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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)

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.

8 Dec 2007: Wymann, M. Zvelebil, M. Laffargue, Trends. Pharmacol. Sci. 24, 366 (2003).4. ... Chem. 276, 21544 (2001). 24. E. H. Walker, O. Perisic, C.

27 Jun 2007: First, notice that. (δdw, w) = ‖dw‖2, w C0 (Mint); (3.24)thus, δd is a non-negative operator. ... Let σp(P) stand for the principal symbolof P. Then (3.24) implies that for any such w and a fixed x. (

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.