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27 Apr 2006: As a result of the crystalli- zation and different fluid dynamical processes op- erating in each of the described experiments, the concentration of the input fluid is considerably reduced before it

19 Apr 2006: "! $#&%(')! ,.-/%103246587797: 0<;=>&?%/3#60A@ B4%)CD0CEGFHI6KJ&0ML80ONPRQ8%S 4T0. UWVYXOZ [MV6]AXV_ba c&dfehgjiZ k.l<]m.XOV$c=nPo$Zpp.V6qUhal VC]rsZ qoftuvxw=y"z. {}|x|C) 9(A6Wf69O6AR.E&RAAA9E9 //.¡¢E£¤E(¥ª«¢¥ª<E4OP/GK=. |Y|&µEºA)»|&{f|

20 Nov 2006: indirect op-tical transitionssX point phonons in cubic BNd, "vd is theenergy of the direct band gap, and"vl the laser energy. ... III. The peak at 2940 cm1 slabeled overb. in Fig. 4d is asso-ciated with the overbending of the in-plane longitudinal

21 Nov 2006: In these situations, an op-timal hyperplane is found to minimise the probabilityof error, averaged over the training set.

14 Sep 2006: Now the problem of finding an op-timal replacement of pixels in patch p′ from those in patch m′ is equivalent to finding apath in the graph such that the error

12 Oct 2006: 20. 0 120 1. 2 h0 1 2 h0 1. – –––. – –. KO. PS. -2/K. OP. S-0. Time (h). 5′3′ 5′.

4 Dec 2006: op--o. --. rg. 1 A. M. Liu and M. L. Cohen, Science24, 841 1989!; Phys.

19 Apr 2006: 4.2. Modelingg the SED. The spectral energy distribution (SED) of Corvi from op-tical to submillimeter wavelengths is plotted in Figure 4.

19 Mar 2006: The optimal. values were found to be2.3 and6.2 for visual data; the op-timal filter for thermal data was found to be alow-passfilterwith W2 = 2.8 (i.e.

22 Nov 2006: Theseallow high-dimensional kernel feature-spaces to be de-fined and calculated using only simple transducer op-erations on discrete sequences (or lattices) of observa-tions.

23 Feb 2006: The model boundaryconditions were modified by using the BOUNDARY, OP=MOD option. ... Without changing the boundary conditions, T1 was increased to 20 N byusing the LOAD, OP=MOD command while keeping T2 constant at 5 N.

23 Feb 2006: HU }. Various levels of informationcan be propagated. 1. No information: The lower bound for allU utterances is op-timised.

19 Apr 2006: " $#%&%&' ()" #$%%'-,.0/(12&34657798:";" =<>? @$$A$>;"? BC? ";D= ;" EF46 "9/ GHJI"K"KMLBNPOQ R9SOETUQ VFW"OXTMY!Z[QS W"OXW"]BV. GTMY_OXVFW"O. (a Nb?K"K&c K"K"K"KdUe(K"K"K"K"K"K"K"K"K"K"K"K"K"K"KMe. fhgji kmlon_pqnsr turwv xzy|{|}ns{|r {|wi}_. 6sJ

23 Feb 2006: The op-erating point selected for this work was to use the 1 hour of Englishdata from the TDT4 Mandarin source, along with 10 hours of datafrom the TDT4 English data.

21 Sep 2006: Figure 11 illustrates the op-eration of the classifiers at different levels of the tree.

12 Dec 2006: et-ne. ac-op-de-n Si. alan-. ressn-at aen-. Si,. ases. the. sus. an-.

16 Nov 2006: 1. THE SIXTH SIR DAVID WILLIAMS LECTURE. THE RULE OF LAW. It is an immense honour and privilege to give the Sixth Sir David. Williams Lecture. It is also a formidable challenge, since Sir David’s. scholarly reputation is so high as to discourage

28 Sep 2006: arX. iv:a. stro. -ph/. 0603. 608. v2. 1 Se. p 20. 06. Mon. Not. R. Astron. Soc. 000, 1–26 (2006) Printed 4 September 2006 (MN LATEX style file v2.2). The UKIRT Infrared Deep Sky Survey Early Data Release. S. Dye1, S. J. Warren2, N. C. Hambly3, N.

19 Apr 2006: To probe the nature of the Vega disk further, wehave fitted it with models including realistic grain op-tical properties.

19 Apr 2006: 10 µm) to spiral inwards toward the star.Which of these two effects is dominant depends on the op-tical depth of the dust disk, but for all but the most