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arX iv:0 704. 0873 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf18 Apr 2007: 200. 7. Mon. Not. R. Astron. Soc. 000, 1–6 (2006) Printed 9 April 2007 (MN LATEX style file v2.2). ... Doppler systems arepredicted here to form from 5-200 Jupiter masses of gas inthe disk, enough to make gas giant planets. -
seminar.dvi
www.statslab.cam.ac.uk/~rrw1/talks/binpacking.pdf18 Jan 2007: PAIRS j;k FOR WHICH FFD HAS LINEAREXPECTED WASTE UNDER Ufj;kg0 100 200 300 400 500. ... 0. 50. 100. 150. 200. 250. k. j. FFD RESULTSTHEOREMIf j < k1=2 then the expected waste for FFD is O(1).THEOREMThere exist pairs j;k with j arbitrarily large -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.pdf5 Jun 2007: a factor of 200:1 based onthe well established space densities of the foreground L and T dwarfs. ... Observing efficiency % per tile - - 73.3 - 69.9Time for 8,200 sq deg = 5467 tiles of 1.5 sq degTotal Elapsed Hours - - 373 - 391. -
Pupils in Northern Ireland learn about life at Cambridge | University …
https://www.cam.ac.uk/news/pupils-in-northern-ireland-learn-about-life-at-cambridge19 Mar 2007: A total of 200 pupils from 34 schools as far afield as Belfast, Enniskillen and Newry will be spending the morning at Cookstown High School on Tuesday, March 20. -
journal.dvi
mi.eng.cam.ac.uk/~mjfg/kcs_csl.pdf4 Apr 2007: observationMPE trajectoryfMPEMPE trajectory. 50 100 150 200 250 3000.2. 0.1. 0. ... Dev. of pMPE trajectory. 50 100 150 200 250 300. 0.8. -
finitet4.dvi
www.damtp.cam.ac.uk/user/ngb23/publications/finitet4.pdf24 Aug 2007: 100 200 300 400 500 600. 500. 1000. 1500. 2000. 2500. ... T /Tλ. 0 200 400 600 8000. 100. 200. 300. 400. -
Proceedingsofthe E-MRS 2006 Symposium E: Scienceand Technologyof…
www-g.eng.cam.ac.uk/nms/publications/pdf/Ferrari_PE2007.pdf30 Mar 2007: Calleja 200. Electronic properties of InAs/GaAs nanowire superlattices. Y.M. Niquet 204. ... Calleja, E. 200. Canc-ado, L.G. 88. Cantoro, M. 1. Carbone, L. -
LETTERS Breakdown of the adiabaticBorn–Oppenheimer approximationin…
www-g.eng.cam.ac.uk/nms/publications/pdf/Pisana_NM2007.pdf2 Mar 2007: Acc. Chem. Res. 35, 193–200 (2002).7. Alfe, D., Gillan, M. J. & ... Nature 438,. 197–200 (2005).16. Zhang, Y., Tan, Y. W., Stormer, H. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf5 Jun 2007: The Y-J colour is ESSENTIAL since the so called ’rare’ L and T dwarfs outnumberthe quasars by a factor of 200:1 based on the well established space densities of ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467 -
No Job Name
www-g.eng.cam.ac.uk/nms/publications/pdf/Hofmann_NL2007.pdf16 Apr 2007: Tecnai F20,200 kV), and Raman spectroscopy (Renishaw 1000 Ramanspectrometer, 514, 633, and 785 nm excitation). ... The0.18 nm lattice spacing observed in Figure 3a can be assignedto (200) lattice planes in metallic Ni.
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