Zobrazeno 1 - 10
of 32
pro vyhledávání: '"David Zeke Besson"'
Autor:
Zachary S. Meyers, Allan Hallgren, Katie Carter, Anna Nelles, Thomas Meures, Ryan Krebs, Lilly Pyras, Krijn D. de Vries, N. Bingefors, John L. Kelley, Patrick Allison, U. Latif, Benjamin Hokanson-Fasig, Juan A. Aguilar, Dieder J. Van Den Broeck, Simon De Kockere, R. Lahmann, Ilse Plaisier, Stephanie Wissel, David Zeke Besson, Jorge Torres, M. A. DuVernois, Mitchell Magnuson, Simona Toscano, Kaeli Hughes, D. Tosi, Christian Glaser, Maddalena Cataldo, Bob Oeyen, Dirk Ryckbosch, Robert Young, Rno-g, Steffen Hallmann, Cosmin Deaconu, Zachary Curtis-Ginsberg, Daniel Southall, J. J. Beatty, Daniel Smith, Hans Bernhoff, C. Hornhuber, Katharine Mulrey, Paramita Dasgupta, Olga Botner, Sjoerd Bouma, Olaf Scholten, D. Seckel, Brian Clark, Alexander Novikov, Amy Connolly, Christoph Welling, Spencer Klein, Hershal Pandya, Stijn Buitink, Bryan Hendricks, Nick van Eijndhoven, Eric Oberla, A. Karle, Abigail G. Vieregg, Adrian Zink, Jordan C. Hanson
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The Radio Neutrino Observatory Greenland (RNO-G) is scheduled for deployment in the summerof 2021. It will target the detection of astrophysical and cosmogenic neutrinos above 10 PeV. With 35 autonomous stations, it will be the largest implementation
Autor:
B. K. Shin, Tsung-Che Liu, Christian Hornhuber, David Zeke Besson, Min-Zu Wang, Jiwoo Nam, Jian-Jung Huang, M.-H. A. Huang, Shih-Ying Hsu, Pisin Chen, Chung Hei Leung, Yaocheng Chen, Alexander Novikov, Yu-Hsin Wang, Chung-Yun Kuo, R. Young, Shih-Hao Wang
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
We present a portable calibration pulser system applied to radio antennas in order to detect ultra-high energy cosmic rays and neutrinos. The system consists of a solid-state high-voltage impulse generator, a digital attenuator, a wide band (150-350
Autor:
J. J. Beatty, Hans Bernhoff, Robert Lahmann, C. Hornhuber, Christian Glaser, Daniel P. Smith, Lilly Pyras, J. L. Kelley, Alexander Novikov, M. A. DuVernois, Brian Hendricks, Stijn Buitink, Cosmin Deaconu, Ilse Plaisier, Mitchell Magnuson, Albrecht Karle, Eric Oberla, K. D. de Vries, Steffen Hallmann, Paramita Dasgupta, Brian Clark, Adrian Zink, N. van Eijndhoven, H. Pandya, Dirk Ryckbosch, P. Allison, S. Toscano, Olga Botner, Daniel Southall, Abigail G. Vieregg, D. Van den Broeck, Jorge Torres, Zachary S. Meyers, C. Welling, Daniel García-Fernández, Katie Carter, Anna Nelles, Ryan Krebs, N. Bingefors, Olaf Scholten, A. Connolly, D. Seckel, S. De Kockere, Robert Young, N. Feigl, Allan Hallgren, J. C. Hanson, Stephanie Wissel, T. Meures, Kaeli Hughes, Bob Oeyen, Ben Hokanson-Fasig, David Zeke Besson, Juanan Aguilar, Spencer Klein
Publikováno v:
Journal of Instrumentation 16(03), P03025 (2021). doi:10.1088/1748-0221/16/03/P03025
Journal of Instrumentation, 16 (03
Journal of Instrumentation
JOURNAL OF INSTRUMENTATION
Journal of Instrumentation, 16 (03
Journal of Instrumentation
JOURNAL OF INSTRUMENTATION
This article presents the design of the Radio Neutrino Observatory Greenland (RNO-G) and discusses its scientific prospects. Using an array of radio sensors, RNO-G seeks to measure neutrinos above 10 PeV by exploiting the Askaryan effect in neutrino-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::197f99a83d50deaf04caf8734c596861
https://biblio.vub.ac.be/vubir/design-and-sensitivity-of-the-radio-neutrino-observatory-in-greenland-rnog(1f7c6874-70e6-4c1e-ac64-03eb6c745832).html
https://biblio.vub.ac.be/vubir/design-and-sensitivity-of-the-radio-neutrino-observatory-in-greenland-rnog(1f7c6874-70e6-4c1e-ac64-03eb6c745832).html
Autor:
