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11 - 20 of 614 search results for KaKaoTalk:vb20 200 where 0 match all words and 614 match some words.

  1. Results that match 1 of 2 words

  2. 1 Evaluating Temporal Robustness ofMobile Networks Salvatore…

    https://mobile-systems.cl.cam.ac.uk/papers/tmc11.pdf
    31 Oct 2011: 0 50 100 150 200 250 300. t. 0.00. 0.05. 0.10. ... Group members do notselect any target; instead they just follow their groupleader according to the pursuit force [21] which is setto give a group span of 200 meters: this force actsas

  3. 39 WILDSENSING: Design and Deployment of a Sustainable SensorNetwork…

    https://mobile-systems.cl.cam.ac.uk/papers/tosn2011.pdf
    27 Apr 2011: 39. WILDSENSING: Design and Deployment of a Sustainable SensorNetwork for Wildlife Monitoring. VLADIMIR DYO, University of BedfordshireSTEPHEN A. ELLWOOD, DAVID W. MACDONALD, ANDREW MARKHAM, NIKITRIGONI, and RICKLEF WOHLERS, University of

  4. 978-1-4577-0351-5/11/$26.00 c©2011 IEEE Diversity Decay in…

    https://mobile-systems.cl.cam.ac.uk/papers/wowmom11wip.pdf
    3 May 2011: The default time it takes to perform adownload D is set to 200 seconds, equivalent to 5MB filestransferred at 200Kbit/s. ... This dataset includes journey traces collectedin the London Underground over one month containing twoseparate train lines at

  5. A Fixed Point in Coptic Chronology: The Solar Eclipse of 10 March, 601

    https://people.ast.cam.ac.uk/~gil/Coptic-Eclipse.pdf
    5 Aug 2011: 190-192]. Zu den Luxusspeisen und -getränken in griechischen Papyri [pp. 193-200].

  6. Astroparticle_15

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_15.pdf
    25 Mar 2011: R is now 200 microns. This is very large on a quantum scale, but small on the scale used to test gravity in experiments – close to current limit of 100

  7. https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt

    https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt
    3 Jun 2011: 200.76777495 3.7214707 25.29 24.61 23.14 23.00 19.97 4 140.21862225 30.4611002 23.07 23.08 22.58 20.84 19.00 5

  8. Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf
    5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.

  9. arX iv:1 104. 0007 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/ramb11.pdf
    5 Apr 2011: Here we assume thatQD = 200 J kg. 1. and that it does not vary withD. ... 0.4. 0.8 200 Myr. Semimajor Axis (AU). Ecc. entr. icity. Log(Water Mass Fraction).

  10. arX iv:1 107. 1239 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vwmb11.pdf
    16 Nov 2011: HAUL. HAUL. Star. Planet. -350 -300 -250 -200 -150 -100 -50. ... Shown is the eccentricity evolution over 104 years of evolution of a0 = 200 AU planets (orbelt particles; left panel) and a0 = 103 AU planets (or belt particles; right panel) orbiting a

  11. Noname manuscript No.(will be inserted by the editor) DEBRIS ...

    https://people.ast.cam.ac.uk/~wyatt/wcb11.pdf
    28 Mar 2011: Noname manuscript No.(will be inserted by the editor). DEBRIS DISK SIZE DISTRIBUTIONS: STEADY STATECOLLISIONAL EVOLUTION WITH P-R DRAG AND. OTHER LOSS PROCESSES. M. C. WYATT1, C. J. CLARKE1 and M. BOOTH1,2,31 Institute of Astronomy, University of

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