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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

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.

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.

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.

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.

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.

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.

20 Apr 2007: 24. Definition 7.19. Suppose G is a group acting on a non-empty set X.

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

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)

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.

5 Dec 2007: Conditions in the outer flow, including the boundary conditions, can be chosen in a special way (Warn & Warn 1978, 56; (2.24) below) such that the changes induced in the outer ... 2.24) jl,n being the nth zero of the Bessel function J1.

8 Dec 2007: e. 0 40 60 80 100200.20. 0.22. 0.24. 0.26. 0.28. 0.30. ... EMBO J. 24,3658–3669 (2005). 18. Babst, M., Katzmann, D. J., Estepa-Sabal, E.

14 Apr 2007: S. Ayres,1 B. Baller,11 B. Barish,5 M. A. Barker,24 P. D. ... M. DeMuth,22 A. De Santo,24 M. Dierckxsens,4 M. V. Diwan,4. M.

24 Apr 2007: of conformations [23,24,25]. The success of this approach. relies on the ability of the conformational sampling to. ... states [24,26,27]. In a series of recent studies, NMR. chemical shift information has been used to restrain.