Zobrazeno 1 - 10
of 1 198
pro vyhledávání: '"BOGGS, S."'
Autor:
Aramaki, T., Boezio, M., Boggs, S. E., Bonvicini, V., Bridges, G., Campana, D., Craig, W. W., von Doetinchem, P., Everson, E., Fabris, L., Feldman, S., Fuke, H., Gahbauer, F., Gerrity, C., Ghislotti, L., Hailey, C. J., Hayashi, T., Kawachi, A., Kozai, M., Lazzaroni, P., Law, M., Lenni, A., Lowell, A., Manghisoni, M., Marcelli, N., Mizukoshi, K., Mocchiutti, E., Mochizuki, B., Mognet, S. A. I., Munakata, K., Munini, R., Okazaki, S., Olson, J., Ong, R. A., Osteria, G., Perez, K., Perfetto, F., Quinn, S., Re, V., Riceputi, E., Roach, B., Rogers, F., Ryan, J. L., Saffold, N., Scotti, V., Shimizu, Y., Shutt, K., Sparvoli, R., Stoessl, A., Tiberio, A., Vannuccini, E., Xiao, M., Yamatani, M., Yee, K., Yoshida, T., Zampa, G., Zeng, J., Zweerink, J.
Compilation of papers presented by the GAPS Collaboration at the 38th International Cosmic Ray Conference (ICRC), held July 26 through August 3, 2023 in Nagoya, Japan.
Externí odkaz:
http://arxiv.org/abs/2310.10181
Autor:
Saffold, N., Aramaki, T., Bird, R., Boezio, M., Boggs, S. E., Bonvicini, V., Campana, D., Craig, W. W., von Doetinchem, P., Everson, E., Fabris, L., Fuke, H., Gahbauer, F., Garcia, I., Gerrity, C., Hailey, C. J., Hayashi, T., Kato, C., Kawachi, A., Kobayashi, S., Kozai, M., Lenni, A., Lowell, A., Manghisoni, M., Marcelli, N., Mognet, S. I., Munakata, K., Munini, R., Nakagami, Y., Olson, J., Ong, R. A., Osteria, G., Perez, K., Pope, I., Quinn, S., Re, V., Reed, M., Riceputi, E., Roach, B., Rogers, F., Ryan, J. L., Scotti, V., Shimizu, Y., Sonzogni, M., Sparvoli, R., Stoessl, A., Tiberio, A., Vannuccini, E., Wada, T., Xiao, M., Yamatani, M., Yoshida, A., Yoshida, T., Zampa, G., Zweerink, J.
The General Antiparticle Spectrometer (GAPS) is an Antarctic balloon experiment designed for low-energy (0.1$-$0.3 GeV/$n$) cosmic antinuclei as signatures of dark matter annihilation or decay. GAPS is optimized to detect low-energy antideuterons, as
Externí odkaz:
http://arxiv.org/abs/2012.05834
Autor:
von Doetinchem, P., Perez, K., Aramaki, T., Baker, S., Barwick, S., Bird, R., Boezio, M., Boggs, S. E., Cui, M., Datta, A., Donato, F., Evoli, C., Fabris, L., Fabbietti, L., Bueno, E. Ferronato, Fornengo, N., Fuke, H., Gerrity, C., Coral, D. Gomez, Hailey, C., Hooper, D., Kachelriess, M., Korsmeier, M., Kozai, M., Lea, R., Li, N., Lowell, A., Manghisoni, M., Moskalenko, I. V., Munini, R., Naskret, M., Nelson, T., Ng, K. C. Y., Nozzoli, F., Oliva, A., Ong, R. A., Osteria, G., Pierog, T., Poulin, V., Profumo, S., Poeschl, T., Quinn, S., Re, V., Rogers, F., Ryan, J., Saffold, N., Sakai, K., Salati, P., Schael, S., Serksnyte, L., Shukla, A., Stoessl, A., Tjemsland, J., Vannuccini, E., Vecchi, M., Winkler, M. W., Wright, D., Xiao, M., Xu, W., Yoshida, T., Zampa, G., Zuccon, P.
Publikováno v:
JCAP08(2020)035
The precise measurement of cosmic-ray antinuclei serves as an important means for identifying the nature of dark matter and other new astrophysical phenomena, and could be used with other cosmic-ray species to understand cosmic-ray production and pro
Externí odkaz:
http://arxiv.org/abs/2002.04163
Autor:
Bird, R., Aramaki, T., Boezio, M., Boggs, S. E., Bonvicini, V., Campana, D., Craig, W. W., Everson, E., Fabris, L., Fuke, H., Gahbauer, F., Garcia, I., Gerrity, C., Hailey, C. J., Hayashi, T., Kato, C., Kawachi, A., Kondo, M., Kozai, M., Lowell, A., Manghisoni, M., Marcelli, N., Martucci, M., Mognet, S. I., Munakata, K., Munini, R., Okazaki, S., Olson, J., Ong, R. A., Osteria, G., Perez, K., Quinn, S., Re, V., Riceputi, E., Rogers, F., Ryan, J. L., Saffold, N., Scotti, V., Shimizu, Y., Sparvoli, R., Stoessl, A., Takeuchi, S., Vannuccini, E., von Doetinchem, P., Wada, T., Xiao, M., Yoshida, A., Yoshida, T., Zampa, G., Zweerink, J.
