Zobrazeno 1 - 10
of 5 361
pro vyhledávání: '"Chen, C W"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Chiou, J. W., Ray, Sekhar C., Peng, S. I., Chuang, C. H., Wang, B. Y., Tsai, H. M., Pao, C. W., Lin, H. -J., Shao, Y. C., Wang, Y. F., Chen, S. C., Pong, W. F., Yeh, Y. C., Chen, C. W., Chen, L. -C., Chen, K. -H., Tsai, M. -H., Kumar, A., Ganguly, A., Papakonstantinou, P., Yamane, H., Kosugi, N., Regier, T., Liu, L., Sham, T. K.
Publikováno v:
Journal of Physical Chemistry C, (2012), 116, 16251--16258
This study investigates the strong photoluminescence (PL) and X-ray excited optical luminescence observed in nitrogen-functionalized 2D graphene nanoflakes (GNFs:N), which arise from the significantly enhanced density of states in the region of {\pi}
Externí odkaz:
http://arxiv.org/abs/1208.0885
Autor:
Reed, M. D., Harms, S. L., Poindexter, S., Zhou, A. -Y., Eggen, J. R., Morris, M. A., Quint, A. C., McDaniel, S., Baran, A., Dolez, N., Kawaler, S. D., Kurtz, D. W., Moskalik, P., Riddle, R., Zola, S., Ostensen, R. H., Solheim, J. -E., Kepler, S. O., Costa, A. F. M., Provencal, J. L., Mullally, F., Winget, D. W., Vuckovic, M., Crowe, R., Terry, D., Avila, R., Berkey, B., Stewart, S., Bodnarik, J., Bolton, D., Binder, P. -M., Sekiguchi, K., Sullivan, D. J., Kim, S. -L., Chen, W. -P., Chen, C. -W., Lin, H. -C., Jian, X. -J., Wu, H., Gou, J. -P., Liu, Z., Leibowitz, E., Lipkin, Y., Akan, C., Cakirli, O., Janulis, R., Pretorius, R., Ogloza, W., Stachowski, G., Paparo, M., Szabo, R., Csubry, Z., Zsuffa, D., Silvotti, R., Marinoni, S., Bruni, I., Vauclair, G., Chevreton, M., Matthews, J. M., Cameron, C., Pablo, H.
KPD 1930+2752 is a short-period pulsating subdwarf B (sdB) star. It is also an ellipsoidal variable with a known binary period just over two hours. The companion is most likely a white dwarf and the total mass of the system is close to the Chandresak
Externí odkaz:
http://arxiv.org/abs/1011.0387
Autor:
Provencal, J. L., Montgomery, M. H., Kanaan, A., Shipman, H. L., Childers, D., Baran, A., Kepler, S. O., Reed, M., Zhou, A., Eggen, J., Watson, T. K., Winget, D. E., Thompson, S. E., Riaz, B., Nitta, A., Kleinman, S. J., Crowe, R., Slivkoff, J., Sherard, P., Purves, N., Binder, P., Knight, R., Kim, S. -L., Chen, Wen-Ping, Yang, M., Lin, H. C., Lin, C. C., Chen, C. W., Jiang, X. J., Sergeev, A. V., Mkrtichian, D., Janiashvili, E., Andreev, M., Janulis, R., Siwak, M., Zola, S., Koziel, D., Stachowski, G., Paparo, M., Bognar, Zs., Handler, G., Lorenz, D., Steininger, B., Beck, P., Nagel, T., Kusterer, D., Hoffman, A., Reiff, E., Kowalski, R., Vauclair, G., Charpinet, S., Chevreton, M., Solheim, J. E., Pakstiene, E., Fraga, L., Dalessio, J.
