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1 Jun 2006: 24 M. G. Worster and R. C. Kerr. with most metals, it has a low entropy of fusion and forms highly branched, rather than prism-like, crystals.

22 May 2006: Communications of theACM, 24(6):381–395, 1981. 15. [5] A. H. Gee, R. ... H. Berman. Engineering a freehand 3Dultrasound system. Pattern Recognition Letters, 24:757–777, 2003.

28 Nov 2006: 23,24]. Furthermore, electronic Raman scattering introdu-. ces an extra dependence of the lineshape with the excitation. ... 24] N.H. Nickel, P. Lengsfeld, I. Sieber, Phys. Rev., B 61 (2000) 15558.

6 Apr 2006: 24.27%) 5.66 neutralM 0.53 1.60 2.38(24.90%) 4.89 chargedM 0.30 1.63 2.40(25.10%) 1.57.

18 Nov 2006: 24 J.E. CREMONA, T.A. FISHER, C. O’NEIL, D. SIMON, AND M. ... 24, 235–265 (1997).The Magma home page is at http://magma.maths.usyd.edu.au/magma/. [8] D.

19 Mar 2006: 24] P. S. Penev. Dimensionality reduction by sparsification in a local-features representation of human faces. ... Ross and A. Jain. Information fusion in biometrics.PatternRecognition Letters, 24(13):2115–2125, 2003.

20 Feb 2006: 2419.5. 2324.5. 2208.94. 2206.19. 2108.67. 2097.96. 2042.24. 2038.81. 1984.96. 1819.94. 1815.18. ... 1211.24. 1176.47. 1147.32. 1080.84. 1012.11. 963.47. 771.78. 655.02. 509.12. 456.62. 456.58.

27 Nov 2006: The EPCs near K between bands [24] allow theaccurate determination of the intensity and shape of theRaman D peak. ... Jianget al., Chem. Phys. Lett. 392, 383 (2004). [24] For the branch near A01 at K, jg2Kk0q0;Kk0j2 hg2KiF1 cos'00.

19 Apr 2006: This latter study is based on weak IRAS excesses,and four of the six systems identified with IRAS at 25 µm do nothave 24-µm excesses on re-examination by Spitzer

5 May 2006: www.damtp.cam.ac.uk/lab/digiflow/ 2005.23 G. S. Campbell, Annu. Rev. Fluid Mech. 22, 57 1990.24 T.

13 May 2006: Remark 1.24. Generically, the splitting field of Φ has Galois group theaffine general linear group, AGL(2,n), which sits in an exact sequence. ... 24 J.E. CREMONA, T.A. FISHER, C. O’NEIL, D. SIMON, AND M.

27 Nov 2006: 154.5 Missing Energy. 174.6 Hadronic Tau Decays. 204.7 B tagging. 24. ... Analytic parameterizations of these distributions,shown as smooth curves in Figure 24, were used to construct log-likelihood functions.

2 Nov 2006: 0.5M2v2rel = M1Q? D whereas DD03 define S to be the specific bind-ing energy of the two objects (giving their equation 24). ... dNc(D > Dpb)/dt = 1000r13/3(dr/r)t2ageDcD. 3pb. M4/3? Q? D. 5/6e5/3, (24).

22 Oct 2006: 1/24. From this and Lemma 2.8 it follows that the number of appropriately directed 4-cycles.

12 Apr 2006: J. Symbolic Comput. 24, 235265 (1997). See alsohttp://magma.maths.usyd.edu.au/magma/. 9. C. O'Neil.

17 Feb 2006: 24]). Briefly, we estimate multivariate Gaussian components using the ExpectationMaximization (EM) algorithm [14], initialized by k-means clustering. ... appearance. IJCV, 14:5–24, 1995.34. S. Palanivel, B. S. Venkatesh, and B Yegnanarayana.

13 Nov 2006: Further information. FIG. 24. Color online a DispG and b FWHMG@244 asa function of the H content for amorphous carbons, includingGLCHH. ... Met. 139, 885 2003.24 S. Piscanec, M. Lazzeri, F. Mauri, A.

13 Nov 2006: Peng et al. [24] reported a root. mean square (rms) roughness of 0.11 nm in a-C:H deposited. ... Technol. 174–175 (2003) 1135. [24] X.L. Peng, Z.H. Barber, T.W. Clyne, Surf.

