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Showing 1 - 20 results of 26 for search '"photon energy"', query time: 0.32s Refine Results
  1. 1
    ... is approximately equal to the photon energy, a suppression in thermoelectric current and negativity in the heat...
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  2. 2
    ... illumination, is modeled computationally. The relaxation of the photon energy into the protein matrix is also...
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  3. 3
    by Stamatikos, M, Band, D L
    Published 2006
    ... prompt photon energy fit to the Band function, utilize an observed spectroscopic redshift, for isotropic...
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  4. 4
    ... of 100 EeV where their gyroradii exceed the size of our galaxy. More than 6 orders of magnitude in photon...
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  5. 5
    ... incident photon energy of 56.4 keV at beamline ID15B of the European Synchrotron Radiation Facility...
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  6. 6
    by S. Barwick, F. Halzen, P. B. Price
    Published 1995
    ... the GeV photon energy of satellite-borne telescopes, to wavelengths smaller than 10 −16 cm, have been...
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  7. 7
    ... continuous illumination, is modeled computationally. The relaxation of the photon energy into the protein...
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  8. 8
    ... photon energy spectrum, whose spectral fit parameters are characterized by the Band function...
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  9. 9
    ... spectroscopy in the photon-energy range of 390–2800 cm -1 . The complex adopts a C 2v -symmetry structure...
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  10. 10
    ... illumination, is modeled computationally. The relaxation of the photon energy into the protein matrix is also...
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  11. 11
    .... The intensity and photon energy, particularly of the red/infrared and yellow emission bands, vary significantly...
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  12. 12
    ... regime, when the photon energy is smaller than the energy spacing between the lowest electron states...
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  13. 13
    ... or the terahertz regime. Tuning the photon energy, Rabi-resonant states emerge and in turn resonant current peaks...
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  14. 14
    ... featuring a prompt photon energy fit to the Band function, utilize an observed spectroscopic redshift...
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  15. 15
    ... the energy difference between the lowest states of the quantum dot system is smaller than the photon energy...
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  16. 16
    .... The intensity and photon energy, particularly of the red/infrared and yellow emission bands, vary significantly...
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  17. 17
    ... illumination, is modeled computationally. The relaxation of the photon energy into the protein matrix is also...
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  18. 18
    by Stamatikos, M, Ackermann, M, Achterberg, A, Ahrens, J, Atlee, D W, Bahcall, J N, Bai, X, Baret, B, Bartelt, M, Bay, R, Barwick, S W, Beattie, K, Becka, T, Becker, K H, Becker, J K, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, D Z, Blaufuss, E, Boersma, D J, Bohm, C, Boser, S, Botner, O, Bouchta, A, Braun, J, Burgess, C, Burgess, T, Castermans, T, Chirkin, D, Clem, J, Conrad, J, Cooley, J, Cowen, D F, D'Agostino, M V, Davour, A, Day, C T, De Clercq, C, Desiati, P, De Young, T R, Dreyer, J, Duvoort, M R, Edwards, W R, Ehrlich, R, Ekstrom, P, Ellsworth, R W, Evenson, P A, Fazely, A R, Feser, T, Filimonov, K, Gaisser, T K, Gallagher, J, Ganugapati, R, Geenen, H, Gerhardt, L, Greene, M G, Grullon, S, Goldschmidt, A, Goodman, J, Gro, A, Gunasingha, R M, Hallgren, A, Halzen, F, Hanson, K, Hardtke, D, Hardtke, R, Harenberg, T, Hart, J E, Hauschildt, T, Hays, D, Heise, J, Helbing, K, Hellwig, M, Herquet, P, Hill, G C, Hodges, J, Hoffman, K D, Hoshina, K, Hubert, D, Hughey, B, Hulth, P O, Hultqvist, K, Hundertmark, S, Ishihara, A, Jacobsen, J, Japaridze, G S, Jones, A, Joseph, J M, Kampert, K H, Karle, A, Kawai, H, Kelley, J L, Kestel, M, Kitamura, N, Klein, S R, Klepser, S, Kohnen, G, Kolanoski, H, Köpke, L, Krasberg, M, Kühn, K, Kujawski, E, Landsman, H, Lang, R, Leich, H, Liubarsky, I, Lundberg, J, Madsen, J, Marciniewski, P, Mase, K, Matis, H S, McCauley, T, McParland, C P, Meli, A, Messarius, T, Mészáros, P, Minor, R H, Miocinovic, P, Miyamoto, H, Mokhtarani, A, Montaruli, T, Morey, A, Morse, R, Movit, S M, Munich, K, Nahnhauer, R, Nam, J W, Niessen, P, Nygren, D R, Ogelman, H, Olbrechts, P, Olivas, A, Patton, S, Peña-Garay, C, Perez de los Heros, C, Pieloth, D, Pohl, A C, Porrata, R, Pretz, J, Price, P B, Przybylski, G T, Rawlins, K, Razzaque, S, Refflinghaus, F, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Rizzo, A, Robbins, S, Rott, C, Rutledge, D, Sander, H G, Schlenstedt, S, Schneider, D, Schwarz, R, Seckel, D, Seo, S H, Silvestri, A, Smith, A J, Solarz, M, Song, C, Sopher, J E, Spiczak, G M, Spiering, C, Stanev, T, Steffen, P, Stezelberger, T, Stokstad, R G, Stoufer, M, Stoyanov, S, Sulanke, K H, Sullivan, G W, Sumner, T J, Taboada, I, Tarasova, O, Tepe, A, Thollander, L, Tilav, S, Toale, P A, Turcan, D, van Eijndhoven, N, Vandenbroucke, J, Voigt, B, Wagner, W, Walck, C, Waldmann, H, Walter, M, Wang, Y R, Wendt, C, Wiebusch, C, Wikström, G, Williams, D, Wischnewski, R, Wissing, H, Woschnagg, K, Xu, X W, Yoshida, S, Yodh, G, Kurtzweil, J, Clarke, M J
    Published 2005
    ... photon energy spectrum, whose spectral fit parameters are characterized by the Band function...
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  19. 19
    by Lott, B.
    Published 2011
    ... (LAT) at photon energies E>100 MeV reached (66+/-2) x 10^-6 ph cm^-2 s^-1. The 3-hr peak flux...
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    Conference Object
  20. 20
    by Lott, B.
    Published 2011
    ... (LAT) at photon energies E>100 MeV reached (66+/-2) x 10^-6 ph cm^-2 s^-1. The 3-hr peak flux...
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    Conference Object
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