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Event Generator Physics 4 Bryan Webber Event Generator Physics ...
https://www.hep.phy.cam.ac.uk/theory/webber/MCnet/MClecture4.pdf19 Apr 2007: 11 -50.76 31.35 35.3 69.5 4.95 14 W+ 24 195 12 11 19 20 50.36 -31.10 -35.0 104.5 78.64. ... 23 9.40 65.65 13.2 67.8 4.95 26 W- -24 195 24 23 32 33 -9.37 -65.43 -13.1 106.4 82.28. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.pdf5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2) -
Unsupervised Language Model Adaptation for Mandarin…
mi.eng.cam.ac.uk/reports/svr-ftp/mrva_icslp06.pdf20 Jan 2007: Test set baseline N-gram adaptfixed weights dynamic weights. dev05bcm (BC) 25.6 24.5eval04 (BN) 14.7 14.8dev04f (BN) 6.4 6.5. ... P3 27.4 25.6 24.5 24.3 24.3. Table 3: P2, P3 stage dev05bcm CERs. -
Correlation Effectsin Super-Arrhenius Diffusion Vanessa de…
https://www-wales.ch.cam.ac.uk/Telluride/Souza.pdf19 Apr 2007: Changes in colour show disconnected branches – highly disconnected. Correlation Effects in Super-Arrhenius Diffusion – p.24/27. ... 220. 225. 230. Correlation Effects in Super-Arrhenius Diffusion – p.24/27. Diffusive Connections. -
arX iv:0 704. 0873 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf18 Apr 2007: hot Jupiter –0.08 to 0.39 1.7–5 [500–1600] 70–200 1 % 2 1 %cool Jupiter –0.44 to 0.40 0.24–1.7 [75–500] ... 200 8 % 9 (5–11) %. planet & debris –0.13 to 0.27 0.10–0.24 [30–75] 5–30 5 % 3 1 %debris –0.52 to 0.18 -
arX iv:0 704. 3369 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf26 Apr 2007: 24). In Figure 4 we compare models having5 MJ between the planets with and without disc matter lo-cated inside the inner planet. ... The mass distributionfollows equation (24) and the outer disc mass is varied bychanging parameter Σ0out. -
Space–time percolation Geoffrey R. Grimmett Abstract. The…
www.statslab.cam.ac.uk/~grg/papers/cperc.pdf22 Jun 2007: Theorem 2.4 and the preceding discussion). Seealso [24]. 6. The mean-field continuum model. ... 24] D. S. Fisher. Critical behavior of random transverse-field Ising spin chains. -
842 Publications of the Astronomical Society of the Pacific, ...
https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf18 Sep 2007: stellar luminosities. TheA stars (dark blue) are a sample of 46 detected at both 24 and 70mm (Wyattet al. ... A0, 3.6–24.8 pc for G0, and 1.8–8.6 pc for M0. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2) -
Microsoft PowerPoint - wyattpub
https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf24 Apr 2007: stars at 24,70,160μm• Akari (2006-) currently doing all-sky survey 2-180μm• Herschel (2008-) observations at 60-670μm• Spica (2017+) planned 5-200μm. ... Structure is wavelength dependent!850μm. (Holland et al. 2006)24 and 70μm. (Su et al.
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