Zobrazeno 1 - 10
of 113
pro vyhledávání: '"Thomas Meures"'
Autor:
Colin B. Adams, Giovanni Ambrosi, Michelangelo Ambrosio, Carla Aramo, Timothy Arlen, Wystan Benbow, Bruna Bertucci, Elisabetta Bissaldi, Jonathan Biteau, Massimiliano Bitossi, Alfonso Boiano, Carmela Bonavolontà, Richard Bose, Aurelien Bouvier, Mario Buscemi, Aryeh Brill, Anthony M. Brown, James H. Buckley, Rodolfo Canestrari, Massimo Capasso, Mirco Caprai, Paolo Coppi, Corbin E. Covault, Davide Depaoli, Leonardo Di Venere, Manel Errando, Stephan Fegan, Qi Feng, Emanuele Fiandrini, Amy Furniss, Markus Garczarczyk, Alasdair Gent, Nicola Giglietto, Francesco Giordano, Enrico Giro, Robert Halliday, Olivier Hervet, Gareth Hughes, Simone Incardona, Thomas B. Humensky, Maria Ionica, Weidong Jin, Caitlin A. Johnson, David Kieda, Frank Krennrich, Andrey Kuznetsov, Jon Lapington, Francesco Licciulli, Serena Loporchio, Giovanni Marsella, Vincenzo Masone, Kevin Meagher, Thomas Meures, Brent A. W. Mode, Samuel A. I. Mognet, Reshmi Mukherjee, Akira Okumura, Francesca R. Pantaleo, Riccardo Paoletti, Federico Di Pierro, Deivid Ribeiro, Luca Riitano, Emmet Roache, Duncan Ross, Julien Rousselle, Andrea Rugliancich, Marcos Santander, Michael Schneider, Harm Schoorlemmer, Ruo-Yu Shang, Brandon Stevenson, Leonardo Stiaccini, Hiroyasu Tajima, Leslie P. Taylor, Julian Thornhill, Luca Tosti, Giovanni Tripodo, Valerio Vagelli, Massimo Valentino, Justin Vandenbroucke, Vladimir V. Vassiliev, Scott P. Wakely, Jason J. Watson, Richard White, Patrick Wilcox, David A. Williams, Matthew Wood, Peter Yu, Adrian Zink
Publikováno v:
Journal of astronomical telescopes, instruments, and systems 8(01), 014007-1 (2022). doi:10.1117/1.JATIS.8.1.014007
Journal of astronomical telescopes, instruments, and systems 8(01), 014007-1 (2022). doi:10.1117/1.JATIS.8.1.014007
The prototype Schwarzschild-Couder Telescope (pSCT) is a candidate for a medium-sized telescope in the Cherenkov Telescope Array.
The prototype Schwarzschild-Couder Telescope (pSCT) is a candidate for a medium-sized telescope in the Cherenkov Telescope Array.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::366c77c9afc87484899e33221e2da98b
https://hdl.handle.net/10447/588451
https://hdl.handle.net/10447/588451
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:
G. Pareschi, Manel Errando, Corbin Covault, F. Di Pierro, S. I. Mognet, V. Masone, N. Giglietto, D. B. Kieda, L. Di Venere, E. Roache, M. Ambrosio, Julien Rousselle, Justin Vandenbroucke, D. Ribeiro, N. Otte, Maria Ionica, Alasdair E. Gent, F. R. Pantaleo, Enrico Giro, A. Boiano, K. Meagher, Serena Loporchio, E. Fiandrini, H. Tajima, Valerio Vagelli, Atsushi Okumura, Marcos Santander, B. A. W. Mode, Luca Tosti, S. Incardona, L. P. Taylor, E. Pueschel, G. Ambrosi, David A. Williams, M. Capasso, V. V. Vassiliev, M. Bitossi, P. I. Batista, Bruna