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1 - 20 of 416 search results for KaKaoTalk:vb20 200 where 0 match all words and 416 match some words.

  1. Results that match 1 of 2 words

  2. GW Gray Medal for 2004

    blcs.eng.cam.ac.uk/wp-content/uploads/2013/05/newsletter_oct_2007.pdf
    16 May 2013: The approximately 200 attendees of the lecture came from a very diverse background, many of them.

  3. 195-234deansc

    https://jotter.educ.cam.ac.uk/volume4/195-234-deansc/195-234deansc.pdf
    2 Jul 2013: JoTTER Vol. 4 (2013)  Clare Deans, 2013. 200. All about balance?

  4. Exploiting Foursquare and Cellular Data to InferUser Activity in ...

    https://mobile-systems.cl.cam.ac.uk/papers/mdm2013.pdf
    20 Mar 2013: For instance if three place categories are observedin the area, namely Work, Food and Shops, with check-ins380, 200 and 120 respectively, then yi is set to be equalto Work.

  5. wifiparking.dvi

    https://mobile-systems.cl.cam.ac.uk/papers/mobicom2013.pdf
    23 Jul 2013: 200. 400. 600. 800. Time (s). Cur. rent. (m. A). Scan Start Scan End. ... ized. Spe. ed. 0 200 400 600 8000. 0.5. 1. Time (s).

  6. METIS: Exploring mobile phone sensing offloading for efficiently…

    https://mobile-systems.cl.cam.ac.uk/papers/percom2013.pdf
    24 Jan 2013: 80. 100. 120. 140. 160. 180. 200. 220. 240. 1 5 15 30. ... 60. 80. 100. 120. 140. 160. 180. 200. 220. 10 30 50 70 90.

  7. Cambridge STARS Homepage

    https://people.ast.cam.ac.uk/~stars/
    28 Feb 2013: In most circumstances, just 200 points are sufficient. Simultaneous solution of structure and composition.

  8. STARS draft version, October 28, 2012 2 Contents 1 ...

    https://people.ast.cam.ac.uk/~stars/doc/stars.pdf
    14 Mar 2013: Eachset of reaction rates comes as a block of 200 numbers in 20 rows and 10 columns, just like the charged particlereaction data.

  9. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt
    29 Mar 2013: For the record these are: 20121013 runs 200-205; 20121025 runs 130-139; 20121112 runs 155-168 = not exactly a massive haul!

  10. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt
    28 May 2013: For the record, previous (re)processed nights were for missing Chilean data 20121013 200-205 20121025 130-139 20121112 155-168 ] We also spotted since the beginning of P91 that ESO

  11. VIRCAM Pipeline: vircam_tfits

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/group__vircam__tfits.html
    10 Apr 2013: Returns:. The output vircam_tfits object list. Author:. Jim Lewis, CASU. Definition at line 200 of file vircam_tfits.c.

  12. VIRCAM Pipeline: vircam_matchxy.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__matchxy_8c-source.html
    10 Apr 2013: 00334 00335 cpl_msg_info(fctid,"Doing the matching for extension %d",j); 00336 (void)ps.cat1f), 00337 vircam_tfits_get_table(ps.cat2f),200.0, 00338 &(vircam_matchxy_config.xoff),

  13. VIRCAM Pipeline: vircam_tfits.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__tfits_8c-source.html
    10 Apr 2013: vircam_tfits.c. 00001 / $Id: vircam_tfits.c,v 1.13 2007/10/25 17:34:01 jim Exp $ 00002 00003 This file is part of the VIRCAM Pipeline 00004 Copyright (C) 2005 Cambridge Astronomy Survey Unit 00005 00006 This program is free software; you can

  14. VIRCAM Pipeline: vircam_utils.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__utils_8c-source.html
    10 Apr 2013: fitslist[i]); 01534 val = cpl_image_get_mean_window(im,100,100,200,200); 01535 if (val > lthr && val < hthr) 01536 fitslist[m++] = fitslist[i]; 01537 else 01538 if (ditch) 01539

  15. arX iv:1 311. 2947 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/bkwj13.pdf
    14 Nov 2013: ity. 0. 6. 12. 18. 24. 30. 36. 20 200. 30.0Blackbody radius (AU).

  16. MNRAS 433, 2334–2356 (2013) doi:10.1093/mnras/stt900Advance Access…

    https://people.ast.cam.ac.uk/~wyatt/kw13.pdf
    16 Jul 2013: 88692 HD 165439 1.2 200 A2 11 Myr? Age uncertain? (22)89046 HD 166191 45.9? ... Inany case, removal of the coolest few sources (those below 200 Ksay) would make little difference to our analysis.

  17. arX iv:1 311. 2977 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf
    14 Nov 2013: Observations at wavelengths> 200 µm are sensitive to dust that is large enough totrace the planetesimal distribution.

  18. mnr_15360

    https://people.ast.cam.ac.uk/~wyatt/mw09.pdf
    17 Apr 2013: At this radius, the time-scale for planet stir-ring is only 0.65 Myr, orders of magnitude less than the star’s age(200 Myr; Barrado y Navascues et al.

  19. Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf
    29 Oct 2013: 2010). Possible (< 3σ) detection of orbital motionη Tel-B 48 2 200 6 Neuhäuser et al.

  20. arX iv:1 310. 1395 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vewt13.pdf
    8 Oct 2013: 10. 20. 50. 100. 200. Rkpc. UHk. msL. UHRL u sed fo r flyby co m pu tatio n s.

  21. arX iv:1 302. 3615 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vmbw13.pdf
    12 Apr 2013: 100 AU. 200 AU. 500 AU. 1000 AU. Figure 6. The number of orbits taken by an isolated planet arounda star throughout its MS phase.

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