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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

28 Sep 2006: The low sensitivityof most optical CCD detectors at 1 µm, coupled with therelatively bright sky-background curtailed interest from op-tical astronomers.