C., Yoshida, S., Young, R.
In the pursuit of the measurement of the still-elusive ultrahigh-energy (UHE) neutrino flux at energies of order EeV, detectors using the in-ice Askaryan radio technique have increasingly targeted lower trigger thresholds. This has led to improved tr
Externí odkaz:
http://arxiv.org/abs/2202.07080
Autor:
Aguilar, J. A., Anker, A., Allison, P., Archambault, S., Baldi, P., Barwick, S. W., Beatty, J. J., Beise, J., Besson, D., Bishop, A., Bondarev, E., Botner, O., Bouma, S., Buitink, S., Cataldo, M., Chen, C. C., Chen, C. H., Chen, P., Chen, Y. C., Clark, B. A., Clay, W., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Flaherty, J., Friedman, E., Gaior, R., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Harty, N., Hendricks, B., Hoffman, K. D., Hornhuber, C., Hsu, S. Y., Hu, L., Huang, J. J., Huang, M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Klein, S. R., Kleinfelder, S. A., Kim, K. -C., Kim, M. -C., Kravchenko, I., Krebs, R., Ku, Y., Kuo, C. Y., Kurusu, K., Lahmann, R., Landsman, H., Latif, U., Li, C. -J., Liu, J., Liu, T. -C., Lu, M. -Y., Madison, K., Mammo, J., Mase, K., McAleer, S., Meures, T., Meyers, Z. S., Michaels, K., Mikhailova, M., Mulrey, K., Nam, J., Nichol, R. J., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Osborn, J., Pan, Y., Pandya, H., Paul, M. P., Persichilli, C., Plaisier, I., Punsuebsay, N., Pyras, L., Rice-Smith, R., Roth, J., Ryckbosch, D., Scholten, O., Seckel, D., Seikh, M. F. H., Shiao, Y. -S., Smith, D., Southall, D., Tatar, J., Torres, J., Toscano, S., Tosi, D., Touart, J., Broeck, D. J. Van Den, van Eijndhoven, N., Varner, G. S., Vieregg, A. G., Wang, M. -Z., Wang, S. -H, Wang, Y. H., Welling, C., Williams, D. R., Wissel, S., Xie, C., Yoshida, S., Young, R., Zhao, L., Zink, A.
The proposed IceCube-Gen2 (ICG2) seeks to instrument ~500 sq. km of Antarctic ice near the geographic South Pole with radio antennas, in order to observe the highest energy (E>1 EeV) neutrinos in the Universe. To this end, ICG2 will use the impulsive
Externí odkaz:
http://arxiv.org/abs/2103.06079
Autor:
ARA Collaboration, Allison, P., Archambault, S., Beatty, J. J., Beheler-Amass, M., Besson, D. Z., Beydler, M., Chen, C. C., Chen, C. H., Chen, P., Clark, B. A., Clay, W., Connolly, A., Cremonesi, L., Davies, J., de Kockere, S., de Vries, K. D., Deaconu, C., Duvernois, M., Friedman, E., Gaior, R., Hanson, J., Hanson, K., Hoffman, K. D., Hokanson-Fasig, B., Hong, E., Hsu, S. Y., Hu, L., Huang, J. J., Huang, M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Khandelwal, R., Kim, K. -C., Kim, M. -C., Kravchenko, I., Kurusu, K., Landsman, H., Latif, U. A., Laundrie, A., Li, C. -J., Liu, T. -C., Lu, M. -Y., Madison, B., Mase, K., Meures, T., Nam, J., Nichol, R. J., Nir, G., Novikov, A., Nozdrina, A., Oberla, E., O'Murchadha, A., Osborn, J., Pan, Y., Pfendner, C., Roth, J., Sandstrom, P., Seckel, D., Shiao, Y. -S., Shultz, A., Smith, D., Torres, J., Touart, J., van Eijndhoven, N., Varner, G. S., Vieregg, A. G., Wang, M. -Z., Wang, S. -H., Wissel, S. A., Yoshida, S., Young, R.
