The Coordinated Radio and Infrared Survey for High-mass Star Formation. II. Source Catalog

The CORNISH project is the highest resolution radio continuum survey of the Galactic plane to date. It is the 5 GHz radio continuum part of a series of multi-wavelength surveys that focus on the northern GLIMPSE region (10° < l < 65°), observed by the Spitzer satellite in the mid-infrared. Observations with the Very Large Array in B and BnA configurations have yielded a 1.''5 resolution Stokes I map with a root mean square noise level better than 0.4 mJy beam 1. Here we describe the data-processing methods and data characteristics, and present a new, uniform catalog of compact radio emission. This includes an implementation of automatic deconvolution that provides much more reliable imaging than standard CLEANing. A rigorous investigation of the noise characteristics and reliability of source detection has been carried out. We show that the survey is optimized to detect emission on size scales up to 14'' and for unresolved sources the catalog is more than 90% complete at a flux density of 3.9 mJy. We have detected 3062 sources above a 7σ detection limit and present their ensemble properties. The catalog is highly reliable away from regions containing poorly sampled extended emission, which comprise less than 2% of the survey area. Imaging problems have been mitigated by down-weighting the shortest spacings and potential artifacts flagged via a rigorous manual inspection with reference to the Spitzer infrared data. We present images of the most common source types found: H II regions, planetary nebulae, and radio galaxies. The CORNISH data and catalog are available online at http://cornish.leeds.ac.uk.

Contribución al diseño de GNSS-SDR, un receptor GNSS de código abierto

[ANGLÈS] This project introduces GNSS-SDR, an open source Global Navigation Satellite System software-defined receiver. The lack of reconfigurability of current commercial-of-the-shelf receivers and the advent of new radionavigation signals and systems make software receivers an appealing approach to design new architectures and signal processing algorithms. With the aim of exploring the full potential of this forthcoming scenario with a plurality of new signal structures and frequency bands available for positioning, this paper describes the software architecture design and provides details about its implementation, targeting a multiband, multisystem GNSS receiver. The result is a testbed for GNSS signal processing that allows any kind of customization, including interchangeability of signal sources, signal processing algorithms, interoperability with other systems, output formats, and the offering of interfaces to all the intermediate signals, parameters and variables. The source code release under the GNU General Public License (GPL) secures practical usability, inspection, and continuous improvement by the research community, allowing the discussion based on tangible code and the analysis of results obtained with real signals. The source code is complemented by a development ecosystem, consisting of a website (http://gnss-sdr.org), as well as a revision control system, instructions for users and developers, and communication tools. The project shows in detail the design of the initial blocks of the Signal Processing Plane of the receiver: signal conditioner, the acquisition block and the receiver channel, the project also extends the functionality of the acquisition and tracking modules of the GNSS-SDR receiver to track the new Galileo E1 signals available. Each section provides a theoretical analysis, implementation details of each block and subsequent testing to confirm the calculations with both synthetically generated signals and with real signals from satellites in space.

Possible hot spots excited by the relativistic jets of Cygnus X-3

We present the results of a deep search for associated radio features in the vicinity of the microquasar Cygnus X-3. The motivation behind is to find out evidence for interaction between its relativistic jets and the surrounding interstellar medium, which could eventually allow us to perform calorimetry of the total energy released by this microquasar during its flaring lifetime. Remarkably, two radio sources with mJy emission level at centimeter wavelengths have been detected in excellent alignment with the position angle of the inner radio jets. We propose that these objects could be the hot spots where the relativitic outflow collides with the ambient gas in analogy with Fanaroff-Riley II radio galaxies. These candidate hot spots are within a few arc-minutes of Cygnus X-3 and, if physically related, the full linear extent of the jet would reach tens of parsecs. We discuss here the evidence currently available to support this hypothesis based on both archival data and our own observations.

