Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Meyers, Z. S."'
Autor:
Agarwal, S., Aguilar, J. A., Ali, S., Allison, P., Betts, M., Besson, D., Bishop, A., Botner, O., Bouma, S., Buitink, S., Cataldo, M., Clark, B. A., Coleman, A., Couberly, K., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, C., Glüsenkamp, T., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Henrichs, J., Heyer, N., Hornhuber, C., Hughes, K., Karg, T., Karle, A., Kelley, J. L., Korntheuer, M., Kowalski, M., Kravchenko, I., Krebs, R., Lahmann, R., Latif, U., Laub, P., Liu, C. -H., Marsee, M. J., Meyers, Z. S., Mikhailova, M., Monstein, C., Mulrey, K., Muzio, M., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Punsuebsay, N., Pyras, L., Ravn, M., Ryckbosch, D., Schlüter, F., Scholten, O., Seckel, D., Seikh, M. F. H., Stoffels, J., Terveer, K., Toscano, S., Tosi, D., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Vijai, A., Welling, C., Williams, D. R., Windischhofer, P., Wissel, S., Young, R., Zink, A.
The science program of the Radio Neutrino Observatory-Greenland (RNO-G) extends beyond particle astrophysics to include radioglaciology and, as we show herein, solar physics, as well. Impulsive solar flare observations not only permit direct measurem
Externí odkaz:
http://arxiv.org/abs/2404.14995
Autor:
Fijma, S., Rowlinson, A., Wijers, R. A. M. J., de Ruiter, I., de Blok, W. J. G., Chastain, S., van der Horst, A. J., Meyers, Z. S., van der Meulen, K., Fender, R., Woudt, P. A., Andersson, A., Zijlstra, A., Healy, J., Maccagni, F. M.
Transient surveys are a vital tool in exploring the dynamic universe, with radio transients acting as beacons for explosive and highly energetic astrophysical phenomena. However, performing commensal transient surveys using radio imaging can require
Externí odkaz:
http://arxiv.org/abs/2306.16383
Autor:
Aguilar, J. A., Allison, P., Besson, D., Bishop, A., Botner, O., Bouma, S., Buitink, S., Castiglioni, W., Cataldo, M., Clark, B. A., Coleman, A., Couberly, K., Curtis-Ginsberg, Z., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Eimer, A., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Henrichs, J., Heyer, N., Hornhuber, C., Hughes, K., Karg, T., Karle, A., Kelley, J. L., Korntheuer, M., Kowalski, M., Kravchenko, I., Krebs, R., Lahmann, R., Lehmann, P., Latif, U., Laub, P., Liu, C. H., Mammo, J., Marsee, M. J., Meyers, Z. S., Michaels, K., Mulrey, K., Muzio, M., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Plaisier, I., Punsuebsay, N., Pyras, L., Ryckbosch, D., Schlüter, F., Scholten, O., Seckel, D., Seikh, M. F. H., Smith, D., Stoffels, J., Southall, D., Terveer, K., Toscano, S., Tosi, D., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Vischer, J. Z., Welling, C., Williams, D. R., Wissel, S., Young, R., Zink, A.
Glacial ice is used as a target material for the detection of ultra-high energy neutrinos, by measuring the radio signals that are emitted when those neutrinos interact in the ice. Thanks to the large attenuation length at radio frequencies, these si
Externí odkaz:
http://arxiv.org/abs/2304.06181
Autor:
Aguilar, J. A., Allison, P., Besson, D., Bishop, A., Botner, O., Bouma, S., Buitink, S., Cataldo, M., Clark, B. A., Couberly, K., Curtis-Ginsberg, Z., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Eimer, A., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Henrichs, J., Heyer, N., Hornhuber, C., Hughes, K., Karg, T., Karle, A., Kelley, J. L., Korntheuer, M., Kowalski11, M., Kravchenko, I., Krebs, R., Lahmann, R., Latif, U., Mammo, J., Marsee, M. J., Meyers, Z. S., Michaels, K., Mulrey, K., Muzio, M., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Plaisier, I., Punsuebsay, N., Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Seikh, M. F. H., Smith, D., Stoffels, J., Southall, D., Terveer, K., Toscano, S., Tosi, D., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Vischer, J. Z., Welling, C., Williams, D. R., Wissel, S., Young, R., Zink, A.
