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16 May 2006: For example, the lexicographic order on [4](2) is12, 13, 14, 23, 24, 34.). ... on Q5: , 1, 2, 3, 4, 5, 12, 13, 14, 15, 23, 24, 25, 34, 35, 45, 123, 124,125, 134, 135, 145, 234, 235, 245, 345, 1234, 1235, 1245, 1345,

5 Jan 2006: The experimentswere generally left to run for 24 hours, but heat loss to the laboratory became asignificant factor after roughly 10 hours. ... dy. dτ= (1 θ). (1 y)(1 Λθ). (3.24). y(τ = 0) = 1, (3.25).

1 Jun 2006: n = 7. {τ0x. 20 x1x6 (1/λ2)τ2τ3τ4τ5x2x5. τ0x20 λx1x6 (1/λ3)τ2τ 23 τ 24 τ5x3x4. & ... Simis, Effective computation of symbolic powers by Jacobian matrices,. Comm. Algebra 24 (1996), no.

26 Apr 2006: salinity of the ice) is very small; k #1 0 24 [Gross et al., 1987].

26 Apr 2006: Leppäranta, pp. 24–104,Univ. of Helsinki Press, Helsinki, 1998. Wettlaufer, J. S., Heat flux at the ice-ocean interface, J. ... E. Huppert, The phase evolution ofyoung sea ice, Geophys. Res. Lett., 24, 1251–1254, 1997a.

13 Nov 2006: 26] (see footnote 24, for qK, 00 0) andRef. [24]. This differs from the model of Ref. ... Pfeiffer et al., Phys. Rev. B 71, 155409 (2005).[24] J. Maultzsch, S.

22 Nov 2006: The set of parameters,Θ(sm),. 1Using this form of auxiliary function yields the same update formulae asusing the extended Baum-Welch (EBW) algorithm [24], [25]. ... Wmpem =B2D. 2m B1Dm B0β. (c)m Dm. (23). where. B2 = Σ̂m (24).

10 Apr 2006: Becker,21 A. Belias,25 T. Bergfeld,27,b R. H. Bernstein,11. D. Bhattacharya,24 M. ... McDonald,24 A. McGowan,1,21 J. R. Meier,21 G. I. Merzon,19 M. D.

13 Nov 2006: of CdSeis only a function of the powder temperature and is independentof the Ar partial pressure [24]. ... 94 6005. [24] Merten U and Bell W E 1967 The Characterization ofHigh-Temperature Vapors (New York: Margrave) chapter 4.

1 Jun 2006: 1 -. f = 16-21 min. 24.5 25.0 25.5 26.0 26.5 27.0 27.5 28.0 28.5 29.0 T. ... 0 - 1 24.5 25.0 25.5 26.0 26.5 27.0 27.5 28.0 28.5 29.0 29.5 30.0 30.5.

30 May 2006: University of Cambridge, Silver Street, Cambridge CB3 9EW, UK. (Received 17 October 1994 and in revised form 24 May 1995). ... Each freezing experiment took on the order of 24 hours, after which the solid crystalline block was cut up into pieces and the

1 Jun 2006: Okuz. 24 FLU 251.

22 Nov 2006: Km(Oi, Oj ; λ(1)) (24)where Kl(Oi, Oj ; λ) is the dot-product of the log-likelihoodratios and Kc(Oi, Oj ; λ(1)), Km(Oi, Oj ; λ(1)), etc., ... than in the ML case. This is because the MMI base-line performs much better than the ML baseline

21 Dec 2006: In the ensemble ofstructures that we determined, 12 of the 24 mutations investigatedby Capaldi et al. ... The native helices I (red), II (green), III(magenta), and IV (yellow) include residues 12–24, 32– 45, 51–56, and 66 –79,respectively.

10 Apr 2006: gaps between Tungsten increase effective RMoliere)• Lateral segmentation: 1cm2 matched to RMoliere• Longitudinal segmentation: 40 layers (24 X0, 0.9λhad). • ... 24.27%) 5.66 neutralM 0.53 1.60 2.38(24.90%) 4.89 chargedM 0.30 1.63 2.40(25.10%) 1.57.

30 May 2006: 2.21). (2.22). (2.23). (2.24). where EN is the value of [ at r = rN(t). ... Substituting (2.23) and (2.24) into (2.21) and (2.22), we find that $ ( z ) , where z = c/&, satisfies.

19 Apr 2006: MIR.but more common around stars < 100 Myr. MIPS 24 um image of Vega disk. ... MIPS-24 MIPS-70. MIPS-160 JCMT-450CSO-350. HST. Do Stars with Inner Planets (< 5 AU) Also Have Kuiper Disks?

13 Nov 2006: C2H2 60 nm/s 0.002 cc/Package/24 H 20. CH4 4 nm/s 0.030 cc/Package/24 H 1.3. ... C2H4 25 nm/s 0.012 cc/Pckage/24 H 3.3. a BIF: Barrier Improvement Factor is the ratio of a non-coated bottle to a.

17 Jan 2006: treatment. Results were normalised againstthe amount of CD8 reaching the TGN after 24 minutes in control-treated cells, and were expressed the s.e.m. ... 9A).Compared with control cells, suppression of SNX1 led to a54.57.8% reduction in the amount of anti

30 May 2006: 24-2. 740 J. Y. Holyer and H. E. Huppert. model for energy dissipation. ... The wavelengths given by (6.3) and (6.4) are 6.1 cm on the lower interface and 24-1 cm on the upper interface.