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31 - 40 of 674 search results for KaKaoTalk:vb20 200 where 0 match all words and 674 match some words.
  1. Results that match 1 of 2 words

  2. Energy-Accuracy Trade-offs in Querying Sensor Data forContinuous…

    https://mobile-systems.cl.cam.ac.uk/papers/ubiworkshop10.pdf
    5 Jul 2010: 0. 10. 20. 30. 40. 50. 60. 70. 5 20 35 50 65 80 95 110 125 140 155 170 185 200 215. ... 80. 100. 120. 140. 160. 180. 200. 5 20 35 50 65 80 95 110 125 140 155 170 185 200 215.
  3. RCCAAcc10 R

    https://newn.cam.ac.uk/wp-content/uploads/2015/09/NCAccounts200910.pdf
    16 Nov 2010: 149Graduate Fee Income (per Capita Fee £2,190; 2008/9 £2,127) 291,200 246,874. ... Rents from College Subsidiaries 176,250 171,200. Total 3,222,163 2,883,692. 3. ENDOWMENT INCOMERestricted Unrestricted 2009/10 2008/09.
  4. L and N in the UK

    https://people.ast.cam.ac.uk/~vasily/oxford_homepage/ln.html
    13 Jul 2010: The amount of duty being evaded on these sales was well in excess of 200,000.
  5. arX iv:1 001. 5177 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/gw10.pdf
    29 Jan 2010: 200 mJy (Wyatt 2005) and the corresponding limit for ISOwas around 90 mJy (Decin et al.
  6. Are Debris Disks Self-Stirred?

    https://people.ast.cam.ac.uk/~wyatt/kw10.pdf
    19 Feb 2010: Our model shows a fairly slow decline untilafter 200–600 Myr, when stirring reaches the outer diskedge and the excess decreases more rapidly because massis being lost at all radii. ... Given that PRdrag is unlikely to be the cause, the further drop in
  7. 25 Nov 2010: C. Wyatt. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400of. fset. (Sa. turn. rad. ii). -100 -50 0 50 100offset (arcmin).
  8. arX iv:1 009. 0248 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf
    2 Sep 2010: 0.5. 1-50. 51-100. 101-150. 151-200. 201-250. 251-300. 301-350. 351-400. 401-450. 451-500.
  9. arX iv:1 004. 0644 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/sw10.pdf
    6 Apr 2010: arX. iv:1. 004. 0644. v1 [. astr. o-ph. EP. ] 5. Apr. 201. 0Astronomy & Astrophysicsmanuscript no. astars˙3rd c ESO 2010April 6, 2010. Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. Wyatt2. 1 Astrophysics Group,
  10. CARLSBERG MERIDIAN CATALOGUELA PALMA Number 13 CCD observations of ...

    https://research.ast.cam.ac.uk/cmt/cmc13_documentation.pdf
    29 Sep 2010: System: Automatic and remotely controlledDrift scans (generates 3 Gb of data per night)Data automatically parameterized (reduced to 6-7 Mb)Daily reductions take about 30 min.100,000–200,000
  11. https://research.ast.cam.ac.uk/cmt/data/camcext.04

    https://research.ast.cam.ac.uk/cmt/data/camcext.04
    29 Sep 2010: 040928 1 0.105 0.003 0.006 4 6.17 0.00 040929 1 0.200 0.008 0.017 5 6.43 0.00 040930 0 0.00

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