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1 - 10 of 233 search results for KaKaoTalk:po03 op where 0 match all words and 233 match some words.

  1. Results that match 1 of 2 words

  2. BLCSnews_0704.PDF

    blcs.eng.cam.ac.uk/wp-content/uploads/2013/05/newsletter_jul_2004.pdf
    28 Feb 2014: Kelker and R. Hatz. op. cit. pp529-531.9. P. Vukusic Natural Photonics.

  3. Colclough challenges aid allocation WP

    https://ceid.educ.cam.ac.uk/researchprogrammes/recoup/publications/workingpapers/WP40_RECOUPchallengesAidallocation.pdf
    12 May 2014: 1. RECOUP Working Paper No. 40 Challenges for the Optimal Allocation of Educational Aid: Should MDG Priorities be More Prominent? Christopher Colclough, University of Cambridge, UK. March 2011. 2. Author’s acknowledgements. The author is grateful

  4. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture05.pdf
    13 Oct 2014: The full calculation of stellar opacities is a major endeavour. For this rea-son, the Opacity Project (op) was set-up in 1984 as an international collab-oration to calculate the ... Similar work conducted at the LawrenceLivermore National Laboratory, the

  5. Irwin06draft.dvi

    https://people.ast.cam.ac.uk/~wfcam/ukreview/Irwin06draft.pdf
    23 Jul 2014: Mon. Not. R. Astron. Soc. 000, 1–26 (2006) Printed 15 May 2013 (MN LATEX style file v2.2). Pipeline processing of wide-field near-infrared data fromWFCAM (draft - not for circulation). Mike Irwin1, Jim Lewis1, Marco Riello1, Simon Hodgkin1,.

  6. arX iv:1 312. 4531 v2 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf
    21 Jan 2014: However, this similarityrequires that both components are radially optically thickand op-tically thin in the viewing direction, or the opening anglesmust belarger. ... The length of this period is uncertain due to the possibilityof non-axisymmetry and an

  7. arX iv:1 408. 4116 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kw14.pdf
    22 Aug 2014: For all systems, photometry ranging from op-tical to sub-mm wavelengths is compiled from a wide vari-ety of sources, including all-sky surveys such as Hipparcos(Perryman & ESA 1997;

  8. Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw14.pdf
    2 Jul 2014: yielding the ratio of the total cross-sectional area on op-posing sides of the disc.

  9. Five steps in the evolution from protoplanetary to debrisdisk ...

    https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf
    17 Dec 2014: Thus the dividingline is usually placed at f 0.01, which is around thelevel at which the dust might be expected to become op-tically thin in the radial direction to

  10. Mitrokhin’s KGB archive opens to public | University of Cambridge

    https://www.cam.ac.uk/research/news/mitrokhins-kgb-archive-opens-to-public
    Thumbnail for Mitrokhin’s KGB archive opens to public | University of Cambridge 7 Jul 2014: maps and details of secret Russian arms caches in Western Europe and the USA; and files on Melita Norwood, ‘the spy who came in from the Co-op’.
    By: @cambridge_uni

  11. University of Cambridge Research magazine issue 23

    https://www.cam.ac.uk/system/files/issue_23_research_horizons.pdf
    3 Jun 2014: op. yrig. ht m. ater. ial i. n T. he N.
    By: University of Cambridge

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