Publikováno v:
Phys. Rev. D 102, 043021 (2020)
The Askaryan Radio Array (ARA) is an ultra-high energy (UHE, $>10^{17}$ eV) neutrino detector designed to observe neutrinos by searching for the radio waves emitted by the relativistic products of neutrino-nucleon interactions in Antarctic ice. In th
Externí odkaz:
http://arxiv.org/abs/1912.00987
Autor:
Allison, P., Archambault, S., Beatty, J. J., Besson, D. Z., Chen, C. C., Chen, C. H., Chen, P., Christenson, A., Clark, B. A., Clay, W., Connolly, A., Cremonesi, L., Deaconu, C., Duvernois, M., Friedman, L., Gaior, R., Hanson, J., Hanson, K., Haugen, J., Hoffman, K. D., Hong, E., Hsu, S. Y., Hu, L., Huang, J. J., Huang, A. M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Khandelwal, R., Kim, M. -C., Kravchenko, I., Kruse, J., Kurusu, K., Kuwabara, T., Latif, U. A., Laundrie, A., Li, C. -J., Liu, T. -C., Lu, M. -Y., Madison, B., Mase, K., Meures, T., Nam, J., Nichols, R. J., Novikov, A., Nozdrina, A., Oberla, E., Pan, Y., Pfendner, C., Relich, M., Sandstrom, P., Seckel, D., Shiao, Y. S., Shultz, A., Smith, D., Song, M., Torres, J., Touart, J., Varner, G. S., Vieregg, A., Wang, M. Z., Wang, S. H., Wissel, S., Yoshida, S., Young, R.
We report on analysis of englacial radio-frequency (RF) pulser data received over horizontal baselines of 1--5 km, based on broadcasts from two sets of transmitters deployed to depths of up to 1500 meters at the South Pole. First, we analyze data col
Externí odkaz:
http://arxiv.org/abs/1908.10689
Autor:
Aguilar, J. A., Allison, P., Archambault, S., Beatty, J. J., Besson, D. Z., Botner, O., Buitink, S., Chen, P., Clark, B. A., Connolly, A., Deaconu, C., de Kockere, S., DuVernois, M. A., van Eijndhoven, N., Finley, C., Garcia, D., Hallgren, A., Halzen, F., Hanson, J., Hanson, K., Heros, C. Pérez de los, Hoffman, K. D., Hokanson-Fasig, B., Hughes, K., Hultqvist, K., Ishihara, A., Karle, A., Kelley, J. L., Klein, S. R., Kowalski, M., Kravchenko, I., Latif, U. A., Liu, T. C., Lu, M. -Y., Mase, K., Morse, R., Nam, J., Nelles, A., Oberla, E., Pfendner, C., Pan, Y., Plaisier, I., Prohira, S., Robertson, S., Rolla, J., Ryckbosch, D., Schröder, F. G., Seckel, D., Shultz, A., Smith, D., Southall, D., O'Sullivan, E., Toscano, S., Torres-Espinosa, J., Unger, E., Vieregg, A. G., de Vries, K., Wang, S. -H., Welling, C., Wissel, S. A., Yoshida, S.
RNO is the mid-scale discovery instrument designed to make the first observation of neutrinos from the cosmos at extreme energies, with sensitivity well beyond current instrument capabilities. This new observatory will be the largest ground-based neu
Externí odkaz:
http://arxiv.org/abs/1907.12526
Autor:
ARA Collaboration, Allison, P., Archambault, S., Bard, R., Beatty, J. J., Beheler-Amass, M., Besson, D. Z., Beydler, M., Chen, C. -C., Chen, C. -H., Chen, P., Clark, B., Clough, A., Connolly, A., Davies, J., Deaconu, C., DuVernois, M. A., Fender, C., Friedman, E., Hanson, J., Hanson, K., Haugen, J., Hoffman, K. D., Hong, E., Hsu, S. -Y., Hu, L., Huang, J. -J., Huang, M. -H., Ishihara, A., Karle, A., Kelley, J. L., Khandelwal, R., Kim, M., Kravchenko, I., Kruse, J., Kurusu, K., Landsman, H., Latif, U. A., Laundrie, A., Li, C. -J., Liu, T. C., Lu, M. -Y., Mase, K., Meures, T., Nam, J., Nichol, R. J., Nir, G., Oberla, E., O'Murchadha, A., Pan, Y., Ratzlaff, K., Roth, J., Sandstrom, P., Seckel, D., Shiao, Y. -S., Shultz, A., Song, M., Touart, J., Vieregg, A. G., Wang, M. -Z., Wang, S. -H., Wissel, S. A., Yoshida, S., Young, R.
