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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: 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

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.

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.

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.

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.

24 Jun 2007: Could generalise to F theory with ds2 = g(2,2) dx82. Dunajski (DAMTP, Cambridge) ASD in ( ) 27 March 2007 24 / 26.

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)

20 Jul 2007: 480x360. 1.24 GB. WebM. 480x360. 441.66 MB. MPEG-4 Video. 480x360. 331.96 MB.