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  2. 200 years of science publishing now online at University of Cambridge …

    https://www.cam.ac.uk/news/200-years-of-science-publishing-now-online-at-university-of-cambridge
    8 Mar 2006: Search. Search. 200 years of science publishing now online at University of Cambridge. ... News. 200 years of science publishing now online at University of Cambridge..
  3. 200 years of science publishing now online at University of Cambridge …

    https://www.cam.ac.uk/research/news/200-years-of-science-publishing-now-online-at-university-of-cambridge
    8 Mar 2006: Search. Search. 200 years of science publishing now online at University of Cambridge. ... Research. 200 years of science publishing now online at University of Cambridge..
  4. hmm lab christmas party 031205 200

    https://www2.mrc-lmb.cam.ac.uk/groups/hmm/people/Christmas2005/Christmas2005-Pages/Image63.html
    12 Jun 2006:
  5. Education Minister visits Summer School | University of Cambridge

    https://www.cam.ac.uk/news/education-minister-visits-summer-school
    7 Sep 2006: Each March, a one-day event is held at Leeds United Football Club aimed at Year 12 students and their advisers, attracting more than 200 each time.
  6. Gonville & Caius expands for the 21st century | University of…

    https://www.cam.ac.uk/research/news/gonville-caius-expands-for-the-21st-century
    17 Oct 2006: 200 years later, at the intervention of alumnus John Caius, it was renovated and renamed Gonville & Caius with a new royal charter in 1557.
  7. 120 L fermentor: Quick guide

    https://www2.mrc-lmb.cam.ac.uk/groups/JYL/WWWfermentor/runfermentor.html
    27 Feb 2006: Press "Activate". Switch on stirrer to dissolve powder (Control: Ag(itation) speed=100-200 rpm). ... Stirrer 100-200, oxygen enrichment on (sp=0), air 60-100 (watch out for too much foam); NOTE: DO should be OFF.
  8. Archive: Chemical Informatics Letters

    https://www-jmg.ch.cam.ac.uk/CIL/archive/vol11.html
    27 Jul 2006: Technology Research News has 200 000 visitors a month, but needs to ask for donations.
  9. gphoto2-fuse-fs

    https://www.hep.phy.cam.ac.uk/~lester/gphoto2-fuse-fs/
    27 Feb 2006: At least, not very easily. In fact I could never get gtkam to work on my machine, and I couldn't understand how it worked, so instead I wrote a 200
  10. ATLAS SUSY Working Group: Rome Production

    https://www.hep.phy.cam.ac.uk/~lester/snaps/romeindex.html
    20 Jul 2006: 0, tan beta = 50, sgn(mu) = ). low mass point at limit of RunII reach (isasugra 7.71: m0=200 GeV, m12 = 160 GeV, A0 = -400 GeV, tan beta = 10, sgn(mu) = ).
  11. RomeSUSYWiki

    https://www.hep.phy.cam.ac.uk/~lester/snaps/RomeSUSYWiki.html
    20 Jul 2006: White. (9=) SU4 low mass point at limit of runII reach (isasugra 7.71: m0=200 geV, m12 = 160 geV, A0 = -400 geV, tan beta = 10, sgn(mu) = ). 100k Voss. (9=)
  12. Supplementary Figure 1 EPR spectra of R1-labeled endophilin A1 ...

    https://www2.mrc-lmb.cam.ac.uk/groups/hmm/publica/GallopEndophilinEMBO/EndoSupFigures.pdf
    8 Jun 2006: 150. 200. 247. Supplementary Figure 2. Sequence alignments and 3D models of C.
  13. PII: 0022-0248(93)90538-8

    www.itg.cam.ac.uk/people/heh/Paper116.pdf
    27 Apr 2006: The mean volume fraction 4,. 0 I I,,,, I0 100 200 300 400 500. ... whoseheight h ‘ H. Substituting. 0 0 100 200 300 500 M0 M= p0AH (A.4).
  14. 1 Jun 2006: 1. 0 100 200 300 400 Time (min). 0.6. 0.5 0. ... 38 M. G. Worster and R. C. Kerr. 300. 250. 200 n G 'g 150.
  15. IEEE TRANS. ON SAP, VOL. ?, NO. ??, ????? ...