The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) neutrino telescope at the South Pole consisting of an array of radio antennas aimed at detecting the Askaryan radiation produced by neutrino interactions in the ice. Currently, the experime
Externí odkaz:
http://arxiv.org/abs/1907.11125
Autor:
Aguilar, J.A., Anker, A., Allison, P., Archambault, S., Baldi, P., Barwick, S.W., Beatty, J.J., Beise, J., Besson, D., Bishop, A., Bondarev, E., Botner, O., Bouma, S., Buitink, S., Cataldo, M., Chen, C.C., Chen, C.H., Chen, P., Chen, Y.C., Choi, T., Clark, B.A., Clay, W., Curtis-Ginsberg, Z., Connolly, A., Cremonesi, L., Dasgupta, P., Davies, J., de Kockere, S., de Vries, K.D., Deaconu, C., DuVernois, M.A., Flaherty, J., Friedman, E., Gaior, R., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Ham, Y.-B., Hanson, J.C., Harty, N., Hendricks, B., Hoffman, K.D., Hong, E., Hornhuber, C., Hsu, S.Y., Hu, L., Huang, J.J., Huang, M.-H., Hughes, K., Ishihara, A., Jee, G., Jung, J., Karle, A., Kelley, J.L., Klein, S.R., Kleinfelder, S.A., Kim, J., Kim, K.-C., Kim, M.-C., Kravchenko, I., Krebs, R., Ku, Y., Kuo, C.Y., Kurusu, K., Kwon, Hyuck-Jin, Lahmann, R., Landsman, H., Latif, U., Lee, C., Leung, C.-H., Li, C.-J., Liu, J., Liu, T.-C., Lu, M.-Y., Madison, K., Mammo, J., Mase, K., McAleer, S., Meures, T., Meyers, Z.S., Michaels, K., Mikhailova, M., Mulrey, K., Nam, J., Nichol, R.J., Nir, G., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Osborn, J., Pan, Y., Pandya, H., Paul, M.P., Persichilli, C., Pfendner, C., Plaisier, I., Punsuebsay, N., Pyras, L., Rice-Smith, R., Roth, J., Ryckbosch, D., Scholten, O., Seckel, D., Seikh, M.F.H., Shiao, Y.-S., Shin, B.-K., Shultz, A., Smith, D., Southall, D., Tatar, J., Torres, J., Toscano, S., Tosi, D., Touart, J., Van Den Broeck, D.J., van Eijndhoven, N., Varner, G.S., Vieregg, A.G., Wang, M.-Z., Wang, S.-H., Wang, Y.H., Welling, C., Williams, D.R., Wissel, S., Xie, C., Yoshida, S., Young, R., Zhao, L., Zink, A.
Publikováno v:
In Astroparticle Physics March 2023 145
Autor:
Allison, P., Archambault, S., Bard, R., Beatty, J. J., Beheler-Amass, M., Besson, D. Z., Beydler, M., Bogdan, M., Chen, C. -C., Chen, C. -H., Chen, P., Clark, B. A., Clough, A., Connolly, A., Cremonesi, L., Davies, J., Deaconu, C., DuVernois, M. A., Friedman, E., Hanson, J., Hanson, K., Haugen, J., Hoffman, K. D., Hokanson-Fasig, B., Hong, E., Hsu, S. -Y., Hu, L., Huang, J. -J., Huang, M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Khandelwal, R., Kim, M., Kravchenko, I., Kruse, J., Kurusu, K., Landsman, H., Latif, U. A., Laundrie, A., Li, C. -J., Liu, T. C., Lu, M. -Y., Ludwig, A., Mase, K., Meures, T., Nam, J., Nichol, R. J., Nir, G., Oberla, E., OMurchadha, A., Pan, Y., Pfendner, C., Ransom, M., Ratzla, K., Roth, J., Sandstrom, P., Seckel, D., Shiao, Y. -S., Shultz, A., Smith, D., Song, M., Sullivan, M., Touart, J., Vieregg, A. G., Wang, M. -Z., Wang, S. -H., Wei, K., Wissel, S. A., Yoshida, S., Young, R.
