Search

29 Sep 2006: This raises thefollowing question: how sensitive is the behavior of the size op-timized beam model to the conversion scheme adopted?

14 Sep 2006: 1. Model-Based Hand Tracking Using a HierarchicalBayesian Filter. Björn Stenger , Arasanathan Thayananthan , Philip H. S. Torr ,and Roberto Cipolla. Abstract— This paper sets out a tracking framework,. which is applied to the recovery of

13 May 2006: Suppose given Ap SLn(Op) for all p S and let ε > 0. ... Suppose given Ap Matn(Op) with det(Ap) = δ for all p S and letε > 0.

19 Apr 2006: ApJ accepted, 7 November 2005Preprint typeset using LATEX style emulateapj v. 04/21/05. DUST IN RESONANT EXTRASOLAR KUIPER BELTS — GRAIN SIZE AND WAVELENGTH DEPENDENCEOF DISK STRUCTURE. M. C. Wyatt1. UK Astronomy Technology Centre, Royal

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

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

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.

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.

24 Nov 2006: op of the Cu layer. A 140 nm thick HfO2 was then deposited byputtering. ... Finally the. op electrodes were released by removing the unwanted seedayer, and then the a-Si sacrificial layer was etched using SF6lasma.

7 Feb 2006: OP , where O denotes the origin. (2) Let V be the open subset {0 < u < π, 0 < v < 2π}, and σ : V S2 be given by.