Zobrazeno 1 - 10
of 6 405
pro vyhledávání: '"Nishiyama, K."'
Publikováno v:
Clinical Ophthalmology, Vol Volume 18, Pp 2147-2154 (2024)
Ai Kozaki,* Rishu Inoue,* Naoko Yaji,* Koichi Nishiyama,* Toshu Inoue* Olympia Eye Hospital, Tokyo, Japan*These authors contributed equally to this workCorrespondence: Ai Kozaki, Olympia Eye Hospital, 2-18-12 Jingumae, Shibuya
Externí odkaz:
https://doaj.org/article/ce6cff856d044cd9b9cf8a36cda1db83
Autor:
Stewart, S.M., Corlett, M.T., Gardner, G.E., Ura, A., Nishiyama, K., Shibuya, T., McGilchrist, P., Steel, C.C., Furuya, A.
Publikováno v:
In Meat Science August 2024 214
Autor:
Henze, M., Darnley, M. J., Williams, S. C., Kato, M., Hachisu, I., Anupama, G. C., Arai, A., Boyd, D., Burke, D., Chinetti, K., Ciardullo, R., Cook, L. M., Cook, M. J., Erdman, P., Gao, X., Harris, B., Hartmann, D. H., Hornoch, K., Horst, J. Chuck, Hounsell, R., Husar, D., Itagaki, K., Kabashima, F., Kafka, S., Kaur, A., Kiyota, S., Kojiguchi, N., Kucakova, H., Kuramoto, K., Maehara, H., Mantero, A., Masci, F. J., Matsumoto, K., Naito, H., Ness, J. -U., Nishiyama, K., Oksanen, A., Osborne, J. P., Page, K. L., Paunzen, E., Pavana, M., Pickard, R., Prieto-Arranz, J., Rodriguez-Gil, P., Sala, G., Sano, Y., Shafter, A. W., Sugiura, Y., Tan, H., Tordai, T., Vratil, J., Wagner, R. M., Watanabe, F., Williams, B. F., Bode, M. F., Bruno, A., Buchheim, B., Crawford, T., Goff, B., Hernanz, M., Igarashi, A. S., Jose, J., Motta, M., O'Brien, T. J., Oswalt, T., Poyner, G., Ribeiro, V. A. R. M., Sabo, R., Shara, M. M., Shears, J., Starkey, D., Starrfield, S., Woodward, C. E.
Since its discovery in 2008, the Andromeda galaxy nova M31N 2008-12a has been observed in eruption every single year. This unprecedented frequency indicates an extreme object, with a massive white dwarf and a high accretion rate, which is the most pr
Externí odkaz:
http://arxiv.org/abs/1803.00181
Autor:
Marciniak, A., Pilcher, F., Oszkiewicz, D., Santana-Ros, T., Urakawa, S., Fauvaud, S., Kankiewicz, P., Tychoniec, Ł., Fauvaud, M., Hirsch, R., Horbowicz, J., Kamiński, K., Konstanciak, I., Kosturkiewicz, E., Murawiecka, M., Nadolny, J., Nishiyama, K., Okumura, S., Polińska, M., Richard, F., Sakamoto, T., Sobkowiak, K., Stachowski, G., Trela, P.
Publikováno v:
Marciniak et al. 2015, PSS, 118, 256
Physical studies of asteroids depend on an availability of lightcurve data. Targets that are easy to observe and analyse naturally have more data available, so their synodic periods are confirmed from multiple sources. Also, thanks to availability of
Externí odkaz:
http://arxiv.org/abs/1711.02429
Autor:
Kadono, R., Imazato, J., Ishikawa, T., Nishiyama, K., Nagamine, K., Yamazaki, T., Bosshard, A., Döbeli, M., van Elmbt, L., Schaad, M., Truöl, P., Bay, A., Perroud, J. P., Deutsch, J., Tasiaux, B., Hagn, E.