Publikováno v:
Astrophys.J.693:564-585,2009
We report on the analysis of 436.1 hrs of nearly continuous high-speed photometry on the pulsating DB white dwarf GD358 acquired with the Whole Earth Telescope (WET) during the 2006 international observing run, designated XCOV25. The Fourier transfor
Externí odkaz:
http://arxiv.org/abs/0811.0768
Autor:
Abbasi, R., Abu-Zayyad, T., Belov, K., Belz, J., Cao, Z., Dalton, M., Fedorova, Y., Huentemeyer, P., Jones, B. F., Jui, C. C. H., Loh, E. C., Manago, N., Martens, K., Matthews, J. N., Maestas, M., Smith, J., Sokolsky, P., Springer, R. W., Thomas, J., Thomas, S., Chen, P., Field, C., Hast, C., Iverson, R., Ng, J. S. T., Odian, A., Reil, K., Walz, D., Bergman, D. R., Thomson, G., Zech, A., Chang, F-Y., Chen, C-C., Chen, C-W., Huang, M. A., Hwang, W-Y. P., Lin, G-L.
Publikováno v:
Astropart.Phys.29:77-86,2008
Measurements are reported of the yield and spectrum of fluorescence, excited by a 28.5 GeV electron beam, in air at a range of pressures of interest to ultra-high energy cosmic ray detectors. The wavelength range was 300 - 420 nm. System calibration
Externí odkaz:
http://arxiv.org/abs/0708.3116
Autor:
Reed, M. D., O'Toole, S. J., Terndrup, D. M., Eggen, J. R., Zhou, A. -Y., An, D., Chen, C. -W., Chen, W. P., Lin, H. -C., Akan, C., Cakirli, O., Worters, H., Kilkenny, D., Siwak, M., Zola, S., Kim, Seung-Lee, Gelven, G. A., Harms, S. L., Wolf, G. W.
Publikováno v:
Astrophys.J.664:518-535,2007
We present follow-up observations of pulsating subdwarf B (sdB) stars as part of our efforts to resolve the pulsation spectra for use in asteroseismological analyses. This paper reports on multisite campaigns of the pulsating sdB stars PG 1618+563B a
Externí odkaz:
http://arxiv.org/abs/0704.1496
Autor:
Huang, K. Y., Urata, Y., Kuo, P. H., Ip, W. H., Ioka, K., Aoki, T., Chen, C. W., Chen, W. P., Isogai, M., Lin, H. C., Makishima, K., Mito, H., Miyata, T., Nakada, Y., Nishiura, S., Onda, K., Qiu, Y., Soyano, T., Tamagawa, T., Tarusawa, K., Tashiro, M., Yoshioka, T.
Publikováno v:
Astrophys.J.654:L25-L28,2006
Multi-wavelength B, V, R, I observations of the optical afterglow of GRB 050319 were performed by the 1.05-m telescope at Kiso Observatory and the 1.0-m telescope at Lulin Observatory from 1.31 hours to 9.92 hours after the burst. Our R band lightcur
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611323
Autor:
He, X. M.1, Chen, C. W.1, Zhu, F. C.1, Qiao, D. L.1, Chen, N. F.1, Song, C.1 lanniao812329218@163.com
Publikováno v:
Current Topics in Nutraceutical Research. 2022, Vol. 20 Issue 3, p470-477. 8p.
Autor:
Belz, J., Cao, Z., Huentemeyer, P., Jui, C. C. H., Martens, K., Matthews, J., Maestas, M., Smith, J., Sokolsky, P., Springer, R. W., Thomas, J., Thomas, S., Chen, P., Field, C., Hast, C., Iverson, R., Ng, J. S. T., Odian, A., Reil, K., Vincke, H., Walz, D., Goldammer, A., Guest, D., Thomson, G., Chang, F-Y., Chen, C-C., Chen, C-W., Huang, M. A., Hwang, W-Y. P., Lin, G-L.
Publikováno v:
Astropart.Phys.25:57-63,2006
Measurements are reported on the fluorescence of air as a function of depth in electromagnetic showers initiated by bunches of 28.5 GeV electrons. The light yield is compared with the expected and observed depth profiles of ionization in the showers.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510375