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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: 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

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.

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.

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

22 Aug 2007: 2a)7,8,23,24. 1MRC Laboratory of Molecular Biology, Hills Road, Cambridge CB2 0QH, UK. ... Nature Biotechnol. 24, 1270–1278(2006). 42. Smith, C. J., Grigorieff, N. & Pearse, B.