'Radio power' diaporamas de présentation

Research Profile of My Group

Research Profile of My Group. Guoliang Xing Department of Computer Science City University of Hong Kong. Facts of My Group. Members Three PhD students CityU, CityU-USTC, CityU-WuhanU One Master student Two research assistants (joint supervision) Part of CityU wireless group

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Spitzer Observations of 3C Quasars and Radio Galaxies:

Spitzer Observations of 3C Quasars and Radio Galaxies: Mid-Infrared Properties of Powerful Radio Sources. K. Cleary 1 , C.R. Lawrence 1 , J.A. Marshall 2 , L. Hao 2 , D. Meier 1. 1: JPL, California Institute of Technology 2: Cornell University. Summary. Why observe in infrared? Previous Work

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Advantages of TSMP

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Research Profile of My Group

Research Profile of My Group. Guoliang Xing Department of Computer Science City University of Hong Kong. Facts of My Group. Members Three PhD students CityU, CityU-USTC, CityU-WuhanU One Master student Two research assistants (joint supervision) Part of CityU wireless group

373 views • 23 slides

S kills : none

The physical layer. S kills : none C oncepts : wired hardware characteristics , wireless hardware characteristics (frequency and power), modulation schemes. This work is licensed under a Creative Commons Attribution-Noncommercial-Share Alike 3.0 License. Where does this topic fit?.

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On Dichotomies in Active Galaxies or The Jet-Accretion Connection

On Dichotomies in Active Galaxies or The Jet-Accretion Connection. Annalisa Celotti - S.I.S.S.A. [celotti@sissa.it]. Jets/outflows in accreting systems. Active Galactic Nuclei ~10% AGN 'radio-loud' extended / compact jets aligned up to 10 8 decades q < few degrees

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The luminosity-dependent evolution of the radio luminosity function

The luminosity-dependent evolution of the radio luminosity function. Emma Rigby University of Nottingham Collaborators: P. Best, M. Brookes, J. Dunlop, J. Peacock, L. Ker, H. Rottgering, J. Wall. Model of a radio-loud AGN (Urry & Padovani). Why study radio galaxy evolution?.

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Sensor Node Architectures

Sensor Node Architectures. EE202A Lecture Oct 1, 2003 Ram Kumar {ram@ee.ucla.edu}. Sensor Network Vision. Ack: Jason Hill, UC Berkeley. SENSING SUB-SYSTEM. PROCESSING SUB-SYSTEM. COMMUNICATION SUB-SYSTEM. ACTUATION SUB-SYSTEM. POWER MGMT. SUB-SYSTEM.

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Yetta

Reliable Clinical Monitoring using Wireless Sensor Networks: Experience in a Step-down Hospital Unit. Yetta. Outline. Introduction Monitoring system Clinical study Clinical deterioration detection Conclusion. Introduction. Clinical deterioration detection

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Constraining B in the ICM from Statistic s o f Giant Radio Halos

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Random Access MAC for Efficient Broadcast Support in Ad Hoc Networks

Random Access MAC for Efficient Broadcast Support in Ad Hoc Networks. Ken Tang, Mario Gerla Computer Science Department University of California, Los Angeles Los Angeles, CA 90095 http://www.cs.ucla.edu/NRL/wireless. Motivation.

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Radio Galaxy workshop: so what?

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Abstract

Complex Structures in the Jets of 3C371 and PKS 2201+044. R.M. Sambruna 1 , D. Donato 1 , F. Tavecchio 2 , L. Maraschi 2 , C.C. Cheung 3 , & C.M.Urry 4 1 NASA/GSFC, 2 OAB, 3 KIPAC/Stanford, 4 Yale. PKS 2201+044. 3C 371. Abstract

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