The General Antiparticle Spectrometer (GAPS) will carry out a sensitive dark matter search by measuring low-energy ($\mathrm{E} < 0.25 \mathrm{GeV/nucleon}$) cosmic ray antinuclei. The primary targets are low-energy antideuterons produced in the anni
Externí odkaz:
http://arxiv.org/abs/1908.03154
Autor:
Burns, E., Zhu, S., Hui, C. M., Ansoldi, S., Barthelmy, S., Boggs, S., Cenko, S. B., Christensen, N., Fryer, C., Goldstein, A., Harding, A., Hartmann, D., Joens, A., Kanbach, G., Kerr, M., Kierans, C., McEnery, J., Patricelli, B., Perkins, J., Racusin, J., Ray, P., Schlieder, J., Schoorlemmer, H., Schussler, F., Stamerra, A., Tomsick, J., Wadiasingh, Z., Wilson-Hodge, C., Younes, G., Zhang, B., Zoglauer, A.
The first multimessenger observation of a neutron star merger was independently detected in gamma-rays by Fermi-GBM and INTEGRAL SPI-ACS and gravitational waves by Advanced LIGO and Advanced Virgo. Gravitational waves are emitted from systems with ac
Externí odkaz:
http://arxiv.org/abs/1903.04472
Autor:
Vannuccini, E., Aramaki, T., Bird, R., Boezio, M., Boggs, S. E., Bonvicini, V., Campana, D., Craig, W. W., von Doetinchem, P., Everson, E., Fabris, L., Gahbauer, F., Gerrity, C., Fuke, H., Hailey, C. J., Hayashi, T., Kato, C., Kawachi, A., Kozai, M., Lowell, A., Martucci, M., Mognet, S. I., Munini, R., Munakata, K., Okazaki, S., Ong, R. A., Osteria, G., Perez, K., Quinn, S., Ryan, J., Re, V., Rogers, F., Saffold, N., Shimizu, Y., Sparvoli, R., Stoessl, A., Yoshida, A., Yoshida, T., Zampa, G., Zweerink, J.
The General Antiparticle Spectrometer (GAPS) is designed to carry out indirect dark matter search by measuring low-energy cosmic-ray antiparticles. Below a few GeVs the flux of antiparticles produced by cosmic-ray collisions with the interstellar med
Externí odkaz:
http://arxiv.org/abs/1812.06691
Autor:
Middleton, M. J., Walton, D. J., Alston, W., Dauser, T., Eikenberry, S., Jiang, Y-F, Fabian, A. C., Fuerst, F., Brightman, M., Marshall, H., Parker, M., Pinto, C., Harrison, F. A., Bachetti, M., Altamirano, D., Bird, A. J., Perez, G., Miller-Jones, J., Charles, P. A., Boggs, S., Christensen, F., Craig, W., Forster, K., Grefenstette, B., Hailey, C., Madsen, K., Stern, D., Zhang, W.
SS433 is the only Galactic binary system known to persistently accrete at highly super-critical (or hyper-critical) rates, similar to those in tidal disruption events, and likely needed to explain the rapid growth of those very high redshift quasars
Externí odkaz:
http://arxiv.org/abs/1810.10518
Autor:
Quinn, S., Aramaki, T., Bird, R., Boezio, M., Boggs, S. E., Bonvicini, V., Campana, D., Craig, W. W., von Doetinchem, P., Everson, E., Fabris, L., Gahbauer, F., Gerrity, C., Fuke, H., Hailey, C. J., Hayashi, T., Kato, C., Kawachi, A., Kozai, M., Lowell, A., Martucci, M., Mognet, S. I., Munini, R., Munakata, K., Okazaki, S., Ong, R. A., Osteria, G., Perez, K., Ryan, J., Re, V., Rogers, F., Saffold, N., Shimizu, Y., Sparvoli, R., Stoessl, A., Vannuccini, E., Yoshida, A., Yoshida, T., Zampa, G., Zweerink, J.
The General AntiParticle Spectrometer (GAPS) is a balloon-borne instrument designed to detect cosmic-ray antimatter using the novel exotic atom technique, obviating the strong magnetic fields required by experiments like AMS, PAMELA, or BESS. It will
Externí odkaz:
http://arxiv.org/abs/1809.09714
Autor:
Buisson, D. J. K., Parker, M. L., Kara, E., Vasudevan, R. V., Lohfink, A. M., Pinto, C., Fabian, A. C., Ballantyne, D. R., Boggs, S. E., Craig, F. E. Christensen W. W., Farrah, D., Hailey, C. J., Harrison, F. A., Ricci, C., Stern, D., Walton, D. J., Zhang, W. W.
We present two new NuSTAR observations of the narrow line Seyfert 1 (NLS1) galaxy Mrk 766 and give constraints on the two scenarios previously proposed to explain its spectrum and that of other NLS1s: relativistic reflection and partial covering. The
Externí odkaz:
http://arxiv.org/abs/1808.00014
Autor:
Ong, R. A., Aramaki, T., Bird, R., Boezio, M., Boggs, S. E., Carr, R., Craig, W. W., von Doetinchem, P., Fabris, L., Gahbauer, F., Gerrity, C., Fuke, H., Hailey, C. J., Kato, C., Kawachi, A., Kozai, M., Mognet, S. I., Munakata, K., Okazaki, S., Osteria, G., Perez, K., Re, V., Rogers, F., Saffold, N., Shimizu, Y., Yoshida, A., Yoshida, T., Zampa, G., Zweerink, J.
The GAPS experiment is designed to carry out a sensitive dark matter search by measuring low-energy cosmic ray antideuterons and antiprotons. GAPS will provide a new avenue to access a wide range of dark matter models and masses that is complementary
Externí odkaz:
http://arxiv.org/abs/1710.00452