Radio Imaging of the Very-High-Energy γ-Ray Emission Region in the Central Engine of a Radio Galaxy

The accretion of matter onto a massive black hole is believed to feed the relativistic plasma jets found in many active galactic nuclei (AGN). Although some AGN accelerate particles to energies exceeding 1012 electron volts and are bright sources of very-high-energy (VHE) γ-ray emission, it is not yet known where the VHE emission originates. Here we report on radio and VHE observations of the radio galaxy Messier 87, revealing a period of extremely strong VHE γ-ray flares accompanied by a strong increase of the radio flux from its nucleus. These results imply that charged particles are accelerated to very high energies in the immediate vicinity of the black hole.

Deep radio images of the HEGRA and Whipple TeV sources in the Cygnus OB2 region.

The modern generation of Cherenkov telescopes has revealed a new population of gamma-ray sources in the Galaxy. Some of them have been identified with previously known X-ray binary systems while other remain without clear counterparts a lower energies. Our initial goal here was reporting on extensive radio observations of the first extended and yet unidentified source, namely TeV J2032+4130. This object was originally detected by the HEGRA telescope in the direction of the Cygnus OB2 region and its nature has been a matter of debate during the latest years. The situation has become more complex with the Whipple and MILAGRO telescopes new TeV detections in the same field which could be consistent with the historic HEGRA source, although a different origin cannot be ruled out. Aims.We aim to pursue our radio exploration of the TeV J2032+4130 position that we initiated in a previous paper but taking now into account the latest results from new Whipple and MILAGRO TeV telescopes. The data presented here are an extended follow up of our previous work. Methods.Our investigation is mostly based on interferometric radio observations with the Giant Metre Wave Radio Telescope (GMRT) close to Pune (India) and the Very Large Array (VLA) in New Mexico (USA). We also conducted near infrared observations with the 3.5 m telescope and the OMEGA2000 camera at the Centro Astronómico Hispano Alemán (CAHA) in Almería (Spain). Results.We present deep radio maps centered on the TeV J2032+4130 position at different wavelengths. In particular, our 49 and 20 cm maps cover a field of view larger than half a degree that fully includes the Whipple position and the peak of MILAGRO emission. Our most important result here is a catalogue of 153 radio sources detected at 49 cm within the GMRT antennae primary beam with a full width half maximum (FWHM) of 43 arc-minute. Among them, peculiar sources inside the Whipple error ellipse are discussed in detail, including a likely double-double radio galaxy and a one-sided jet source of possible blazar nature. This last object adds another alternative counterpart possibility to be considered for both the HEGRA, Whipple and MILAGRO emission. Moreover, our multi-configuration VLA images reveal the non-thermal extended emission previously reported by us with improved angular resolution. Its non-thermal spectral index is also confirmed thanks to matching beam observations at the 20 and 6 cm wavelengths.

Cooperative Transmission and Radio Resources Management for Wireless Networks

Report for the scientific sojourn at the Multimedia Communications Laboratory, University of Texas at Dallas, USA, from September to December 2005. The cooperative transmission has been analyzed taking a broadcast relay channel which assumes a scenario with one source and multiple destinations. Moreover, in order to improve the performance in terms of mutual information, it has been considered that for each destination there is another nearby terminal (called relay) which will help to improve the performance of the destination. This scheme combines different types of channels considered in the information theory, such as the relay channel, broadcast channel and interference channel (if the relays transmit information intended only to its associated destination). In this work, the author has studied the optimal way to encode the signals for the different users, known as capacity region (i.e. related to radio resources management ), of the broadcast relay channel.

Software de monitorització de dades rebudes en un GPS

"Aquest document conté originàriament altre material i/o programari només consultable a la Biblioteca de Ciències i d'Enginyeries".

