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Hosp 91 877 2287777 Ext 2289 2378 2382Fax No 91 877 2286803 Mobile 9849050833. ibmcom Emina Torlak IBM Research etorlakusibmcom Shaon Barman UC Berkeley sbarmancsberkeleyedu Rastislav Bodik UC Berkeley bodikcsberkeleyedu ABSTRACT Software ships with known bugs because it is expensive to pinpoint and 64257x the bug exposed by a umassedu Department of Electrical and Computer Engineering Uni ersity of Massachusetts Amherst gongecsumassedu Abstract Since web orkloads are kno wn to ary dynamically with time in this paper we ar gue that dynamic resource allocation techniques are S t describ th appropriatio o thei experience an struggle b hegemoni whit women movements colonizatio ha bee use t characteriz everythin fro th mos eviden economi an politica hierarchie t th productio o a particula cultura dis cours abou wha i calle Sarat Chandra Kanth Indian Institute of Science Bangalore Physics Puja Roy Presidency University Kolkata Physics Vilasini Venkatesh Sri Venkateswara College University of Delhi Physics Himanshu Khanchandani Indian Institute of Technology Roorkee Phy 1 2 PREFACE There is an increasing awareness about organic agricultural practices in the world. But, Indian farmers yet to be realize about ill effect of modern agriculture. Hence alternative farmin L. ensing . A. nd . S. upernova survey with . H. ubble. Marc Postman, STScI. Future Directions in Galaxy Cluster Surveys, Paris, June 2014. Post-. doctoral fellow. Graduate . student. The CLASH Science Team:. . Statistics. : . 1.8 . Ms. ½. . sq. .deg. . @. 160 . ksec. 1761 . sources. Dec. ’06-June ’07. Catalog. : . Elvis . et. al., . 2009, ApJS 184, 158. Martin Elvis, Francesca . Civano. , . Aldcroft. Manjil P. Saikia. Department of Mathematical Sciences,. School of Science and Technology,. Tezpur University, India. The Man. and. The Machine. Manjil P. Saikia. 2. Manjil P. Saikia. 3. Chandra can observe X-rays from particles up to the last second before they fall into a black hole!!!. Survey: Radio Properties. Of X-Ray Selected AGN. Manuela Molina. INAF/IASF Milano. AGN9 – Ferrara, 24/27 May 2010. In collaboration with: M. Polletta, L. Chiappetti, L. Paioro (INAF/IASF-Mi), G.Trinchieri (OA Brera), F. Owen (NRAO) and Chandra/SWIRE Team. . Ian Evans. On behalf of the Chandra Source Catalog Project Team. Chandra Users’ Committee Meeting. October 23, 2014. Summary. Summary of Progress Since . Last CUC . Meeting and Future Plan. Completed algorithm development and implementation through source detection and evaluation (through “. Una Hwang (NASA/GSFC, JHU). &. J Martin Laming (NRL). Boston AAS 24 May 2011. Cas A First-light Chandra image (Hughes+ 2000). Red: Fe. , . Green: Si . Cassiopeia A. . Core-collapse SNR with the most prominent Fe ejecta emission. (17 Years of SN 1987A with Chandra). David Burrows and Kari A. Frank. FOE51 Corvallis June 6, 2017. Built on the work of. PSU Chandra observations:. David Burrows. Sangwook. Park. Judith . for the Neutrino . Program . at Fermilab. Chandra Bhat. Fermilab. Acknowledgements. W. . Pellico. , C. . Drennan. , K. Triplett, S. . Chaurize. , . K. . Seiya. , F. Garcia, B. Hendricks, . T. . . Sullivan and A. Waller. National Centre for Radio Astrophysics. Tata Institute of Fundamental Research. Poonam Chandra. What are Gamma Ray bursts (GRBs)?. Most energetic events in the universe. Long duration GRBs (t>2s) .