    mi.eng.cam.ac.uk/~mjfg/liu_ASL07.pdf
    22 Nov 2006: IEEE TRANS. ON SAP, VOL? , NO? ,? 200? 1. Automatic Model Complexity Control Using. ... 200? 7. as the average phone correctness of all possible word sequences {W̃},.
  16. 5 May 2006: 0 20 40 60 80 100 120. 500400300200100. 0–100–200. 200300. 1000. ... 0 20 40 60 80 100 120. –100–200–300. Time (s)Time (s).
  17. 26 Apr 2006: The mushy layer starts to grow more slowlythan predicted by the theory after about 200 minutes. ... This is likely to be an indirectconsequence of the brine expulsion which begins at about 200 minutes, as shown infigure 6.
  18. PDF/36/aa3391-05.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/wyat05c.pdf
    19 Apr 2006: the range 110–200 AU with low eccentricitiesand inclinations (e < 0.01, I < 0.573). ... One problem is thatboth the 200 and 325 AU spirals have large azimuthal densityvariations which make them appear clumpy.
  19. M411_31c 568..571

    www.itg.cam.ac.uk/people/grae/47.pdf
    27 Apr 2006: that. a. b. µm0 100 200. Figure 1 The hydraulic system of polycrystalline ice. ... Separation (m). 2,000. 2,200. 2,400. 2,600. 2,800. 3,000. Dep. th (m. )
  20. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: higher surface brightness at r >200 AU compared to the r4 power law. ... but has slightlyhigher surface brightness at r > 200 AU compared to ther4 power law.
  21. PDF/48/aa5873-06.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf
    14 Dec 2006: 2004), we estimate for the firsttime the detection rate of cold debris disks around field M-dwarfs with ages between 20 and 200 Myr. ... al. 2005), the Castor moving group(200 Myr), the Ursa Maj moving group (500 100 Myr asrevised by King et al.
  22. 5 May 2006: pulses, 512 µs in duration and anacquisition width of 200 kHz was used. ... In our velocity imaging experiments the echo time TE was 10.3 ms, while theobservation time was 200 ms.
  23. Moment-free numerical approximation of highly oscillatory…

    www.damtp.cam.ac.uk/user/na/NA_papers/NA2006_09.pdf
    27 Nov 2006: The moments cannot be. 4. 50 100 150 200. 0.01. 0.02. ... 11 cos x e. iω(4x2x3). 50 100 150 200. 0.01. 0.02.
  24. PII: 0012-821X(90)90126-I

    www.itg.cam.ac.uk/people/grae/13.pdf
    27 Apr 2006: 0 0. c) loo. 50 100 150 200. TIME (yrs). 50 100 150 200. ... 100. 8O. 60. 40. 20. O " '. ". ' ". " ' -. 0 50 100 150 200. TIME (yrs) Fig.
  25. Axisymmetric particle-driven gravity currents

    www.itg.cam.ac.uk/people/heh/Paper127.pdf
    30 May 2006: 200. n 150 W. 50. 1 I I I I 0 20 40 60 80. ... R. Lister. 60 I n g'. (cm s-3 Expt Theory 42 21 11 0 - -. 0 - A. 0. I - - - 9 - - - --.__ I 100 I 150 I 200.
  26. NPGRJ_NSMB_1158 1..8

    https://www2.mrc-lmb.cam.ac.uk/groups/JYL/PDF/nsmbFtsK2006.pdf
    12 Oct 2006: c) Superdex 200 gel filtration of E. coli FtsKg in the presence of DNA. ... Storage buffer was. 20 mM Tris-HCl, 200 mM NaCl, 1 mM EDTA and 1 mM sodium azide.
  27. Particle-driven gravity currents