Análisis y diseño de filtros apilados basados en resonadores acústicos

Durant els últims anys la demanda de filtres pas banda de ràdio freqüència, de reduïdes dimensions, lleugers i d'elevades prestacions destinats a sistemes de comunicacions inalàmbriques s'ha incrementat de forma significativa. Aquests sistemes principalment són els sistemes de telefonia mòbil de tercera generació UMTS y el sistema de navegació GPS. Els filtres actuals, basats en ressonadors SAW (Surface Acoustic Wave), tenen unes dimensions reduïdes però estan limitats en freqüència (3 GHz) i la seva tecnologia no és compatible amb les tecnologies estàndards de circuits integrats. Per aquestes raons s'espera que els filtres basats en ressonadors BAW (Bulk Acoustic Wave) substitueixin als SAW. Els dos tenen dimensions similars, però els filtres BAW poden funcionar a freqüències superiors a 3 GHz, poden treballar amb nivells de potència majors, i és important destacar el fet que la seva tecnologia és compatible amb les tecnologies estàndards de circuits integrats. La investigació en l'àmbit dels filtres BAW s'ha centrat en millorar els processos tecnològics i la qualitat dels materials, però s'ha treballat poc en l'adaptació de les tècniques sistemàtiques de disseny de filtres a les particularitats d'aquesta tecnologia, per tant el principal objectiu d'aquest treball és presentar mètodes sistemàtics per al disseny de filtres BAW, centrant-se en l'estudi d’estructures apilades.

Relay-assisted transmission and radio resource management for wireless networks

The following paper presents an overview of the Ph.D Thesis1 presented in [1], which compiles all the research done during the period of time between 2004-2007. In that dissertation the relay-assisted transmission with half-duplex relays is analyzed from different points of view. This study is motivated by the necessity of finding innovative solutions to cope with the requirements of next generation wireless services, and with current radio technology. The use of relayed communications represents a change of paradigm of conventional communications, and requires the definition and evaluation of protocols to be applied to single or multiple-user relay communication. With the two fold goal of enhancing spectral efficiency and homogenize service in cellular communications, system design is investigated at physical (type of transmissions of the relay, decoding mode, ..) and upper layers (resource allocation, dynamic link control).

Real time GPS precise positioning of LEO satellites

Report for the scientific sojourn at the German Aerospace Center (DLR) , Germany, during June and July 2006. The main objective of the two months stay has been to apply the techniques of LEO (Low Earth Orbiters) satellites GPS navigation which DLR currently uses in real time navigation. These techniques comprise the use of a dynamical model which takes into account the precise earth gravity field and models to account for the effects which perturb the LEO’s motion (such as drag forces due to earth’s atmosphere, solar pressure, due to the solar radiation impacting on the spacecraft, luni-solar gravity, due to the perturbation of the gravity field for the sun and moon attraction, and tidal forces, due to the ocean and solid tides). A high parameterized software was produced in the first part of work, which has been used to asses which accuracy could be reached exploring different models and complexities. The objective was to study the accuracy vs complexity, taking into account that LEOs at different heights have different behaviors. In this frame, several LEOs have been selected in a wide range of altitudes, and several approaches with different complexity have been chosen. Complexity is a very important issue, because processors onboard spacecrafts have very limited computing and memory resources, so it is mandatory to keep the algorithms simple enough to let the satellite process it by itself.

Creación de una radio musical participativa con difusión online y FM

Este proyecto propone crear un sistema inteligente y autónomo de emisión conjunta por Internet y FM. A través de una interfaz Web cómoda y sencilla, el oyente podrá interactuar con la emisora e influir en la emisión, exponiendo sus preferencias. El sistema tomará de forma autónoma y dinámica las decisiones pertinentes que garantizarán que la emisión cumple las preferencias definidas.

Adaptación del CSS al marketing político

Resum El present treball és un estudi sobre l’adaptació de la coneguda tècnica de marketing dels Estudis de Satisfacció de Clients -Costumers Satisfaction Survey (CSS)- al marketing polític. En ell es desenvolupa el concepte estratègic de client així com la importància d’una bona gestió de la cartera de clients en l’empresa. Fent un compendi dels atributs més rellevants dels CSS, s’estableix un paral•lelisme entre empresa i administració per extrapolar-ne els CSS i obtenir els Estudis de Satisfacció Ciutadana –Citizen Survey Satisfaction (CzSS). Finalment, s’estudia la utilitat dels CzSS, i la seva aplicació al marketing polític, plantejant-ne un cas pràctic amb el disseny d’una enginyeria de CzSS pel Perú.

