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Energy-Accuracy Trade-offs in Querying Sensor Data forContinuous…
https://mobile-systems.cl.cam.ac.uk/papers/ubiworkshop10.pdf5 Jul 2010: 0. 10. 20. 30. 40. 50. 60. 70. 5 20 35 50 65 80 95 110 125 140 155 170 185 200 215. ... 80. 100. 120. 140. 160. 180. 200. 5 20 35 50 65 80 95 110 125 140 155 170 185 200 215. -
RCCAAcc10 R
https://newn.cam.ac.uk/wp-content/uploads/2015/09/NCAccounts200910.pdf16 Nov 2010: 149Graduate Fee Income (per Capita Fee £2,190; 2008/9 £2,127) 291,200 246,874. ... Rents from College Subsidiaries 176,250 171,200. Total 3,222,163 2,883,692. 3. ENDOWMENT INCOMERestricted Unrestricted 2009/10 2008/09. -
L and N in the UK
https://people.ast.cam.ac.uk/~vasily/oxford_homepage/ln.html13 Jul 2010: The amount of duty being evaded on these sales was well in excess of 200,000. -
arX iv:1 001. 5177 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/gw10.pdf29 Jan 2010: 200 mJy (Wyatt 2005) and the corresponding limit for ISOwas around 90 mJy (Decin et al. -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: Our model shows a fairly slow decline untilafter 200–600 Myr, when stirring reaches the outer diskedge and the excess decreases more rapidly because massis being lost at all radii. ... Given that PRdrag is unlikely to be the cause, the further drop in -
Collisional Evolution of Irregular Satellite Swarms: Detectable Dust…
https://people.ast.cam.ac.uk/~wyatt/kw11.pdf25 Nov 2010: C. Wyatt. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400of. fset. (Sa. turn. rad. ii). -100 -50 0 50 100offset (arcmin). -
arX iv:1 009. 0248 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf2 Sep 2010: 0.5. 1-50. 51-100. 101-150. 151-200. 201-250. 251-300. 301-350. 351-400. 401-450. 451-500. -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: arX. iv:1. 004. 0644. v1 [. astr. o-ph. EP. ] 5. Apr. 201. 0Astronomy & Astrophysicsmanuscript no. astars˙3rd c ESO 2010April 6, 2010. Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. Wyatt2. 1 Astrophysics Group, -
CARLSBERG MERIDIAN CATALOGUELA PALMA Number 13 CCD observations of ...
https://research.ast.cam.ac.uk/cmt/cmc13_documentation.pdf29 Sep 2010: System: Automatic and remotely controlledDrift scans (generates 3 Gb of data per night)Data automatically parameterized (reduced to 6-7 Mb)Daily reductions take about 30 min.100,000–200,000 -
https://research.ast.cam.ac.uk/cmt/data/camcext.04
https://research.ast.cam.ac.uk/cmt/data/camcext.0429 Sep 2010: 040928 1 0.105 0.003 0.006 4 6.17 0.00 040929 1 0.200 0.008 0.017 5 6.43 0.00 040930 0 0.00
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