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  2. 30 May 2007: t=1. (γjm(t)/cjm γj (t)) (23). and. γjm(t) = P (qt = sjm|O1:T ; λ) (24). ... Thomas, U.S. Virgin Islands,December 2003. [24] A. Stolcke, E. Brill, and M.
  3. Unsupervised Language Model Adaptation for Mandarin…

    mi.eng.cam.ac.uk/reports/svr-ftp/mrva_icslp06.pdf
    20 Jan 2007: Test set baseline N-gram adaptfixed weights dynamic weights. dev05bcm (BC) 25.6 24.5eval04 (BN) 14.7 14.8dev04f (BN) 6.4 6.5. ... P3 27.4 25.6 24.5 24.3 24.3. Table 3: P2, P3 stage dev05bcm CERs.
  4. Correlation Effectsin Super-Arrhenius Diffusion Vanessa de…

    https://www-wales.ch.cam.ac.uk/Telluride/Souza.pdf
    19 Apr 2007: Changes in colour show disconnected branches – highly disconnected. Correlation Effects in Super-Arrhenius Diffusion – p.24/27. ... 220. 225. 230. Correlation Effects in Super-Arrhenius Diffusion – p.24/27. Diffusive Connections.
  5. arX iv:0 704. 0873 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf
    18 Apr 2007: hot Jupiter –0.08 to 0.39 1.7–5 [500–1600] 70–200 1 % 2 1 %cool Jupiter –0.44 to 0.40 0.24–1.7 [75–500] ... 200 8 % 9 (5–11) %. planet & debris –0.13 to 0.27 0.10–0.24 [30–75] 5–30 5 % 3 1 %debris –0.52 to 0.18
  6. Space–time percolation Geoffrey R. Grimmett Abstract. The…

    www.statslab.cam.ac.uk/~grg/papers/cperc.pdf
    22 Jun 2007: Theorem 2.4 and the preceding discussion). Seealso [24]. 6. The mean-field continuum model. ... 24] D. S. Fisher. Critical behavior of random transverse-field Ising spin chains.
  7. arX iv:0 704. 3369 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf
    26 Apr 2007: 24). In Figure 4 we compare models having5 MJ between the planets with and without disc matter lo-cated inside the inner planet. ... The mass distributionfollows equation (24) and the outer disc mass is varied bychanging parameter Σ0out.
  8. Groups and Geometry The Second Part of Algebra and ...

    https://www.dpmms.cam.ac.uk/~twk/Alg.pdf
    20 Apr 2007: 24. Definition 7.19. Suppose G is a group acting on a non-empty set X.
  9. Analysis I Course C5 T. W. Körner September 18, ...

    https://www.dpmms.cam.ac.uk/~twk/C5.pdf
    18 Sep 2007: 24. and (sin z)2 (cos z)2 = 1 for all z, w C.(iv) sin(z) = sin z, cos(z) = cos z for all z C.(v) sin and cos
  10. 842 Publications of the Astronomical Society of the Pacific, ...

    https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf
    18 Sep 2007: stellar luminosities. TheA stars (dark blue) are a sample of 46 detected at both 24 and 70mm (Wyattet al. ... A0, 3.6–24.8 pc for G0, and 1.8–8.6 pc for M0.
  11. 4 Apr 2007: The log prior may be expressed as. (24). where is the general form defined in (15). ... 24] M. J. F. Gales, “Acoustic factorization,” presented at the ASRU Conf.,2001.

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