Comparativa de la publicitat radiofònica entre Espanya i Itàlia. Estudi de les emissores Els 40 Principals y Radio Deejay

El treball final de carrera “Comparativa de la publicitat radiofònica entre Espanya i Itàlia. Estudi de les emissores Els 40 Principals i Radio Deejay”, és un anàlisi que pretén, mitjançant un estudi de cas de dues emissores de radiofórmula privades i nacionals, una espanyola i una italiana, comparar la publicitat radiofònica entre Espanya i Itàlia en cadenes musicals. L’estudi analitza la història, el target, la programació, la publicitat i les tarifes en cada una de les dues emissores per tal de trobar les semblances i diferències entre elles. La recerca es centra amb l’anàlisi dels tipus d’anunciants, l’estructura dels espais i formats publicitaris i l’anàlisi de la publicitat emesa en cada emissora en la franja horària del matí. Se n’extreuen conclusions que utilitzem com a referència per veure si a Espanya i a Itàlia aquest tipus d’emissores de ràdio usen les mateixes estratègies organitzatives i creatives, veure si en el passat i el present han seguit i segueixen un mateix camí o no.

Experimentació amb un receptor software GPS-Galileo d'alta sensibilitat per a entorns interiors

Este proyecto se centra en el análisis de señales GPS, utilizando un receptor software desarrollado con Matlab en un proyecto de investigación para la Agencia Espacial Europea (ESA), llevado a cabo por parte del departamento de Telecomunicaciones e Ingeniería de Sistemas de la ETSE. Este software utiliza técnicas de procesado de señal de alta sensibilidad (HS-GNSS) que permite al usuario determinar su posición en entornos de difícil propagación como puede ser el caso de los escenarios interiores. Los datos experimentales se analizan en función del nivel de multipath que afecta a la señal de cada uno de los satélites, y la degradación que los escenarios interiores provocan en las señales, a causa del mobiliario, paredes, personas, etc. Para analizar los datos experimentales, se ha utilizado una métrica presentada en el congreso internacional EuCAP 2009, con la que es posible caracterizar las señales en función del nivel de multipath.

Optimització i implementació en Simulink de l'adquisició d'un senyal GPS amb blocs FFT

Aquest projecte es tracta de la optimització i la implementació de l’etapa d’adquisició d’un receptor GPS. També inclou una revisió breu del sistema GPS i els seus principis de funcionament. El procés d’adquisició s’ha estudiat amb detall i programat en els entorns de treball Matlab i Simulink. El fet d’implementar aquesta etapa en dos entorns diferents ha estat molt útil tant de cara a l’aprenentatge com també per la comprovació dels resultats obtinguts. El principal objectiu del treball és el disseny d’un model Simulink que es capaç d’adquirir una senyal capturada amb hardware real. En realitat, s’han fet dues implementacions: una que utilitza blocs propis de Simulink i l’altra que utilitza blocs de la llibreria Xilinx. D’aquesta manera, posteriorment, es facilitaria la transició del model a la FPGA utilitzant l’entorn ISE de Xilinx. La implementació de l’etapa d’adquisició es basa en el mètode de cerca de fase de codi en paral·lel, el qual empra la operació correlació creuada mitjançant la transformada ràpida de Fourier (FFT). Per aquest procés es necessari realitzar dues transformades (per a la senyal entrant i el codi de referència) i una antitransformada de Fourier (per al resultat de la correlació). Per tal d’optimitzar el disseny s’utilitza un bloc FFT, ja que tres blocs consumeixen gran part dels recursos d’una FPGA. En lloc de replicar el bloc FFT, en el model el bloc és compartit en el temps gràcies a l’ús de buffers i commutadors, com a resultat la quantitat de recursos requerits per una implementació en una FPGA es podria reduir considerablement.