Zobrazeno 1 - 10
of 530
pro vyhledávání: '"Ezoe Y"'
Autor:
Dunn, W., Berland, G., Roussos, E., Clark, G., Kollmann, P., Turner, D., Feldman, C., Stallard, T., Branduardi-Raymont, G., Woodfield, E. E., Rae, I. J., Ray, L. C., Carter, J. A., Lindsay, S. T., Yao, Z., Marshall, R., A., A. N. Jaynes, Ezoe, Y., Numazawa, M., Hospodarsky, G. B., Wu, X., Weigt, D. M., Jackman, C. M., Mori, K., Nénon, Q., Desai, R. T, Blum, L. W., Nordheim, T. A., Ness, J. U., Bodewits, D., Kimura, T., Li, W., Smith, H. T., Millas, D., Wibisono, A. D., Achilleos, N., Koutroumpa, D., McEntee, S. C., Collier, H., Bhardwaj, A., Martindale, A., Wolk, S. J., Badman, S. V., Kraft, R. P.
Jupiter's magnetosphere is considered to be the most powerful particle accelerator in the Solar System, accelerating electrons from eV to 70 MeV and ions to GeV energies. How electromagnetic processes drive energy and particle flows, producing and re
Externí odkaz:
http://arxiv.org/abs/2303.02161
Autor:
Simionescu, A., Nakashima, S., Yamaguchi, H., Matsushita, K., Mernier, F., Werner, N., Tamura, T., Nomoto, K., de Plaa, J., Leung, S. -C., Bamba, A., Bulbul, E., Eckart, M. E., Ezoe, Y., Fabian, A. C., Fukazawa, Y., Gu, L., Ichinohe, Y., Ishigaki, M. N., Kaastra, J. S., Kilbourne, C., Kitayama, T., Leutenegger, M., Loewenstein, M., Maeda, Y., Miller, E. D., Mushotzky, R. F., Noda, H., Pinto, C., Porter, F. S., Safi-Harb, S., Sato, K., Takahashi, T., Ueda, S., Zha, S.
High-resolution spectroscopy of the core of the Perseus Cluster of galaxies, using the $Hitomi$ satellite above 2 keV and the $XMM$-$Newton$ Reflection Grating Spectrometer at lower energies, provides reliable constraints on the abundances of O, Ne,
Externí odkaz:
http://arxiv.org/abs/1806.00932
Autor:
Ohashi, T., Ishisaki, Y., Ezoe, Y., Yamada, S., Yamaguchi, S., Miyazaki, N., Tawara, Y., Mitsuda, K., Yamasaki, N. Y., Takei, Y., Sakai, K., Nagayoshi, K., Yamamoto, R., Chiba, A., Hayashi, T.
DIOS (Diffuse Intergalactic Oxygen Surveyor) is a small satellite aiming for a launch around 2020 with JAXA's Epsilon rocket. Its main aim is a search for warm-hot intergalactic medium with high-resolution X-ray spectroscopy of redshifted emission li
Externí odkaz:
http://arxiv.org/abs/1503.08405
Autor:
Smith, R. K., Odaka, H., Audard, M., Brown, G. V., Eckart, M. E., Ezoe, Y., Foster, A., Galeazzi, M., Hamaguchi, K., Ishibashi, K., Ishikawa, K., Kaastra, J., Katsuda, S., Leutenegger, M., Miller, E., Mitsuishi, I., Nakajima, H., Ogawa, T., Paerels, F., Porter, F. S., Sakai, K., Sawada, M., Takei, Y., Tanaka, Y., Tsuboi, Y., Uchida, H., Ursino, E., Watanabe, S., Yamaguchi, H., Yamasaki, N.
This white paper addresses selected new (to X-ray astronomy) physics and data analysis issues that will impact ASTRO-H SWG observations as a result of its high-spectral-resolution X-ray microcalorimeter, the focussing hard X-ray optics and correspond
Externí odkaz:
http://arxiv.org/abs/1412.1172
Autor:
Yamada, Shin'ya, Ezoe, Y., Ishisaki, Y., Ohashi, T., Iijima, N., Mitsuda, K., Nagayoshi, K., Akamatsu, H., Morooka, T., Tanaka, K.
We have fabricated multilayer readout wiring Transition Edge Sensors (TES), which enable us to realize both large effective area and high-energy resolution for future X-ray astrophysical missions, such as DIOS. By sandwiching a SiO2 insulation layer
Externí odkaz:
http://arxiv.org/abs/1402.0285
Autor:
Branduardi-Raymont, G., Sciortino, S., Dennerl, K., Güdel, M., Holmstrom, M., Koutroumpa, D., Maggio, A., Micela, G., Pillitteri, I., Sanz-Forcada, J., Read, A., Bhardwaj, A., Ezoe, Y., Gladstone, R.