Bertucci, J. H. Buckley, A. Brill, A. M. Brown, G. Tripodo, W. Jin, G. Marsella, Wystan Benbow, C. Bonavolontà, S. J. Fegan, Richard Bose, R. Shang, D. Depaoli, R. Paoletti, Jamie Holder, Rodolfo Canestrari, F. Licciulli, Andrea Rugliancich, Thomas Meures, M. Valentino, Amy Furniss, Olivier Hervet, C. B. Adams, Carla Aramo, R. A. Cameron, Q. Feng, T. B. Humensky, Elisabetta Bissaldi, L. Stiaccini, A. Zink, Reshmi Mukherjee, G. H. Tovmassian, L. Riitano, Ferdinando Giordano, R. Halliday, M. Caprai
The Schwarzschild-Couder Telescope (SCT) is a medium-sized telescope technology proposed for the Cherenkov Telescope Array. It uses a novel dual-mirror optical design that removes comatic aberrations across its entire field of view. The SCT camera em
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98707a0d4cb4c643196dd274c9f912fe
http://arxiv.org/abs/2109.06225
http://arxiv.org/abs/2109.06225
Autor:
Patrick Allison, K. D. de Vries, C.Y. Kuo, C. Xie, Alexander Novikov, Michael DuVernois, Eric Oberla, R. Gaior, K. Hughes, A. Karle, A. Nozdrina, M.-C. Kim, J. Davies, I. Kravchenko, J. Touart, Brian Clark, U. Latif, J. Flaherty, Thomas Meures, M.-Y. Lu, N. Harty, W. Clay, J. L. Kelley, M.-H. A. Huang, H. Landsman, A. Shultz, S. Archambault, M. Beydler, J. Roth, Stephanie Wissel, A. O'Murchadha, B. Hendricks, R. J. Nichol, N. Punsuebsay, Simona Toscano, S. Y. Hsu, K. Mase, E. Hong, Chun Hsiung Chen, S. De Kockere, Abigail G. Vieregg, Po-Hsun Chen, L. Cremonesi, A. Ishihara, J. J. Huang, Benjamin Hokanson-Fasig, G. Nir, M. Beheler-Amass, D. Z. Besson, K. Kurusu, P. Dasgupta, D. Seckel, Cosmin Deaconu, M. Z. Wang, R. Krebs, Y.H. Wang, J. C. Hanson, James C. Osborn, B. Madison, Y. Pan, Jiwoo Nam, Jorge Torres, P. Sandstrom, Yi Chen, A. Laundrie, E. Friedman, J. J. Beatty, K. D. Hoffman, Kael Hanson, N. van Eijndhoven, S. Yoshida, S. H. Wang, K.-C. Kim, Y. S. Shiao, Y. Ku, David J. Smith, Tsung-Che Liu, Amy Connolly, Carl Pfendner, R. D. Young, G. S. Varner, R. Khandelwal
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The Askaryan Radio Array (ARA) is a ground-based radio detector at the South Pole designed to capture Askaryan emission from ultra-high energy neutrinos interacting within the Antarctic ice. The newest ARA station has been equipped with a phased arra
Autor:
A. O'Murchadha, S. Yoshida, P. Dasgupta, K. Hughes, P. Sandstrom, I. Kravchenko, U. Latif, M. Beheler-Amass, J. Touart, Y.H. Wang, J. Flaherty, M.-H. A. Huang, C. Xie, Kael Hanson, David J. Smith, M. A. Huang, Y. S. Shiao, G. S. Varner, R. D. Young, Y. Pan, Tsung-Che Liu, W. Clay, J. Roth, R. Krebs, A. Ishihara, Eric Oberla, S. De Kockere, A. Karle, S. Y. Hsu, D. Z. Besson, N. Punsuebsay, K. D. de Vries, R. J. Nichol, H. Landsman, Patrick Allison, James C. Osborn, N. van Eijndhoven, M. Z. Wang, Po-Hsun Chen, Brian Clark, B. Madison, Michael DuVernois, G. Nir, Paramita Dasgupta, C.Y. Kuo, S. Archambault, Jorge Torres, A. Nozdrina, Cosmin Deaconu, Chun Hsiung Chen, Abigail G. Vieregg, K. Mase, E. Hong, R. Gaior, Y. Ku, Jiwoo Nam, A. Shultz, Thomas Meures, R. Khandelwal, D. Seckel, Stephanie Wissel, Yi Chen, K. Kurusu, M Beheler Amass, J. J. Beatty, N. Harty, J. L. Kelley, Simona Toscano, Amy Connolly, Carl Pfendner, S. H. Wang, K.