We recently reported on the radio-frequency attenuation length of cold polar ice at Summit Station, Greenland, based on bistatic radar measurements of radio-frequency bedrock echo strengths taken during the summer of 2021. Those data also include ech
Externí odkaz:
http://arxiv.org/abs/2212.10285
Autor:
Aguilar, J. A., Allison, P., Beatty, J. J., Besson, D., Bishop, A., Botner, O., Bouma, S., Buitink, S., Cataldo, M., Clark, B. A., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Kravchenko, I., Krebs, R., Lahmann, R., Latif, U., Mammo, J., Meyers, Z. S., Michaels, K., Mulrey, K., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Pan, Y., Pandya, H., Plaisier, I., Punsuebsay, N., Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Seikh, M. F. H., Smith, D., Southall, D., Torres, J., Toscano, S., Tosi, D., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Welling, C., Williams, D. R., Wissel, S., Young, R., Zink, A.
Over the last 25 years, radiowave detection of neutrino-generated signals, using cold polar ice as the neutrino target, has emerged as perhaps the most promising technique for detection of extragalactic ultra-high energy neutrinos (corresponding to n
Externí odkaz:
http://arxiv.org/abs/2201.07846
Autor:
ARIANNA Collaboration, Anker, A., Baldi, P., Barwick, S. W., Beise, J., Besson, D. Z., Bouma, S., Cataldo, M., Chen, P., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Liu, J., Magnuson, M., McAleer, S., Meyers, Z. S., Nam, J., Nelles, A., Novikov, A., Paul, M. P., Persichilli, C., Plaisier, I., Pyras, L., Rice-Smith, R., Tatar, J., Wang, S. -H, Welling, C., Zhao, L.
Publikováno v:
JCAP04(2022)022
The ARIANNA detector is designed to detect neutrinos with energies above $10^{17}$eV. Due to the similarities in generated radio signals, cosmic rays are often used as test beams for neutrino detectors. Some ARIANNA detector stations are equipped wit
Externí odkaz:
http://arxiv.org/abs/2112.01501
Autor:
Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, H., Besson, D., Bingefors, N., Botner, O., Bouma, S., Buitink, S., Carter, K., Cataldo, M., Clark, B. A., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Krebs, R., Lahmann, R., Latif, U., Magnuson, M., Meures, T., Meyers, Z. S., Mulrey, K., Nelles, A., Novikov, A., Oberla, E., Oeyen, B., Pandya, H., Plaisier, I., Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Toscano, S., Tosi, D., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Welling, C., Wissel, S., Young, R., Zink, A.
Publikováno v:
Eur. Phys. J. C (2022) 82: 147
Starting in summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) will search for astrophysical neutrinos at energies >10 PeV by detecting the radio emission from particle showers in the ice around Summit Station, Greenland. We present an
Externí odkaz:
http://arxiv.org/abs/2107.02604
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:
Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, H., Besson, D., Bingefors, N., Botner, O., Buitink, S., Carter, K., Clark, B. A., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Feigl, N., Garcia-Fernandez, D., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Krebs, R., Lahmann, R., Magnuson, M., Meures, T., Meyers, Z. S., Nelles, A., Novikov, A., Oberla, E., Oeyen, B., Pandya, H., Plaisier, I., Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Toscano, S., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Welling, C., Wissel, S., Young, R., Zink, A.
Publikováno v:
JINST 16 P03025 2021
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:
http://arxiv.org/abs/2010.12279
Autor:
Collaboration, The IceCube-Gen2, Aartsen, M. G., Abbasi, R., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alispach, C., Allison, P., Amin, N. M., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Arlen, T. C., Auffenberg, J., Axani, S., Bagherpour, H., Bai, X., V., A. Balagopal, Barbano, A., Bartos, I., Bastian, B., Basu, V., Baum, V., Baur, S., Bay, R., Beatty, J. J., Becker, K. -H., Tjus, J. Becker, BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Bohmer, M., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Burley, R. T., Buscher, J., Busse, R. S., Bustamante, M., Campana, M. A., Carnie-Bronca, E. G., Carver, T., Chen, C., Chen, P., Cheung, E., Chirkin, D., Choi, S., Clark, B. A., Clark, K., Classen, L., Coleman, A., Collin, G. H., Connolly, A., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., Deaconu, C., De Clercq, C., DeLaunay, J. J., De Kockere, S., Dembinski, H., Deoskar, K., De