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2MASS resources
https://people.ast.cam.ac.uk/~rgm/vista/airglow/20 Nov 1999: Last modified: Sat Nov 20 20:16:23 1999. -
WFC - Photometric Calibration
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/photom_old.html13 Dec 1999: RGO z'. 22.08. Oct 98. -. -. -. -0.52 R-I. -. 22.20. Dec 98. -. -. -. -0.39 R-I. -. 22.24. Feb 99. -. -. -. -
D:CURRENT_WORKEQUILIBRIUM_PATHSPAPER2.DVI
www-civ.eng.cam.ac.uk/dsl/publications/equilpath2.pdf16 Nov 1999: ϕ1+ 180 [o]. p. 180. [o]. L1. L2. Snap. Snap. 0 20 40 60. ... are shown flat for clarity. 20. 2 Antenna deployment. 21. 3 Simulation model. -
Night Sky Brightness at Cerro Pachon
https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/12 Jul 1999: 11-50 nL. Backround stars (V>20 interstellar scattering):. 13 nL. Galaxies:. 0.1 nL. ... U = 22.0 mag/arcsec2. B = 22.7. V = 21.8. R = 20.9. -
Address by the Vice-Chancellor, Professor Sir Alec Broers |…
https://www.cam.ac.uk/news/address-by-the-vice-chancellor-professor-sir-alec-broers1 Oct 1999: 20. Amongst the host of national and international awards received by members of the University I must mention the Fields Medals awarded to Richard Borcherds and Tim Gowers; the Nobel Prize -
DVIWindo paper_IUTAM.dvi
www-civ.eng.cam.ac.uk/dsl/publications/bistabletubes.pdf19 Oct 1999: a) Tension test. 0 0.01 0.02 0.030. 5. 10. 15. 20. ... m-1. ). x (mm-1). x (mm-1)y (mm-1). 0. 20. 40. 60. -
Sky Brightness Primer
https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/page2.html9 Jul 1999: 11-50 nL. Backround stars (V>20 interstellar scattering):. 13 nL. Galaxies:. 0.1 nL. -
Cerro Tololo Measurements
https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/tololo.html10 Jul 1999: U = 22.0 mag/arcsec2. B = 22.7. V = 21.8. R = 20.9. -
se289900215p
https://www2.mrc-lmb.cam.ac.uk/groups/hmm/research/strucrev.pdf6 Jul 1999: Crystallography; CHC proximal legdomain residues 1210 to 1516 (20). 2.6 CHC proximal leg, clathrin LC. ... 20. J. A. Ybe et al., Nature 399, 371 (1999).21. Single-letter abbreviations for the amino acid resi-. -
st7a11.qxd
https://www2.mrc-lmb.cam.ac.uk/groups/JYL/PDF/MukB%20Structure%201999.pdf10 Sep 1999: We have usedboth secondary structure [19] and coiled-coil predictionprograms [20] to define a domain (residues 1–227), whichdoes not contain residues with significant coiled-coil prob-ability, but includes all ... S1 S2.
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