-C. Kim, J. C. Hanson, B. Hendricks, K. D. Hoffman, A. Laundrie, E. Friedman, J. J. Huang, L. Cremonesi, M. Beydler, Benjamin Hokanson-Fasig, M.-Y. Lu, Alexander Novikov, M.-C. Kim, J. Davies
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Autor:
J. J. Beatty, Patrick Allison, Nick van Eijndhoven, Rose S Stanley, Dieder Van den Broeck, Krijn D. de Vries, A. Nozdrina, S. Prohira, Chung-Yun Kuo, K. Mulrey, Vesna Lukic, Cosmin Deaconu, John Ralston, Jiwoo Nam, Thomas Meures, Enrique Huesca Santiago, Jorge Torres, Amy Connolly, D. Z. Besson, Paramita Dasgupta, U. Latif, Simona Toscano, Dylan Frikken, Cade Sbrocco, Stephanie Wissel, Simon De Kockere, C. Hast, Eric Oberla
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Autor:
A. Ishihara, Y. Pan, Y. S. Shiao, Chun Hsiung Chen, J. Roth, C. Xie, P. Dasgupta, Yi Chen, M.-Y. Lu, M. Z. Wang, S. Y. Hsu, R. J. Nichol, N. van Eijndhoven, Myoungchul Kim, Eric Oberla, R. Gaior, R. D. Young, N. Harty, A. Karle, A. Nozdrina, Cosmin Deaconu, Amy Connolly, L. Cremonesi, Jorge Torres, Patrick Allison, Benjamin Hokanson-Fasig, K. Hughes, Abigail G. Vieregg, James C. Osborn, C.Y. Kuo, Jiwoo Nam, D. Seckel, B. Madison, A. Shultz, B. Hendricks, S. Yoshida, J. C. Hanson, S. H. Wang, A. Laundrie, Stephanie Wissel, K.-C. Kim, Thomas Meures, E. Friedman, M. Beydler, J. J. Huang, I. Kravchenko, N. Punsuebsay, Alexander Novikov, Y.H. Wang, Carl Pfendner, J. Touart, Kael Hanson, K. D. Hoffman, J. J. Beatty, Brian Clark, M. Beheler-Amass, J. L. Kelley, J. Davies, P. Sandstrom, D. Z. Besson, K. Mase, S. De Kockere, Simona Toscano, S. Archambault, E. Hong, U. Latif, K. Kurusu, Po-Hsun Chen, G. Nir, R. Krebs, H. Landsman, A. O'Murchadha, K. D. de Vries, J. Flaherty, W. Clay, David J. Smith, Tsung-Che Liu, G. S. Varner, Y. Ku, R. Khandelwal, Michael DuVernois, M.-H. A. Huang
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Autor:
Thomas Meures, P. Dasgupta, R. Krebs, R. D. Young, J. Flaherty, Y. S. Shiao, A. Ishihara, K. Mase, M. Beydler, Jiwoo Nam, J. Roth, W. Clay, I. Kravchenko, M.-H. A. Huang, S. Y. Hsu, M.-Y. Lu, J. L. Kelley, E. Hong, K. Kurusu, U. Latif, J. Touart, Simona Toscano, Patrick Allison, K. D. de Vries, R. Khandelwal, R. J. Nichol, A. Laundrie, E. Friedman, R. Gaior, C.Y. Kuo, L. Cremonesi, P. Sandstrom, Po-Hsun Chen, Benjamin Hokanson-Fasig, Cosmin Deaconu, G. Nir, Y.H. Wang, D. Z. Besson, N. Harty, Amy Connolly, Chun Hsiung Chen, Alexander Novikov, N. Punsuebsay, Brian Clark, A. O'Murchadha, M.