Search

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: 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.

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.

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.

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-.

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

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