    www.itg.cam.ac.uk/people/heh/Paper115.pdf
    30 May 2006: initial volume fraction 5 YO of 200 pm-diameter sand and initial height of 20 m, for which us = 2 cm sP1 and gh = 0.81 m s -. The dynamics of ... 400. cl. 200. Y I I I L 0 50 100 150 200.
  28. 5 May 2006: Convection in reactive porous media 111. 100 200 300 400 500 600 700 8000. ... 50 100 150 200 250 3000. 0.5. 1.0. 1.5. 2.0. 2.5.
  29. flm483.dvi

    www.itg.cam.ac.uk/people/heh/Paper186.pdf
    5 Jan 2006: 3. 4. 5. 6. 100 200 300 400 500. a(cm). t (min). ... b). 1. 2. 3. 4. 5. 0 50 100 150 200 250 300.
  30. boomerang handout 2006

    www3.eng.cam.ac.uk/~hemh1/boomeranghandout2006.pdf
    14 Nov 2006: Dr Hugh Hunt Gyroscopes and Boomerangs www.hughhunt.co.uk. Normal boomerangs derive their shape from the bent bits of wood that are easy to find in outback. Australia, but their aerodynamic and gyrodynamic efficiency is poor and you need wide open
  31. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 Apr 2006: This 200-AU-sized regioncoincides with the slightly tilted inner disk identified optically withthe Hubble Space Telescope5. ... The possible relationship of these components has yetto be explored, but the lower inferred temperatures of the clumpparticles
  32. PII: 0012-821X(90)90126-I

    www.itg.cam.ac.uk/people/heh/Paper98.pdf
    27 Apr 2006: 0 0. c) loo. 50 100 150 200. TIME (yrs). 50 100 150 200. ... 100. 8O. 60. 40. 20. O " '. ". ' ". " ' -. 0 50 100 150 200. TIME (yrs) Fig.
  33. doi:10.1016/j.jbbm.2005.12.008

    https://www2.mrc-lmb.cam.ac.uk/groups/JYL/PDF/rfcloning2006%20published.pdf
    19 Apr 2006: Miroux personal communication), 200 AM dNTP’s (Roche), 1!reaction buffer,2.5 units PfuTurbok (Stratagene) in a total volume of 50 Al. ... TCF1 200 3–6 2.0 4.6 4/4 OK Yes nd. TCF2 200 3–6 2.0 4.6 4/4 OK Yes nd.
  34. Nonlinear double-diffusive convection

    www.itg.cam.ac.uk/people/heh/Paper25.pdf
    30 May 2006: J. F u i d Xech. (19761, VOZ. 78, part 4? pp. 821-854 Printed in Great Britain. 82 1. Nonlinear double-diffusive convection By H E R B E R T E. H U P P E R T A N D D A N I E L R. MOORE. Department of Applied Mathematics and Theoretical Physics,
  35. future of vibration research

    www3.eng.cam.ac.uk/~hemh1/talks/beamnodes.pps
    10 Dec 2006: 2. =. a. 121. 3. =. a. 200. 4. =. a.
  36. Submitted to ApJ 16 July 2006, Accepted 3 October ...

    https://people.ast.cam.ac.uk/~wyatt/wsgb07.pdf
    2 Nov 2006: belt width isdr = 0.5r; planetesimal strength is Q?D = 200 J kg. ... kg m3, e = 0.05, e/I = 1,Q?D = 200 J kg.
  37. https://www.hep.phy.cam.ac.uk/~lester/dtm662/SctApiLog.UCID:0.1.log

    https://www.hep.phy.cam.ac.uk/~lester/dtm662/SctApiLog.UCID:0.1.log
    6 Apr 2006: pid: 2191 at: Fri Mar 24 13:51:25 2006 pid: 2247 at: Fri Mar 24 13:53:41 2006 Initial setup complete InitialiseAll 1006 foe UCID:0.1 InitialiseModule 20220170100028 InitialiseModule 20220170100056 InitialiseRod SendPrimList (UCID:0.1 1)
  38. DYNAMIC RESOLUTION SELECTIONIN ULTRASONIC STRAIN IMAGING J. E.…