Publikováno v:
Phys. Rev. Lett. 57, 1847 (1986)
A large $\mu^-$ polarization was achieved in muonic Bi atoms with the help of the strong hyperfine field in a polarized nuclear target. Using $^{209}$Bi nuclei polarized to ($59\pm9$)% in ferromagnetic BiMn, we observed a $\mu$-$e$ decay asymmetry of
Externí odkaz:
http://arxiv.org/abs/1610.08238
Autor:
Darnley, M. J., Henze, M., Bode, M. F., Hachisu, I., Hernanz, M., Hornoch, K., Hounsell, R., Kato, M., Ness, J. -U., Osborne, J. P., Page, K. L., Ribeiro, V. A. R. M., Rodriguez-Gil, P., Shafter, A. W., Shara, M. M., Steele, I. A., Williams, S. C., Arai, A., Arcavi, I., Barsukova, E. A., Boumis, P., Chen, T., Fabrika, S., Figueira, J., Gao, X., Gehrels, N., Godon, P., Goranskij, V. P., Harman, D. J., Hartmann, D. H., Hosseinzadeh, G., Horst, J. Chuck, Itagaki, K., Jose, J., Kabashima, F., Kaur, A., Kawai, N., Kennea, J. A., Kiyota, S., Kucakova, H., Lau, K. M., Maehara, H., Naito, H., Nakajima, K., Nishiyama, K., O'Brien, T. J., Quimby, R., Sala, G., Sano, Y., Sion, E. M., Valeev, A. F., Watanabe, F., Watanabe, M., Williams, B. F., Xu, Z.
The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption ten times, including yearly eruptions from 2008-2014. With a measured recurrence period of $P_\mathrm{rec}=351\pm13$ days (we believe the true value to be half of this) a
Externí odkaz:
http://arxiv.org/abs/1607.08082
Autor:
Thuillot, W., Bancelin, D., Ivantsov, A., Desmars, J., Assafin, M., Eggl, S., Hestroffer, D., Rocher, P., Carry, B., David, P., Abe, L., Andreev, M., Arlot, J. -E., Asami, A., Ayvasian, V., Baransky, A., Belcheva, M., Bendjoya, Ph., Bikmaev, I., Burkhonov, O. A., Camci, U., Carbognani, A., Colas, F., Devyatkin, A. V., Ehgamberdiev, Sh. A., Enikova, P., Eyer, L., Galeev, A., Gerlach, E., Godunova, V., Golubaev, A. V., Gorshanov, D. L., Gumerov, R., Hashimoto, N., Helvaci, M., Ibryamov, S., Inasaridze, R. Ya., Khamitov, I., Kostov, A., Kozhukhov, A. M., Kozyryev, Y., Krugly, Yu. N., Kryuchkovskiy, V., Kulichenko, N., Maigurova, N., Manilla-Robles, A., Martyusheva, A. A., Molotov, I. E., Nikolov, G., Nikolov, P., Nishiyama, K., Okumura, S., Palaversa, L., Parmonov, O., Peng, Q. Y., Petrova, S. N., Pinigin, G. I., Pomazan, A., Rivet, J. -P., Sakamoto, T., Sakhibullin, N., Sergeev, O., Sergeyev, A. V., Shulga, O. V., Suarez, O., Sybiryakova, Y., Takahashi, N., Tarady, V., Todd, M., Urakawa, S., Uysal, O., Vaduvescu, O., Vovk, V., Zhang, X. -L.
Astrometric observations performed by the Gaia Follow-Up Network for Solar System Objects (Gaia-FUN-SSO) play a key role in ensuring that moving objects first detected by ESA's Gaia mission remain recoverable after their discovery. An observation cam
Externí odkaz:
http://arxiv.org/abs/1510.00509
Publikováno v:
A&A 582, L8 (2015)
The Andromeda Galaxy recurrent nova M31N 2008-12a has been caught in eruption nine times. Six observed eruptions in the seven years from 2008 to 2014 suggested a duty cycle of ~1 year, which makes this the most rapidly recurring system known and the
Externí odkaz:
http://arxiv.org/abs/1508.06205
Publikováno v:
Phys. Rev. B 92, 075203 (2015)
The hyperfine structure of the interstitial muonium (Mu) in rutile (TiO$_2$, weakly $n$-type) has been identified by means of a muon spin rotation technique. The angle-resolved hyperfine parameters exhibit a tetragonal anisotropy within the $ab$ plan
Externí odkaz:
http://arxiv.org/abs/1508.00309
Publikováno v:
Phys. Rev. B 92, 075203 (2015)
The hyperfine structure of the interstitial muonium (Mu) center in rutile (TiO$_2$, weakly $n$-type) has been identified by means of muon spin rotation technique. The angle-resolved hyperfine parameter has a tetragonal anisotropy within the $ab$ plan
Externí odkaz:
http://arxiv.org/abs/1411.3469