PDF-xUJDxUJDxUJDUfBJELxDJxBJxBTxj ETx BT x10 0x 0 1x0 51x201x2 48x748x11 T
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xUJDxUJDxUJDUfBJELxDJxBJxBTxj ETx BT x10 0x 0 1x0 51x201x2 48x748x11 T: Transcript
x0000HBJP99BL2123224516517058012345678794855955x 37 A7B95B612353x 60 13C556x 60 x 60 99O9Ux 60 BEDLBONNx 60 x 60 IBO9BBR9WRx0003YHx0003SRSXODWLRQVx0003WKHUHx0003WRx0003YHx0003SRSXODWLRQVx0003W. Yoav Zibin (**). David Cunningham (*) . Igor Peshansky (**). Vijay Saraswat (*). (*) IBM TJ Watson Research Center. (**) Google Labs (ex IBMers). ECOOP2012. Avoid access to uninitialized fields. Well-studied problem in Java. Async. -Finish Parallelism. Jonathan K. Lee, Jens . Palsberg. Presented By- . Vasvi. . Kakkad. Outline. Introduction. Featherweight X10. May-Happen-in-Parallel Analysis. Type Inference. Context-insensitive Analysis. J. Komppula. &. JYFL . ion source . group. University of . Jyväskylä. Department . of . Physics. Finland. Motivation. Diagnostics challenging. Experimental plasma parameters. R. i. . =. . n. e. Prof Wladimir . Lyra. Live Oak, 1119-G. Office Hours: Mon 4pm-5pm. Class hours: Mon/Wed 5pm-6:15pm. Formation by Core Accretion. Inward of snowline. Accreting . rocky cores. (small). Outward of snowline. =* 1 PW2k!2XWiniXWjnj+(11)= 1 PW2k!2Xi;jWiWjhninji(12)= 1 PW2k!2Xi;jWiWj2ij(13)=2 PW2i:(14)Thesignal-to-noiseratioofthe`wrong'methodisthereforesnrW=h^SWi q var(^SW)(15)=S PGiWi q P S:x=u;y=v;z=1uv;0u1;0v1ur(u;v)=ui+vj+(1uv)kru=1;0;1]TJ/;༕ ;.9; ;Tf 1;.51; 0 ;Td [;;rv=0;1;1]TJ/;༕ ;.9; Kontron Embedded Modules GmbH Brunnwiesenstr. 16 D-94469 Deggendorf Phone: +49 (0) 991/37024-0 Fax: +49 (0) 991/31275document JAP0051.doc 000; last changed on 10.09.02 08:25 page 1 o 123rr4rnr5322n4463532nnnrn7nn nn5nrn8 93233235/332351-9nn025x10425x1040/23/23929 999/910Arrnnrnnn/5x00008Bnnnnnnnnnrnn nnn28n26C2/8nnn nnnnnnnnnn//92 C/nnnnnnnnnnnnnn8D489D89D89D19Dnnn8D8D8Dn8D89D8D8D ///0r01nnrrnnnrnnrrnnrnn nrnrnnrnnrnrrrnnrrrnrnrnnnrrnnr-rnrrnrrnnrnrrrnnr/rnrr0rnrrnrrrnnrrnnnnnnnrnnrrnrrnnrnrrrrnrrnnrrrnrnnnnnrrrnnrnnn1nnnnrrrnnnnnrnrnrnnnnnr2rrrnnrrnrnnnrrrnrnnnnrnnrn3nrnrrnrnn nrnrnrnrr r rnnrrnnnrrr/00nnrrn12rnr 23r/ 2nrrn4 2n5 rrn 2n64 2rr72899 2rn7nr9 rn65 83rrnrnr rr rnr \n\r\r\r + #\n \n \n\n\r\n$\n \n \n SRITISHMEDICALJOURNALVOLUME2852OCTOBER1982TABLEII-Normal,borderline,andabnormalvaluesintestsofcardiovascularautonomicfunctionNormalBorderlineAbnormalTestsreflectingparasympatheticfunctionHeart-rateres \n\r \r \n \r\r \n\n !"#$ %\n\r&\r '\r( \n\r\n\r\n)* In 1996 Meade, the world\'s largest astronomical telescope manufacturer, introduced the ETX, a low-cost and genuinely portable instrument capable of results close to the theoretical limits of optical performance. Since then several different models have been introduced, most of them controlled by on-board computers that automatically point the telescope at objects selected from a database of 12,000. Unfortunately not all these objects are visible when looking through the ETX! (They are included because they can be imaged with special equipment.) Mike Weasner is a world expert on the ETX range, and describes the best 100 objects to start with, and offers hints and tips about using and looking after the telescope to get the best possible results.
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