    mi.eng.cam.ac.uk/reports/svr-ftp/lindop_tr566.pdf
    29 Sep 2006: 8. 0 100 200 300 400 500 600. 0. 0.2. 0.4. ... ovar. ianc. e. window length = 50250500. (a). 0 100 200 300 400 5000.
  39. berloff.dvi

    www.damtp.cam.ac.uk/user/ngb23/publications/warwick.pdf
    7 Sep 2006: 0 100 200 300 400. 50. 100. 150. 200. 250. p1 p2. ... 100 200 300 400 500 600. 100. 200. 300. 400. 500.
  40. Ice blocks melting into a salinity gradient

    www.itg.cam.ac.uk/people/heh/Paper35.pdf
    30 May 2006: h. 5 200 - 9. ( b ) 400. 34 4 34 5 34 6 34 1 34 4 34 5 34 6 34 7 S ( % a ) S ( % O ). B I L t<h ... 100 0.0026 0.0061 0.0083 0.0184 150 0.0035 0.0077 0.0092 0.0198 200 0.0041 0.0088 00101 0.0210.
  41. 19 Jul 2006: Gaussianise the data for each speaker:. 20 15 10 5 0 5 10 15 200. ... 0.01. 0.02. 0.03. 0.04. 0.05. 0.06. 0.07. 0.08. 0.09. 0.1. 20 15 10 5 0 5 10 15 200.
  42. paper.dvi

    mi.eng.cam.ac.uk/~mjfg/liao_INTER06.pdf
    22 Nov 2006: 180 190 200 210 220 2300. 50. 100. Frame. aii. Figure 3: Plot of log energy for snippet from AURORA digit string8-6-Zero-1-1-6-2, showing joint ... Asanticipated, the extremes previously observed have disappeared. 180 190 200 210 220 230.
  43. flm145.dvi

    www.itg.cam.ac.uk/people/heh/Paper197.pdf
    11 Oct 2006: 1992). The typical grid has 200 intervals over [0, xN (t)] and a time step of0.04. ... 2 4 6 8 10 12 14 16 18 200.
  44. ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf
    19 Apr 2006: ac-count and 200 dust particles were produced with exactlythe same positions and velocities as the parent popula-tion. ... for the librationparameters to be fitted for each particle, and the meanparameters for each population of 200 dust grains to
  45. 1 Jun 2006: 4. 0. Tc W). - 4. 0 200 400 600 800. ... Part 2 347. Equilibrium. t (min). 200 400 600 800. t (min).
  46. 1 Jun 2006: I I I. I I I I 0 200 400 600 800. ... about half a year (hi = 200 cm and T / = 1016 "C).
  47. Paper1.dvi

    www.damtp.cam.ac.uk/user/na/NA_papers/NA2006_05.pdf
    20 Jun 2006: 6. 200. 0.5. 0.4. 0.3. 100. 0.2. 0.1. 800. 6040. 0.1. ... 200. 0 8060. 0.2. 40. 0.3. 100. 0.4. 200. 0.25. 0.2.
  48. SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…

    https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf
    19 Apr 2006: Accurate telescope pointing wascrucial to these observations and was checked before andafter each map using the nearby blazar 2255282 with rmserror of less than 200. ... Very littleinformation can be deduced about sizes or positions differ-ing by 200,
  49. PII: 0377-0273(82)90062-2

    www.itg.cam.ac.uk/people/heh/Paper48.pdf
    27 Apr 2006: 8 c ) and is graphed in Fig. 5. 200 -. 160 h(m). 120. 8 0 -. 4 0 -. 107. o ,6o 26o 36o r(m). ... t f o r d i s c u s s i o n ). 0 200 400 600 Metres I i I. SCALE. Fig. 9.
  50. 23 May 2006: Front spreading in experiments. 0. 100. 200. 300. 400. 500. 600.
  51. Full supersymmetry simulation for ATLAS in DC1

    https://www.hep.phy.cam.ac.uk/~lester/physics/CSC/DC1.pdf
    27 Nov 2006: The second algorithm,. 16. 0. 100. 200. 300. 400. 0 5 10 15 20Nkt jet. ... 10. 10 2. 10 3. 10 4. 0 200 400 600 800 1000.

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