Ridder, S., Desai, A., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., Dharani, S., Diaz, A., Díaz-Vélez, J. C., Dujmovic, H., Dunkman, M., DuVernois, M. A., Dvorak, E., Ehrhardt, T., Eller, P., Engel, R., Evans, J. J., Evenson, P. A., Fahey, S., Farrag, K., Fazely, A. R., Felde, J., Fienberg, A. T., Filimonov, K., Finley, C., Fischer, L., Fox, D., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, E., Garcia-Fernandez, D., Garrappa, S., Gartner, A., Gerhardt, L., Gernhaeuser, R., Ghadimi, A., Glaser, C., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Goswami, S., Grant, D., Grégoire, T., Griffith, Z., Griswold, S., Gündüz, M., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Hanson, J. C., Hanson, K., Hardin, J., Haugen, J., Haungs, A., Hauser, S., Hebecker, D., Heinen, D., Heix, P., Helbing, K., Hellauer, R., Henningsen, F., Hickford, S., Hignight, J., Hill, C., Hill, G. C., Hoffman, K. D., Hoffmann, B., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Holzapfel, K., Hoshina, K., Huang, F., Huber, M., Huber, T., Huege, T., Hughes, K., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jones, B. J. P., Jonske, F., Joppe, R., Kalekin, O., Kang, D., Kang, W., Kang, X., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Katori, T., Katz, U., Kauer, M., Keivani, A., Kellermann, M., Kelley, J. L., Kheirandish, A., Kim, J., Kin, K., Kintscher, T., Kiryluk, J., Kittler, T., Kleifges, M., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Koundal, P., Kovacevich, M., Kowalski, M., Krauss, C. B., Krings, K., Krückl, G., Kulacz, N., Kurahashi, N., Gualda, C. Lagunas, Lahmann, R., Lanfranchi, J. L., Larson, M. J., Latif, U., Lauber, F., Lazar, J. P., Leonard, K., Leszczyńska, A., Li, Y., Liu, Q. R., Lohfink, E., LoSecco, J., Mariscal, C. J. Lozano, Lu, L., Lucarelli, F., Ludwig, A., Lünemann, J., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Maggi, G., Mahn, K. B. M., Makino, Y., Mallik, P., Mancina, S., Mandalia, S., Mariş, I. C., Marka, S., Marka, Z., Maruyama, R., Mase, K., Maunu, R., McNally, F., Meagher, K., Medina, A., Meier, M., Meighen-Berger, S., Merz, J., Meyers, Z. S., Micallef, J., Mockler, D., Momenté, G., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Muth, P., Naab, R., Nagai, R., Nam, J., Naumann, U., Necker, J., Neer, G., Nelles, A., Nguyên, L. V., Niederhausen, H., Nisa, M. U., Nowicki, S. C., Nygren, D. R., Oberla, E., Pollmann, A. Obertacke, Oehler, M., Olivas, A., O'Sullivan, E., Pan, Y., Pandya, H., Pankova, D. V., Papp, L., Park, N., Parker, G. K., Paudel, E. N., Peiffer, P., Heros, C. Pérez de los, Petersen, T. C., Philippen, S., Pieloth, D., Pieper, S., Pinfold, J. L., Pizzuto, A., Plaisier, I., Plum, M., Popovych, Y., Porcelli, A., Rodriguez, M. Prado, Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Rehman, A., Reimann, R., Renschler, M., Renzi, G., Resconi, E., Reusch, S., Rhode, W., Richman, M., Riedel, B., Riegel, M., Roberts, E. J., Robertson, S., Roellinghoff, G., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Cantu, D. Rysewyk, Safa, I., Herrera, S. E. Sanchez, Sandrock, A., Sandroos, J., Sandstrom, P., Santander, M., Sarkar, S., Satalecka, K., Scharf, M., Schaufel, M., Schieler, H., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shaevitz, M. H., Sharma, A., Shefali, S., Silva, M., Smith, D., Smithers, B., Snihur, R., Soedingrekso, J., Soldin, D., Söldner-Rembold, S., Song, M., Southall, D., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stein, R., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Strotjohann, N. L., Stürwald, T., Stuttard, T., Sullivan, G. W., Taboada, I., Taketa, A., Tanaka, H. K. M., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tollefson, K., Tomankova, L., Tönnis, C., Torres, J., Toscano, S., Tosi, D., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Twagirayezu, J. P., Ty, B., Unger, E., Elorrieta, M. A. Unland, Vandenbroucke, J., van Eijk, D., van Eijndhoven, N., Vannerom, D., van Santen, J., Veberic, D., Verpoest, S., Vieregg, A., Vraeghe, M., Walck, C., Watson, T. B., Weaver, C., Weindl, A., Weinstock, L., Weiss, M. J., Weldert, J., Welling, C., Wendt, C., Werthebach, J., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissel, S. A., Wolf, M., Wood, T. R., Woschnagg, K., Wrede, G., Wren, S., Wulff, J., Xu, X. W., Xu, Y., Yanez, J. P., Yoshida, S., Yuan, T., Zhang, Z., Zierke, S., Zöcklein, M.
Publikováno v:
J.Phys.G 48 (2021) 6, 060501
The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messe
Externí odkaz:
http://arxiv.org/abs/2008.04323