K. Mulrey, John Clem, David Zeke Besson, Kurt Liewer, B. D. Fox, P. Cao, R. Prechelt, C. Naudet, Jiwoo Nam, K. Hughes, Chun Hsiung Chen, N. Wang, B. Strutt, K. McBride, Michael Sutherland, Jarred Matthew Roberts, Eric Oberla, Christian Miki, D. Seckel, Konstantin Belov, H. Schoorlemmer, R. Hupe, S. Stafford, Abigail G. Vieregg, Tsung-Che Liu, S. H. Wang, W. R. Binns, J. J. Beatty, J. J. Huang, O. Banerjee, Alexander Novikov, B. Dailey, G. S. Varner, M. H. Israel, P. Allison, Pisin Chen, V. Bugaev, Paul Dowkontt, David Saltzberg, P. W. Gorham, Luca Macchiarulo, Berkeley Hill, L. Cremonesi, C. Hast, Stephanie Wissel, J. W. H. Gordon, J. W. Russell, S. Y. Hsu, Cosmin Deaconu, J. Stockham, Andrew Ludwig, A. Connolly, S. Matsuno, M. Stockham, L. Batten, Andrew Romero-Wolf, S. Prohira, R. J. Nichol, Brian Rauch, Yung-Yaw Chen, J. Ripa, B. Rotter, J. Shiao
The ANtarctic Impulsive Transient Antenna (ANITA) long-duration balloon experiment is sensitive to interactions of ultra high-energy (E > 10^{18} eV) neutrinos in the Antarctic ice sheet. The third flight of ANITA, lasting 22 days, began in December
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d562ae13c8f2f392b7f38217769ab1ba
Autor:
David J. Smith, Tsung-Che Liu, Cosmin Deaconu, R. J. Nichol, Paramita Dasgupta, J. J. Beatty, David Saltzberg, Pisin Chen, P. Allison, L. Batten, Brian Rauch, P. Cao, Alexander Novikov, V. Bugaev, C. Miki, M. H. Israel, Abigail G. Vieregg, S. Prohira, A. Ludwig, John Clem, Stephanie Wissel, W. R. Binns, R. Prechelt, Chun Hsiung Chen, S. Matsuno, David Zeke Besson, G. S. Varner, Eric Oberla, Jiwoo Nam, Peter Gorham, A. Connolly, L. Cremonesi, J. W. Russell, D. Seckel
The balloon-borne ANITA [1] experiment is designed to detect ultra-high energy neutrinos via radio emissions produced by in-ice showers. Although initially purposed for interactions within the Antarctic ice sheet, ANITA also demonstrated the ability
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bea39d231567c24d9181e8275ecd5d9d
Autor:
Ilya Kravchenko, David Zeke Besson
Publikováno v:
The Cryosphere, Vol 7, Iss 3, Pp 855-866 (2013)
Using hardware developed for the ARA (Askaryan Radio Array) particle astrophysics experiment, we herein report on the amplitude and temporal characteristics of polarized surface radar echo data collected in South Polar ice using radio sounding equipm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33184b59b695fa8d0075c11f9e9a5984
https://www.the-cryosphere.net/7/855/2013/
https://www.the-cryosphere.net/7/855/2013/
Autor:
David Zeke Besson, Tim Huege
Publikováno v:
Progress of Theoretical and Experimental Physics. 2017
Radio waves, perhaps because they are uniquely transparent in our terrestrial atmosphere, as well as the cosmos beyond, or perhaps because they are macroscopic, so the basic instruments of detection (antennas) are easily constructable, arguably occup
Autor:
Gordon Thomson, S. Prohira, Daisuke Ikeda, U. Latif, Krijn de Vries, Thomas Meures, Krijn D. de Vries, Simona Toscano, Rasha Abbasi, Kael Hanson, David Zeke Besson, Joshua Macy, B. K. Shin, Aongus O'Murchadha, Michael DuVernois, John N. Matthews, John Belz
Publikováno v:
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017).
Recently the radar scattering technique to probe neutrino induced particle cascades above PeV energies in ice was investigated. The feasibility of the radar detection method was shown to crucially depend on several up to now unknown plasma properties
Publikováno v:
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017).
The Askaryan Radio Array (ARA) operates two stations (ARA-2, ARA-3) each with 16 antennas deployed on the corners of a cuboid at depths of 175-200 m at South Pole. The antennas are sensitive to either vertical (8 antennas) or horizontal (8 antennas)
Autor:
David Zeke Besson
Publikováno v:
Proceedings of 38th International Conference on High Energy Physics — PoS(ICHEP2016).
The Belle-II experiment will begin ramping up data collection at the SuperKEKB accelerator facility in Tsukuba, Japan, within the next 1-2 years. Projecting peak luminosities approximately 40 times higher than KEKB, Belle-II is expected to accumulate