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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.

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.

23 Apr 2007: 25] and by Osborne and Nielsen [24] (see, forexample, [4] and the references therein for further studies). ... satisfying Q 1,S1 log ν. (2.24). 10 G. R. Grimmett, T.

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.

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

18 Jan 2007: 5. r/8 r/24 r/8Amount. 3. 3. 3. 1 1. 3 2. ... O(1); (n)FF (n)? O(1); (n)? COMPUTER PROOFCOMPUTING RESOURCES 128 Megabytes memory 33 MHz MIPS processor CPLEXTM linear programming software ' 24 hours for largest problems Limiting factor is memory

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.