Zobrazeno 1 - 10
of 305
pro vyhledávání: '"Bean, R. A."'
Autor:
Bortel, G., Tegze, M., Sikorski, M., Bean, R., Bielecki, J., Kim, C., Koliyadu, J., Koua, F., Ramilli, M., Round, A., Sato, T., Zabelskii, D., Faigel, G.
X-ray Free Electron Lasers (XFEL) are the most advanced pulsed x-ray sources. Their extraordinary pulse parameters promise unique applications. Indeed, several new methods have been developed at XFEL-s. However, no methods are known, which would allo
Externí odkaz:
http://arxiv.org/abs/2310.18203
Autor:
Chen, J.P.J., Pande, K., Donatelli, J.J., Martin, A.V., Ayyer, K., Chapman, H.N., Bean, R., Schmidt, K.E., Kirian, R.A.
Publikováno v:
In Ultramicroscopy July 2023 249
Autor:
Jain, B., Spergel, D., Bean, R., Connolly, A., Dell'antonio, I., Frieman, J., Gawiser, E., Gehrels, N., Gladney, L., Heitmann, K., Helou, G., Hirata, C., Ho, S., Ivezić, Ž., Jarvis, M., Kahn, S., Kalirai, J., Kim, A., Lupton, R., Mandelbaum, R., Marshall, P., Newman, J. A., Perlmutter, S., Postman, M., Rhodes, J., Strauss, M. A., Tyson, J. A., Walkowicz, L., Wood-Vasey, W. M.
The focus of this report is on the opportunities enabled by the combination of LSST, Euclid and WFIRST, the optical surveys that will be an essential part of the next decade's astronomy. The sum of these surveys has the potential to be significantly
Externí odkaz:
http://arxiv.org/abs/1501.07897
Publikováno v:
In Annals of Nuclear Energy 15 September 2020 145
Autor:
Johnson, R. D., Barone, P., Bombardi, A., Bean, R. J., Picozzi, S., Radaelli, P. G., Oh, Y. S., Cheong, S-W., Chapon, L. C.
Publikováno v:
R. D. Johnson et al., PRL 110, 217206 (2013)
Magnetic domains at the surface of a ferroelectric monodomain BiFeO3 single crystal have been imaged by hard X-ray magnetic scattering. Magnetic domains up to several hundred microns in size have been observed, corresponding to cycloidal modulations
Externí odkaz:
http://arxiv.org/abs/1303.6987
Autor:
Green, J., Schechter, P., Baltay, C., Bean, R., Bennett, D., Brown, R., Conselice, C., Donahue, M., Fan, X., Gaudi, B. S., Hirata, C., Kalirai, J., Lauer, T., Nichol, B., Padmanabhan, N., Perlmutter, S., Rauscher, B., Rhodes, J., Roellig, T., Stern, D., Sumi, T., Tanner, A., Wang, Y., Weinberg, D., Wright, E., Gehrels, N., Sambruna, R., Traub, W., Anderson, J., Cook, K., Garnavich, P., Hillenbrand, L., Ivezic, Z., Kerins, E., Lunine, J., McDonald, P., Penny, M., Phillips, M., Rieke, G., Riess, A., van der Marel, R., Barry, R. K., Cheng, E., Content, D., Cutri, R., Goullioud, R., Grady, K., Helou, G., Jackson, C., Kruk, J., Melton, M., Peddie, C., Rioux, N., Seiffert, M.
In December 2010, NASA created a Science Definition Team (SDT) for WFIRST, the Wide Field Infra-Red Survey Telescope, recommended by the Astro 2010 Decadal Survey as the highest priority for a large space mission. The SDT was chartered to work with t
Externí odkaz:
http://arxiv.org/abs/1208.4012
Autor:
Spergel, D. N., Bean, R., Doré, O., Nolta, M. R., Bennett, C. L., Dunkley, J., Hinshaw, G., Jarosik, N., Komatsu, E., Page, L., Peiris, H. V., Verde, L., Halpern, M., Hill, R. S., Kogut, A., Limon, M., Meyer, S. S., Odegard, N., Tucker, G. S., Weiland, J. L., Wollack, E., Wright, E. L.
Publikováno v:
Astrophys.J.Suppl.170:377,2007
A simple cosmological model with only six parameters (matter density, Omega_m h^2, baryon density, Omega_b h^2, Hubble Constant, H_0, amplitude of fluctuations, sigma_8, optical depth, tau, and a slope for the scalar perturbation spectrum, n_s) fits
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603449
Autor:
Jarosik, N., Barnes, C., Greason, M. R., Hill, R. S., Nolta, M. R., Odegard, N., Weiland, J. L., Bean, R., Bennett, C. L., Doré, O., Halpern, M., Hinshaw, G., Kogut, A., Komatsu, E., Limon, M., Meyer, S. S., Page, L., Spergel, D. N., Tucker, G. S., Wollack, E., Wright, E. L.
Publikováno v:
Astrophys.J.Suppl.170:263,2007
The WMAP satellite has completed 3 years of observations of the cosmic microwave background radiation. The 3-year data products include several sets of full sky maps of the Stokes I, Q and U parameters in 5 frequency bands, spanning 23 to 94 GHz, and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603452
Autor:
Hinshaw, G., Nolta, M. R., Bennett, C. L., Bean, R., Doré, O., Greason, M. R., Halpern, M., Hill, R. S., Jarosik, N., Kogut, A., Komatsu, E., Limon, M., Odegard, N., Meyer, S. S., Page, L., Peiris, H. V., Spergel, D. N., Tucker, G. S., Verde, L., Weiland, J. L., Wollack, E., Wright, E. L.
Publikováno v:
Astrophys.J.Suppl.170:288,2007
We present new full-sky temperature maps in five frequency bands from 23 to 94 GHz, based on the first three years of the WMAP sky survey. The new maps, which are consistent with the first-year maps and more sensitive, incorporate improvements in dat
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603451
Autor:
Page, L., Hinshaw, G., Komatsu, E., Nolta, M. R., Spergel, D. N., Bennett, C. L., Barnes, C., Bean, R., Doré, O., Dunkley, J., Halpern, M., Hill, R. S., Jarosik, N., Kogut, A., Limon, M., Meyer, S. S., Odegard, N., Peiris, H. V., Tucker, G. S., Verde, L., Weiland, J. L., Wollack, E., Wright, E. L.
Publikováno v:
Astrophys.J.Suppl.170:335,2007
The Wilkinson Microwave Anisotropy Probe WMAP has mapped the entire sky in five frequency bands between 23 and 94 GHz with polarization sensitive radiometers. We present three-year full-sky maps of the polarization and analyze them for foreground emi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603450