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16 Nov 2007: 2.5 HLDA and LDA projection 24. 2.6 multiple HLDA projections 25.

5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 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.

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.

19 Apr 2007: 11 -50.76 31.35 35.3 69.5 4.95 14 W+ 24 195 12 11 19 20 50.36 -31.10 -35.0 104.5 78.64. ... 23 9.40 65.65 13.2 67.8 4.95 26 W- -24 195 24 23 32 33 -9.37 -65.43 -13.1 106.4 82.28.

16 Nov 2007: 3.1 State Space Models 24. 3.2 Bayesian Networks 25. 3.3 State Evolution Process 27. ... bank of triangular filters (eg. 24 channels). This smoothed power spectrum is compressed using.

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.

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

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.

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.

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.

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.

23 Apr 2007: It is also interesting to compare N-Best supervisionto the standard 1-Best supervision adaptation approaches suchas iterative MLLR [24]. ... Zθ(O, H)can be simply calculated using the forward algorithm withp̃(ot|θt),. Zθ(O, H) =. θ. P (θ|M). t.

22 Feb 2007: 20. 25. 30. Cambridge UniversityEngineering Department. ICASSP 2006 Tutorial 24. Recent Progress in LVCSR: An HTK Perspective cMark Gales & Phil Woodland, 2006. ... generate a lattice when recognising the adaptation data– accumulate statistics over the

5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)

22 Nov 2007: and apply the preceding two propositions with θ = Vk. 24.

24 Jan 2007: Share. Published. 24 Jan 2007. Search news. Sign up to receive our newsletter.

31 Aug 2007: John Michael Hammersley. JOHN MICHAEL HAMMERSLEY21 March 1920 — 2 May 2004. Elected FRS 1976. By Geoffrey Grimmett and Dominic Welsh. Centre for Mathematical Sciences, University of Cambridge, Cambridge CB3 0WBMerton College, Oxford OX1 4JD. John

18 Jan 2007: u) infx();u()_x=uc(x)x()2 A Z 0 I(u)dt:24.

28 Feb 2007: S. A., 96,3590-3594. [6] Dobson, C. M. (1999) Trends Biochem. Sci., 24, 329-332.[7] Minton, A. ... E. (1999)J. Mol. Biol., 286, 593-606. [24] Smith, A. V. & Hall, C.