Zobrazeno 1 - 10
of 4 416
pro vyhledávání: '"Tashiro, M"'
Autor:
Gandhi, P., Kawamuro, T., Trigo, M. Díaz, Paice, J. A., Boorman, P. G., Cappi, M., Done, C., Fabian, A. C., Fukumura, K., Garcia, J. A., Greenwell, C. L., Guainazzi, M., Makishima, K., Tashiro, M. S., Tomaru, R., Tombesi, F., Ueda, Y.
Microcalorimeters have demonstrated success in delivering high spectral resolution, and have paved the path to revolutionary new science possibilities in the coming decade of X-ray astronomy. There are several research areas in compact object science
Externí odkaz:
http://arxiv.org/abs/2209.10576
Autor:
Svinkin, D., Hurley, K., Ridnaia, A., Lysenko, A., Frederiks, D., Golenetskii, S., Tsvetkova, A., Ulanov, M., Kokomov, A., Cline, T. L., Mitrofanov, I., Golovin, D., Kozyrev, A., Litvak, M., Sanin, A., Goldstein, A., Briggs, M. S., Wilson-Hodge, C., Burns, E., von Kienlin, A., Zhang, X. -L., Rau, A., Savchenko, V., Bozzo, E., Ferrigno, C., Barthelmy, S., Cummings, J., Krimm, H., Palmer, D. M., Tohuvavohu, A., Yamaoka, K., Ohno, M., Fukazawa, Y., Hanabata, Y., Takahashi, T., Tashiro, M., Terada, Y., Murakami, T., Makishima, K., Boynton, W., Fellows, C. W., Harshman, K. P., Enos, H., Starr, R., Goldsten, J., Gold, R., Ursi, A., Tavani, M., Bulgarelli, A., Casentini, C., Del Monte, E., Evangelista, Y., Galli, M., Longo, F., Marisaldi, M., Parmiggiani, N., Pittori, C., Romani, M., Verrecchia, F., Smith, D. M., Hajdas, W., Xiao, S., Cai, C., Yi, Q. B., Zhang, Y. Q., Xiong, S. L., Li, X. B., Huang, Y., Li, C. K., Zhang, S. N., Song, L. M., Liu, C. Z., Li, X. Q., Peng, W. X., Martinez-Castellanos, I.
Publikováno v:
ApJS 259, 34 (2022)
We present the catalog of Interplanetary Network (IPN) localizations for 199 short-duration gamma-ray bursts (sGRBs) detected by the Konus-Wind (KW) experiment between 2011 January 1 and 2021 August 31, which extends the initial sample of IPN localiz
Externí odkaz:
http://arxiv.org/abs/2203.08738
Autor:
Yamashita, M., Tashiro, M., Saiki, K., Yamada, S., Akazawa, M., Shimozawa, M., Taniguchi, T., Takeda, H., Takigawa, M., Shishido, H.
Publikováno v:
Phys. Rev. B 102, 165154 (2020)
We have performed $^{59}$Co NMR measurements of CeCoIn$_5$ down to ultralow temperatures. We find that the temperature dependence of the spin-echo intensity provides a good measure of the sample temperature, enabling us to determine a pulse condition
Externí odkaz:
http://arxiv.org/abs/2004.11730
A new scheme to determine the neutrino mass matrix is proposed using atomic de-excitation between two states of a few eV energy spacing. The determination of the smallest neutrino mass of the order of 1 meV and neutrino mass type, Majorana or Dirac,
Externí odkaz:
http://arxiv.org/abs/1911.01639
Autor:
Huang, K. Y., Shimoda, J., Urata, Y., Toma, K., Yamaoka, K., Asada, K., Nagai, H., Takahashi, S., Petitpas, G., Tashiro, M.
We present the first radio polarimetric observations of a fast-rising blue optical transient, AT2018cow. Two epochs of polarimetry with additional coincident photometry were performed with the Atacama Large Millimeter/submillimeter Array (ALMA). The
Externí odkaz:
http://arxiv.org/abs/1905.09785
Autor:
Urata, Y., Toma, K., Huang, K., Asada, K., Nagai, H., Takahashi, S., Petitpas, G., Tashiro, M., Yamaoka, K.