-C. Kim, J. Davies, Carl Pfendner, G. S. Varner, Y. Ku, S. H. Wang, B. Hendricks, K.-C. Kim, Yue Pan, H. Landsman, M. Z. Wang, C. Xie, J. J. Huang, Michael DuVernois, David J. Smith, A. Shultz, Tsung-Che Liu, K. Hughes, James C. Osborn, M. Beheler-Amass, Stephanie Wissel, Jorge Torres, B. Madison, Eric Oberla, A. Karle, Abigail G. Vieregg, D. Seckel, S. Archambault, A. Nozdrina, S. De Kockere, Y. Pan, K. D. Hoffman, Kael Hanson, Yi Chen, S. Yoshida, N. van Eijndhoven, J. C. Hanson, J. J. Beatty
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) neutrino ($E_{\nu}$ > $10^{17}$ eV) detector at South Pole. ARA aims to utilize radio signals detected from UHE neutrino interactions in the glacial ice to infer properties about the intera
Autor:
J. J. Beatty, Patrick Allison, Rose S Stanley, Thomas Meures, Jiwoo Nam, D. Van den Broeck, Cade Sbrocco, D. Z. Besson, C. Hast, Paramita Dasgupta, Radar Echo Telescope, Simona Toscano, Katie Mulrey, U. Latif, S. Prohira, Vesna Lukic, S. De Kockere, Chung-Yun Kuo, Amy Connolly, John Ralston, A. Nozdrina, Jorge Torres, Dylan Frikken, N. van Eijndhoven, Stephanie Wissel, Cosmin Deaconu, K. D. de Vries, E. Huesca Santiago
Publikováno v:
Physical Review D, 103 (10
Physical Review D
Physical Review D
We investigate the use of parabolic equation (PE) methods for solving radio-wave propagation in polar ice. PE methods provide an approximate solution to Maxwell's equations, in contrast to full-field solutions such as finite-difference-time-domain (F
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2059eef2ff9451d8c68f2fe9fb5ce32b
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/324970
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/324970
Autor:
M. Beydler, D. Z. Besson, M. Relich, C. C. Chen, R. Gaior, Brian Clark, Patrick Allison, J. Roth, Eric Oberla, Y. S. Shiao, R. Young, Po-Hsun Chen, A. Karle, G. Nir, Alexander Novikov, J. C. Hanson, G. S. Varner, A. Ishihara, R. J. Nichol, T. Kuwabara, S. Archambault, S. Y. Hsu, J. L. Kelley, Y. Pan, M.-C. Kim, P. Sandstrom, Cosmin Deaconu, A. Shultz, Stephanie Wissel, E. Hong, Thomas Meures, M.-Y. Lu, A. Christenson, J. Auffenberg, M. Beheler-Amass, M. Z. Wang, J. J. Beatty, I. Kravchenko, Abigail G. Vieregg, J. Touart, R. Bard, L. Cremonesi, D. Seckel, A. Laundrie, U. Latif, J. J. Huang, Kara Hoffman, L. Hu, Amy Connolly, A. O’ Murchadha, R. Khandelwal, C.-J. Li, M. Song, S. H. Wang, Carl Pfendner, J. Kruse, Chun Hsiung Chen, J. Nam, Kenneth L. Ratzlaff, K. Mase, K. Kurusu, S. Yoshida, M.-H. A. Huang, Tsung-Che Liu, L. Friedman, J. Haugen, Kael Hanson, H. Landsman, Michael DuVernois
Publikováno v:
Astroparticle Physics. 108:63-73
Owing to their small interaction cross-section, neutrinos are unparalleled astronomical tracers. Ultra-high energy (UHE; E > 10 PeV) neutrinos probe the most distant, most explosive sources in the Universe, often obscured to optical telescopes. Radio