Ultra-high energy neutrinos are detectable through impulsive radio signals generated through interactions in dense media, such as ice. Subsurface in-ice radio arrays are a promising way to advance the observation and measurement of astrophysical high
Externí odkaz:
http://arxiv.org/abs/1809.04573
Autor:
Allison, P., Archambault, S., Auffenberg, J., Bard, R., Beatty, J. J., Beheler-Amass, M., Besson, D. Z., Beydler, M., Bora, C., Chen, C. -C., Chen, C. -H., Chen, P., Clark, B. A., Clough, A., Connolly, A., Davies, J., Deaconu, C., DuVernois, M. A., Friedman, E., Fox, B., Gorham, P. W., Hanson, J., Hanson, K., Haugen, J., Hill, B., Hoffman, K. D., Hong, E., Hsu, S. -Y., Hu, L., Huang, J. -J., Huang, M. -H., Ishihara, A., Karle, A., Kelley, J. L., Khandelwal, R., Kim, M., Kravchenko, I., Kruse, J., Kurusu, K., Landsman, H., Latif, U. A., Laundrie, A., Li, C. -J., Liu, T. C., Lu, M. -Y., Mase, K., Maunu, R., Meures, T., Miki, C., Nam, J., Nichol, R. J., Nir, G., Oberla, E., ÓMurchadha, A., Pan, Y., Pfendner, C., Ratzlaff, K., Richman, M., Roth, J., Rotter, B., Sandstrom, P., Seckel, D., Shiao, Y. -S., Shultz, A., Song, M., Stockham, J., Stockham, M., Sullivan, M., Touart, J., Tu, H. -Y., Varner, G. S., Vieregg, A. G., Wang, M. -Z., Wang, S. -H., Wissel, S. A., Yoshida, S., Young, R.
The Askaryan Radio Array (ARA) reports an observation of radio emission coincident with the "Valentine's Day" solar flare on Feb. 15$^{\rm{th}}$, 2011 in the prototype "Testbed" station. We find $\sim2000$ events that passed our neutrino search crite
Externí odkaz:
http://arxiv.org/abs/1807.03335
Autor:
Allison, P., Archambault, S., Auffenberg, J., Bard, R., Beatty, J. J., Beheler-Amass, M., Besson, D. Z., Beydler, M., Brabec, C., Chen, C. -C., Chen, C. -H., Chen, P., Christenson, A., Clark, B. A., Connolly, A., Cremonesi, L., Deaconu, C., Duvernois, M., Friedman, L., Gaior, R., Gorham, P. W., Hanson, J., Hanson, K., Haugen, J., Hoffman, K. D., Hong, E., Hsu, S. -Y., Hu, L., Huang, J. -J., Huang, M. -H. A., Ishihara, A., Karle, A., Kelley, J. L., Khandelwal, R., Kim, M. -C., Kravchenko, I., Kuwabara, T., Landsman, H., Laundrie, A., Li, C. -J., Liu, T. C., Lu, M. -Y., Mase, K., Meures, T., Nam, J., Nichols, R. J., Nir, G., Novikov, A., Oberla, E., O'Murchadha, A., Pan, Y., Pfendner, C., Ratzlaff, K., Relich, M., Roth, J., Sandstrom, P., Seckel, D., Shiao, Y. -S., Shultz, A., Song, M., Touart, J., Varner, G. S., Vieregg, A., Wang, M. -Z., Wang, S. -H., Wissel, S., Yang, Y., Yoshida, S., Young, R.
Using data collected by the Askaryan Radio Array (ARA) experiment at the South Pole, we have used long-baseline propagation of radio-frequency signals to extract information on the radio-frequency index-of-refraction in South Polar ice. Owing to the
Externí odkaz:
http://arxiv.org/abs/1712.03301