22 Nov 2006: obtained here compared to previous films produced by the. small ECWR [24] can be explained by the relatively high. ... 24] A.C. Ferrari, J. Robertson, M.G. Beghi, C.E. Bottani, R. Ferulano, R.

6 Dec 2006: Received 24 November 1999! The model and theoretical understanding of the Raman spectra in disordered and amorphous carbon aregiven. ... become localized.24 Olefinic CvCbonds are shorter than aromatic bonds, so they have hi.

6 Dec 2006: Thepresence of a RamanD peak at;1350 cm21 indicates thatthe s p2 phase is clustering into aromatic rings.18 There is arelationship23,24 between the in-plane correlation lengthL a ofthe ... 2.24 I (D)/I (G) is derived from the Raman spectra

28 Oct 2006: 1.7.13 Aide Memoire. 24. 2 Partial Differential Equations 25. 2.0 Why Study This? ... You should be able to do example sheets 1/2/3/4 after lectures 6/12/18/24 respectively.

7 Sep 2006: AP180(27), Eps15(6). Dynamin1,2,3 (89,30,24), Amph1(24). Eps15R(52), AP180(5), Dynamin1(1). Amph1(15), Eps15R(2). Amph2(40), Epsin1(1).

23 Jul 2006: Date: July 24, 2006. Speakers: Prof. Peter Harrison.

13 Nov 2006: Nominally sub-eutectic NW syn-thesis using Au as catalyst has been achieved for severalsemiconductor materials, including Ge [22], InP [23], andZnSe [24]. ... 5, 761 (2005)24 A. Colli, S. Hofmann, A.C. Ferrari, C. Ducati, F.

14 Dec 2006: The sp3 content of the films isestimated at 10% from X-ray photoemission and electron energy loss spectroscopy [19, 24]. ... P., Phys. Rev. B, 35 (1987) 2946. [24] Li Bassi A., Piseri P., Milani P., Ferrari A.

10 Apr 2006: 24.27%) 5.66 neutralM 0.53 1.60 2.38(24.90%) 4.89 chargedM 0.30 1.63 2.40(25.10%) 1.57.

19 Apr 2006: Crosses show the location of a planetesimal in the different resonances (2 : 1, 5 : 3, 3 : 2, and 4 : 3,from top to bottom) at intervals of 1/24 of the ... l1:24. e0:42. ; ð33Þ. D5 :3h i 13:2 þ 290:0=l1:33. ; ð34Þ.

19 Sep 2006: 3b. A simple way of measuring the silhouette coherence using theconcept of visual hull [24] is. ... pp. 245–262, 2001. [24] A. Laurentini, “The visual hull concept for silhouettebased image understanding,”IEEE Trans.

29 Apr 2006: average 92.0 64.1 58.3 17.0std 7.8 9.2 24.3 8.8. video sequences of the person in arbitrary motion (signif-icant translation, yaw and pitch, ... cluded and expression variant faces from a single sample per class.PAMI, 24(6), 2002.

6 Jun 2006: 79.9. 80.2. 80.4. Latitude. AUG SEP. 18 20 22 24 26. ... Longitude. NOV. 18 20 22 24 26. Longitude. DEC. SNOW DEPTHGR ratio: linear relation to snow depth.

23 Feb 2006: Gales et al.: THE CUED BROADCAST NEWS TRANSCRIPTION SYSTEM 7. developing the Cambridge 10RT broadcast news system in1998 [24]11. ... 0.16 0.18 0.2 0.22 0.24 0.2612. 14. 16. 18. 20. 22.

28 Sep 2006: 4.162 2.130 5.626 2.349 -0.529 -0.117 -0.293 0.074 0.105 24.4 2 8.5 283 3.57. ... 4.190 0.301 2.457 1.409 -0.147 0.092 -0.288 0.074 0.132 14.6 10 8.0 859 4.24.

13 Nov 2006: 2Cambridge University, Engineering Department, 9 JJ Thompson Avenue, Cambridge CB3 0FA, United KingdomReceived 29 August 2005; revised manuscript received 24 February 2006; published 25 April 2006. ... S. Dresselhaus, Phys. Rev. B 71,045417 2005. 24 P. B.