We report the first detection of radio polarization of a GRB afterglow with the first intensive combined use of telescopes in the millimeter and submillimeter ranges for GRB171205A. The linear polarization degree in the millimeter band at the sub-per
Externí odkaz:
http://arxiv.org/abs/1904.08111
Autor:
Ohno, M., Kawano, T., Tashiro, M. S., Ueno, H., Yonetoku, D., Sameshima, H., Takahashi, T., Seta, H., Mushotzky, R., Yamaoka, K., team, ASTRO-H SWG, collaborations, Fermi LAT/GBM
ASTRO-H, the sixth Japanese X-ray observatory, which is scheduled to be launched by the end of Japanese fiscal year 2015 has a capability to observe the prompt emission from Gamma-ray Bursts (GRBs) utilizing BGO active shields for the soft gamma-ray
Externí odkaz:
http://arxiv.org/abs/1503.01182
Autor:
Tashiro, M. S., Yonetoku, D., Ohno, M., Sameshima, H., Seta, H., Ueno, H., Nakagawa, T., Tamura, T., Paerels, F., Kawai, N.
In this paper, we demonstrate ASTRO-H's capability to measure the chemical evolution in the high-z (z <~ 3) universe by observing X-ray afterglows of gamma-ray bursts (GRBs) and distant Blazars. Utilizing these sources as background light sources, th
Externí odkaz:
http://arxiv.org/abs/1412.1179
Autor:
Walker, E. S., Mazzali, P. A., Pian, E., Hurley, K., Arcavi, I., Cenko, S. B., Gal-Yam, A., Horesh, A., Kasliwal, M., Poznanski, D., Silverman, J. M., Sullivan, M., Bloom, J. S., Filippenko, A. V., Kulkarni, S. R., Nugent, P. E., Ofek, E., Barthelmy, S., Boynton, W., Goldsten, J., Golenetskii, S., Ohno, M., Tashiro, M. S., Yamaoka, K., Zhang, X. L-.
We present optical photometry and spectroscopy of the broad-lined Type Ic supernova (SNIc-BL) PTF10qts, which was discovered as part of the Palomar Transient Factory. The supernova was located in a dwarf galaxy of magnitude $r=21.1$ at a redshift $z=
Externí odkaz:
http://arxiv.org/abs/1405.5237
Autor:
Chakraborti, Sayan, Soderberg, Alicia, Chomiuk, Laura, Kamble, Atish, Yadav, Naveen, Ray, Alak, Hurley, Kevin, Margutti, Raffaella, Milisavljevic, Dan, Bietenholz, Michael, Brunthaler, Andreas, Pignata, Giuliano, Pian, Elena, Mazzali, Paolo, Fransson, Claes, Bartel, Norbert, Hamuy, Mario, Levesque, Emily, MacFadyen, Andrew, Dittmann, Jason, Krauss, Miriam, Briggs, M. S., Connaughton, V., Yamaoka, K., Takahashi, T., Ohno, M., Fukazawa, Y., Tashiro, M., Terada, Y., Murakami, T., Goldsten, J., Barthelmy, S., Gehrels, N., Cummings, J., Krimm, H., Palmer, D., Golenetskii, S., Aptekar, R., Frederiks, D., Svinkin, D., Cline, T., Mitrofanov, I. G., Golovin, D., Litvak, M. L., Sanin, A. B., Boynton, W., Fellows, C., Harshman, K., Enos, H., von Kienlin, A., Rau, A., Zhang, X., Savchenko, V.
Gamma Ray Bursts (GRBs) are characterized by ultra-relativistic outflows, while supernovae are generally characterized by non-relativistic ejecta. GRB afterglows decelerate rapidly usually within days, because their low-mass ejecta rapidly sweep up a
Externí odkaz:
http://arxiv.org/abs/1402.6336