Zobrazeno 1 - 10
of 5 197
pro vyhledávání: '"Uchida, N"'
Autor:
Abarr, Q., Awaki, H., Baring, M. G., Bose, R., De Geronimo, G., Dowkontt, P., Errando, M., Guarino, V., Hattori, K., Hayashida, K., Imazato, F., Ishida, M., Iyer, N. K., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lisalda, L., Matake, H., Maeda, Y., Matsumoto, H., Mineta, T., Miyazawa, T., Mizuno, T., Okajima, T., Pearce, M., Rauch, B. F., Ryde, F., Shreves, C., Spooner, S., Stana, T. -A., Takahashi, H., Takeo, M., Tamagawa, T., Tamura, K., Tsunemi, H., Uchida, N., Uchida, Y., West, A. T., Wulf, E. A., Yamamoto, R.
XL-Calibur is a hard X-ray (15-80 keV) polarimetry mission operating from a stabilised balloon-borne platform in the stratosphere. It builds on heritage from the X-Calibur mission, which observed the accreting neutron star GX 301-2 from Antarctica, b
Externí odkaz:
http://arxiv.org/abs/2010.10608
Autor:
Abarr, Q., Baring, M., Beheshtipour, B., Beilicke, M., deGeronimo, G., Dowkontt, P., Errando, M., Guarino, V., Iyer, N., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lanzi, J., Li, S., Lisalda, L., Okajima, T., Pearce, M., Press, L., Rauch, B., Stuchlik, D., Takahashi, H., Tang, J., Uchida, N., West, A., Jenke, P., Krimm, H., Lien, A., Malacaria, C., Miller, J. M., Wilson-Hodge, C.
The accretion-powered X-ray pulsar GX 301-2 was observed with the balloon-borne X-Calibur hard X-ray polarimeter during late December 2018, with contiguous observations by the NICER X-ray telescope, the Swift X-ray Telescope and Burst Alert Telescope
Externí odkaz:
http://arxiv.org/abs/2001.03581
Autor:
Ripa, J., Galgóczi, G., Werner, N., Pál, A., Ohno, M., Mészáros, L., Mizuno, T., Tarcai, N., Torigoe, K., Uchida, N., Fukazawa, Y., Takahashi, H., Nakazawa, K., Hirade, N., Hirose, K., Hisadomi, S., Enoto, T., Odaka, H., Ichinohe, Y., Frei, Z., Kiss, L.
Publikováno v:
Astronomische Nachrichten, 340, 666 (2019)
This study presents a background estimation for the Cubesats Applied for MEasuring and LOcalising Transients (CAMELOT), which is a proposed fleet of nanosatellites for the all-sky monitoring and timing based localization of gamma-ray transients with
Externí odkaz:
http://arxiv.org/abs/1909.00339
Autor:
Chauvin, M., Florén, H. -G., Friis, M., Jackson, M., Kamae, T., Kataoka, J., Kawano, T., Kiss, M., Mikhalev, V., Mizuno, T., Ohashi, N., Stana, T., Tajima, H., Takahashi, H., Uchida, N., Pearce, M.
Publikováno v:
Nature Astronomy volume 2, pages 652-655 (2018)
Black-hole binary (BHB) systems comprise a stellar-mass black hole and a closely orbiting companion star. Matter is transferred from the companion to the black hole, forming an accretion disk, corona and jet structures. The resulting release of gravi
Externí odkaz:
http://arxiv.org/abs/1812.09907
Autor:
Chauvin, M., Florén, H. -G., Friis, M., Jackson, M., Kamae, T., Kataoka, J., Kawano, T., Kiss, M., Mikhalev, V., Mizuno, T., Tajima, H., Takahashi, H., Uchida, N., Pearce, M.
The linear polarisation fraction and angle of the hard X-ray emission from the Crab provide unique insight into high energy radiation mechanisms, complementing the usual imaging, timing and spectroscopic approaches. Results have recently been present
Externí odkaz:
http://arxiv.org/abs/1802.07775
Autor:
Abarr, Q., Beheshtipour, B., Beilicke, M., Bose, R., Braun, D., de Geronimo, G., Dowkontt, P., Errando, M., Gadson, T., Guarino, V., Heatwole, S., Hossen, M., Iyer, N., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lanzi, J., Li, S., Lisalda, L., Okajima, T., Pearce, M., Peterson, Z., Press, L., Rauch, B., Simburger, G., Stuchlik, D., Takahashi, H., Tang, J., Uchida, N., West, A.
Publikováno v:
In Astroparticle Physics October 2022 143
Autor:
Chauvin, M., Florén, H. -G., Friis, M., Jackson, M., Kamae, T., Kataoka, J., Kawano, T., Kiss, M., Mikhalev, V., Mizuno, T., Ohashi, N., Stana, T., Tajima, H., Takahashi, H., Uchida, N., Pearce, M.
Strong magnetic fields, synchrotron emission, and Compton scattering are omnipresent in compact celestial X-ray sources. Emissions in the X-ray energy band are consequently expected to be linearly polarized. X-ray polarimetry provides a unique diagno
Externí odkaz:
http://arxiv.org/abs/1706.09203
Autor:
Abarr, Q., Awaki, H., Baring, M.G., Bose, R., De Geronimo, G., Dowkontt, P., Errando, M., Guarino, V., Hattori, K., Hayashida, K., Imazato, F., Ishida, M., Iyer, N.K., Kislat, F., Kiss, M., Kitaguchi, T., Krawczynski, H., Lisalda, L., Matake, H., Maeda, Y., Matsumoto, H., Mineta, T., Miyazawa, T., Mizuno, T., Okajima, T., Pearce, M., Rauch, B.F., Ryde, F., Shreves, C., Spooner, S., Stana, T.-A., Takahashi, H., Takeo, M., Tamagawa, T., Tamura, K., Tsunemi, H., Uchida, N., Uchida, Y., West, A.T., Wulf, E.A., Yamamoto, R.
Publikováno v:
In Astroparticle Physics March 2021 126
Publikováno v:
In Tectonophysics 20 October 2019 769
The importance of the power law has been well realized in econophysics over the last decade. For instance, the distribution of the rate of stock price variation and of personal assets show the power law. While these results reveal the striking scale
Externí odkaz:
http://arxiv.org/abs/physics/0611130