Community articles — Posters

projecto geometria Acuerdate que para realizar la distancia entre los planos primero debes ver si estos estan es su forma cartesiana general de no ser asi copia y pega el siguiente link para que veas como se hace:Da click aqui

Attempt to define various metrics directly related to coverage per compute second; an improvement on which furthers the desired left shift in design verification. A part to the solution to find breaks early in a continuous integration system, qualifying the design prior to important milestones and iterating over recent bug fixes or changes to weed out related issues is proposed. Created with the Jacobs Landscape Poster LaTeX Template Version 1.0 (29/03/13)

a1poster Portrait Poster LaTeX Template Version 1.0 (22/06/13) The a0poster class was created by: Gerlinde Kettl and Matthias Weiser (tex@kettl.de) This template has been downloaded from: http://www.LaTeXTemplates.com License: CC BY-NC-SA 3.0 (http://creativecommons.org/licenses/by-nc-sa/3.0/)

SALÃO UFRGS 2015- POSTER

Poster presented at the 2016 Department of Computer Science Open Evening event at the University of Cape Town. Poster based on beamerposter package.

Using WebRTC we are trying to develop a prod- uct called 'Ping' used for audio, mult-video, file and screen sharing. Ping uses WebRTC for the source of data exchange and XMPP Server for signalling and transporting. Ping works on Browser to Browser connections instead of naive client server approach. Ping guarentees high scalability and upto 60% more efficiency than existin

this is for the poster used on the ICASSP conference

evaluacion de correlaciones para la determinacion del coeficiente de transferecia de calor en un solo tubo

Blazars are a type of Active Galactic Nucleus (AGN), characterized by the emission of a relativistic jet that points close to our line of sight. They are extremely powerful, variable emitters from radio to gamma-ray wavelengths. By cross-correlating light-curves from different energies, it is possible to determine the physical condition of the blazar emitting region, i.e. mechanism, morphology, distance from block hole to the actual emission, etc. In 2007, the 40m telescope at the Owens Valley Radio Observatory (OVRO) embarked on a new research campaign. In support of the Fermi Gamma-ray Space Telescope, the OVRO 40m telescope is monitoring more than 1800 blazars twice per week. In 2014, a new Ku-band spectropolarimeter receiver, KuPol, was installed on the 40m telescope with the aim of elucidating about potential spectral fluctuations that may arise during the flaring events. In this poster, we will present relevant information and preliminar results from KuPol and the actual status of its calibration, and also as well as the current state of the PSD analysis, where we are applying Fourier Transform to the signals.