19 Apr 2006: 25 1.24 0.6 IRAS60 9.80 0.62 IRAS60 7.51 0.92 ISO80 8.86 0.87 ISO100 10.95 0.66 IRAS100 11.04 2.0 ISO120

3 Nov 2006: 18,97 0 6 050 (14) 0 8 052 (23) 0 5 068 (25) 0 1 058 (33) 2f0 6 029 (31) 0 3 033 (24)0 5 052 (29) 0 ... 24,97 0 3 081 (16) 0 10 050 (30) 1f26,97 0 4 075 (16) 0 9 050 (30) 0 5 079 (24) 0 6 042 (19) 1f.

8 Dec 2006: Our results differ considerably from those reported in [24]. c. e. ... 24] Pailard V., Melinon P., Perez J. P., Dupuis V., Perez A., Loubet J.

30 May 2006: J. Fluid Mech. (1996), 001. 308, p p. 289-311 Copyright @ 1996 Cambridge University Press. 289. Entrainment into two-dimensional and axisymmetric turbulent gravity currents. BY M A R K A. H A L L W O R T H ' , H E R B E R T E. H U P P E R T ' , J E

6 Apr 2006: Sparse Partition Regularity. Imre Leader† Paul A. Russell‡. June 3, 2005. Abstract. Our aim in this paper is to prove Deuber’s conjecture on sparse par-tition regularity, that for every m, p and c there exists a subset of thenatural numbers

13 Nov 2006: and E by laser induced acoustic waves and/or by surfaceBrillouin scattering.22–24 Visible and UV Raman measure-ments were performed using Renishaw Ramanspectrometers.1,25 Table I summarizes the ... 374 412GLCH 2 24 0.248 379ta-C:H 2.2 30 250 0.77

11 May 2006: n 16-48 64-96 112-145Elements along tendons 100 116 134Elements at equator 30 24 20Number of elements 3460 3216 3072Number of nodes 1831 1725 1671. ... Figures 24(a) and 24(b) show this type ofplot respectively for nCA118-10-290 and nCR118-10-290 balloons

24 Jul 2006: 480x360. 1.00 GB. WebM. 480x360. 484.29 MB. 480x360. 308.24 MB. 320x240.

17 Mar 2006: Part IID RIEMANN SURFACES (2005–2006): Revision Example Sheet. (a.g.kovalev@dpmms.cam.ac.uk). Note. The present 24-lecture course on Riemann Surfaces was first lectured in the academic

14 Sep 2006: Pattern Analysis andMachine Intelligence, 24(6):748–763, 2002. [22] S. Obdržálek and J. ... ACM Siggraph, 2004. [24] Carsten Rother, Sanjiv Kumar, Vladimir Kolmogorov,and Andrew Blake.

21 Sep 2006: Importantly, when aconservative point mutation (Y108F) that disrupts lectin activity ofCrt (24) was introduced into Crt-GFP [to generate Crt(Y108F)-. ... Biol. Cell 6,. 1173–1184. 24. Kapoor, M., Ellgaard, L., Gopalakrishnapai, J., Schirra, C., Gemma, E

19 Apr 2006: 32 0.02 0.13 0.04 < 0.5HD207129 0.60 0.03 0.15 0.02 0.31 0.04 < 0.24. ... However, sub-mm observations made withSCUBA on the JCMT indicate a diameter of 24 3 arc-sec (Holland et al.

19 Apr 2006: e5pr. [(a/a2)2.5e/(1 [ e2)1@2 [2.5ae/a2 ] O(e2) , (24). where AU2 yr1. ... P-R draga 6.24 ] 104(M/M. _)b. does not change the plane of the particleÏs orbit, I0pr.

20 Oct 2006: From Eq. 22 we have. U1 =E1/y0p1/y0. =1. 2y0, 24. as expected.For large y0 an accurate approximation to the solution.

19 Apr 2006: A&A 433, 1007–1012 (2005)DOI: 10.1051/0004-6361:20042073c ESO 2005. Astronomy&. Astrophysics. The insignificance of P-R drag in detectableextrasolar planetesimal belts. M. C. Wyatt. UK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9

14 Sep 2006: IEEE Trans. Pattern Analysis and Machine Intell., 24(4):509–522,April 2002. 5. M. ... Journal of Computer Vision, 48(1):9–19, June 2002. 24. J. Vermaak, A.