The high resolution non-dispersive spectroscopy and unprecedented sensitivity of Athena+ will revolutionize solar system observing: the origin of the ions producing Jupiter's X-ray aurorae via charge exchange will be conclusively established, as well
Externí odkaz:
http://arxiv.org/abs/1306.2332
Autor:
Herder, J. W. den, Piro, L., Ohashi, T., Kouveliotou, C., Hartmann, D. H., Kaastra, J. S., Amati, L., Andersen, M. I., Arnaud, M., Attéia, J-L., Bandler, S., Barbera, M., Barcons, X., Barthelmy, S., Basa, S., Basso, S., Boer, M., Branchini, E., Branduardi-Raymont, G., Borgani, S., Boyarsky, A., Brunetti, G., Budtz-Jorgensen, C., Burrows, D., Butler, N., Campana, S., Caroli, E., Ceballos, M., Christensen, F., Churazov, E., Comastri, A., Colasanti, L., Cole, R., Content, R., Corsi, A., Costantini, E., Conconi, P., Cusumano, G., de Plaa, J., De Rosa, A., Del Santo, M., Di Cosimo, S., De Pasquale, M., Doriese, R., Ettori, S., Evans, P., Ezoe, Y., Ferrari, L., Finger, H., Figueroa-Feliciano, T., Friedrich, P., Fujimoto, R., Furuzawa, A., Fynbo, J., Gatti, F., Galeazzi, M., Gehrels, N., Gendre, B., Ghirlanda, G., Ghisellini, G., Gilfanov, M., Giommi, P., Girardi, M., Grindlay, J., Cocchi, M., Godet, O., Guedel, M., Haardt, F., Hartog, R. den, Hepburn, I., Hermsen, W., Hjorth, J., Hoekstra, H., Holland, A., Hornstrup, A., van der Horst, A., Hoshino, A., Zand, J. in 't, Irwin, K., Ishisaki, Y., Jonker, P., Kitayama, T., Kawahara, H., Kawai, N., Kelley, R., Kilbourne, C., de Korte, P., Kusenko, A., Kuvvetli, I., Labanti, M., Macculi, C., Maiolino, R., Hesse, M. Mas, Matsushita, K., Mazzotta, P., McCammon, D., Méndez, M., Mignani, R., Mineo, T., Mitsuda, K., Mushotzky, R., Molendi, S., Moscardini, L., Natalucci, L., Nicastro, F., O'Brien, P., Osborne, J., Paerels, F., Page, M., Paltani, S., Pedersen, K., Perinati, E., Ponman, T., Pointecouteau, E., Predehl, P., Porter, S., Rasmussen, A., Rauw, G., Röttgering, H., Roncarelli, M., Rosati, P., Quadrini, E., Ruchayskiy, O., Salvaterra, R., Sasaki, S., Sato, K., Savaglio, S., Schaye, J., Sciortino, S., Shaposhnikov, M., Sharples, R., Shinozaki, K., Spiga, D., Sunyaev, R., Suto, Y., Takei, Y., Tanvir, N., Tashiro, M., Tamura, T., Tawara, Y., Troja, E., Tsujimoto, M., Tsuru, T., Ubertini, P., Ullom, J., Ursino, E., Verbunt, F., van de Voort, F., Viel, M., Wachter, S., Watson, D., Weisskopf, M., Werner, N., White, N., Willingale, R., Wijers, R., Yamasaki, N., Yoshikawa, K., Zane, S.
Publikováno v:
Exp Astron (2012) 34, 519
ORIGIN is a proposal for the M3 mission call of ESA aimed at the study of metal creation from the epoch of cosmic dawn. Using high-spectral resolution in the soft X-ray band, ORIGIN will be able to identify the physical conditions of all abundant ele
Externí odkaz:
http://arxiv.org/abs/1104.2048
Autor:
Maeda, Y., Uchiyama, Y., Bamba, A., Kosugi, H., Tsunemi, H., Helder, E. A., Vink, J., Kodaka, N., Terada, Y., Fukazawa, Y., Hiraga, J., Hughes, J. P., Kokubun, M., Kouzu, T., Matsumoto, H., Miyata, E., Nakamura, R., Okada, S., Someya, K., Tamagawa, T., Tamura, K., Totsuka, K., Tsuboi, Y., Ezoe, Y., Holt, S. S., Ishida, M., Kamae, T., Petre, R., Takahashi, T.
Suzaku X-ray observations of a young supernova remnant, Cassiopeia A, were carried out. K-shell transition lines from highly ionized ions of various elements were detected, including Chromium (Cr-Kalpha at 5.61 keV). The X-ray continuum spectra were
Externí odkaz:
http://arxiv.org/abs/0912.5020
Publikováno v:
Astrophys.J.704:1495-1505,2009
We report an observation of X-ray emission from the exciting region of Cepheus A with the Chandra/ACIS instrument. What had been an unresolved X-ray source comprising the putative power sources is now resolved into at least 3 point-like sources, each
Externí odkaz:
http://arxiv.org/abs/0909.0451
Autor:
Takahashi, T., Abe, K., Endo, M., Endo, Y., Ezoe, Y., Fukazawa, Y., Hamaya, M., Hirakuri, S., Hong, S., Horii, M., Inoue, H., Isobe, N., Itoh, T., Iyomoto, N., Kamae, T., Kasama, D., Kataoka, J., Kato, H., Kawaharada, M., Kawano, N., Kawashima, K., Kawasoe, S., Kishishita, T., Kitaguchi, T., Kobayashi, Y., Kokubun, M., Kotoku, J., Kouda, M., Kubota, A., Kuroda, Y., Madejski, G., Makishima, K., Masukawa, K., Matsumoto, Y., Mitani, T., Miyawaki, R., Mizuno, T., Mori, K., Mori, M., Murashima, M., Murakami, T., Nakazawa, K., Niko, H., Nomachi, M., Okada, Y., Ohno, M., Oonuki, K., Ota, N., Ozawa, H., Sato, G., Shinoda, S., Sugiho, M., Suzuki, M., Taguchi, K., Takahashi, H., Takahashi, I., Takeda, S., Tamura, K., Tamura, T., Tanaka, T., Tanihata, C., Tashiro, M., Terada, Y., Tominaga, S., Uchiyama, Y., Watanabe, S., Yamaoka, K., Yanagida, T., Yonetoku, D.
The Hard X-ray Detector (HXD) on board Suzaku covers a wide energy range from 10 keV to 600 keV by combination of silicon PIN diodes and GSO scintillators. The HXD is designed to achieve an extremely low in-orbit back ground based on a combination of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611232