Gestor de persistència genèric

En aquest TFC es proposa utilitzar una única classe Gestor de Disc parametritzable per un fitxer, concretament un fitxer XML, que reculli les dades necessàries extretes d'una base de dades. Es marca com objectiu que el fitxer XML sigui igual per a qualsevol SGBD amb el que aconseguirem independència de la plataforma.

Creació d'un CD-Live LINUX UOC

Aquesta memòria recull les tasques realitzades per tal d'obtenir un CD que contingui una versió de LINUX personalitzada, amb la utilitat de poder ser utilitzada com a eina bàsica pels alumnes al llarg dels estudis cursats a la UOC. Es tracta d'un CD autoarrencable, cosa que vol dir que es pot executar directament des de qualsevol lector de CD, sense haver-se d'instal·lar permanentment en el disc dur dels PC.

Plataforma GNU/Linux : Servidor de Base de Dades

L'objectiu d'aquest projecte és aconseguir una distribució basada en el projecte Metadistros capaç d'arrencar des del CD. L'avantatge d'aquest tipus de distribucions és disposar de tot un sistema operatiu juntament amb tot un lot d'aplicacions sense necessitat d'instal·lar res al disc dur.

myvideos : creació de repositoris de videos (Moodle)

Amb l'objectiu de fomentar l'ús de recursos audiovisuals, s'ha desenvolupat un bloc de Moodle que permet afegir vídeos codificant-los automàticament al format Flash Video, reduint així l'espai de disc i l'ample de banda necessaris per fer-ne ús. Cada usuari té el seu propi repositori i tots els vídeos afegits com a públics passen a formar part d'un repositori d'accés públic. La darrera versió del programari és disponible a: http://moodle.org/mod/data/view.php?d=13&rid=3977

Gestió dels arxius duplicats distribuïts

El treball diari en diferents entorns, tant pel que fa a sistemes operatius, com maquinariscom llocs físics diferents fa que la informació hagi d'estar a tot arreu. Aquesta informacióha d'estar actualitzada. A més a més, hi ha la possibilitat de l'ús de les diferentspossibilitats d'emmagatzematge (local, disc extern, núvol...).Tot i que les eines de treball al núvol (per exemple, Google Docs, EyeOS...) són moltcompletes, el fet d'utilitzar els programaris instal·lats als ordinadors encara segueix sentnecessari, per les seves capacitats i rapidesa. Més quan, estem treballant amb gransvolums d'informació (com grans documents, imatges, audio...).

Search for dark matter using VHE gamma-ray telescopes

One of the unresolved questions of modern physics is the nature of Dark Matter. Strong experimental evidences suggest that the presence of this elusive component in the energy budget of the Universe is quite significant, without, however, being able to provide conclusive information about its nature. The most plausible scenario is that of weakly interacting massive particles (WIMPs), that includes a large class of non-baryonic Dark Matter candidates with a mass typically between few tens of GeV and few TeVs, and a cross section of the order of weak interactions. Search for Dark Matter particles using very high energy gamma-ray Cherenkov telescopes is based on the model that WIMPs can self-annihilate, leading to production of detectable species, like photons. These photons are very energetic, and since unreflected by the Universe's magnetic fields, they can be traced straight to the source of their creation. The downside of the approach is a great amount of background radiation, coming from the conventional astrophysical objects, that usually hides clear signals of the Dark Matter particle interactions. That is why good choice of the observational candidates is the crucial factor in search for Dark Matter. With MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov Telescopes), a two-telescope ground-based system located in La Palma, Canary Islands, we choose objects like dwarf spheroidal satellite galaxies of the Milky Way and galaxy clusters for our search. Our idea is to increase chances for WIMPs detection by pointing to objects that are relatively close, with great amount of Dark Matter and with as-little-as-possible pollution from the stars. At the moment, several observation projects are ongoing and analyses are being performed.

LHMC : un centre multimèdia Linux

En aquest projecte es desenvolupa el maquinari i el programari d'un centre multimèdia. Aquest és un sistema elemental, capaç de reproduir i copiar fitxers d'imatge, so i vídeo provinents del mateix sistema, d'un dispositiu extern com per exemple un disc òptic o una memòria flash, i també d'altres sistemes connectats en xarxa. El programari és de codi obert, està desenvolupat per funcionar amb el sistema operatiu Linux i està implementat amb Java. Es realitza una aplicació escalable per facilitar l’addició de funcionalitats.

Artrodesis posterior C1-C2. Resultados y comparación de la fijación transarticular e interarticular en una serie de 36 pacientes

Objetivo. Analizar los resultados de la fijación transarticular e interarticular en dos series de pacientes. Métodos. Se analizaron 36 pacientes con inestabilidad C1-C2, 20 tratados mediante fijación transarticular, y 15 con fijación interarticular. Se obtuvieron datos sobre las complicaciones, evolución radiológica y resultados clínicos. Resultados. De los tratados con fijación transarticular se obtuvieron resultados buenos en 17 casos, regular en 2 y malo en 1. En la fijación interarticular en 14 se obtuvieron un buen resultado, y regular en 2. Conclusiones. La fijación C1-C2 transarticular e interarticular resulta segura, con presentando altas tasas de buenos resultados con pocas complicaciones.

Bristle pattern formation in the thorax formation of Drosophila: a systems level approach

A fundamental question in developmental biology is how tissues are patterned to give rise to differentiated body structures with distinct morphologies. The Drosophila wing disc offers an accessible model to understand epithelial spatial patterning. It has been studied extensively using genetic and molecular approaches. Bristle patterns on the thorax, which arise from the medial part of the wing disc, are a classical model of pattern formation, dependent on a pre-pattern of trans-activators and –repressors. Despite of decades of molecular studies, we still only know a subset of the factors that determine the pre-pattern. We are applying a novel and interdisciplinary approach to predict regulatory interactions in this system. It is based on the description of expression patterns by simple logical relations (addition, subtraction, intersection and union) between simple shapes (graphical primitives). Similarities and relations between primitives have been shown to be predictive of regulatory relationships between the corresponding regulatory factors in other Systems, such as the Drosophila egg. Furthermore, they provide the basis for dynamical models of the bristle-patterning network, which enable us to make even more detailed predictions on gene regulation and expression dynamics. We have obtained a data-set of wing disc expression patterns which we are now processing to obtain average expression patterns for each gene. Through triangulation of the images we can transform the expression patterns into vectors which can easily be analysed by Standard clustering methods. These analyses will allow us to identify primitives and regulatory interactions. We expect to identify new regulatory interactions and to understand the basic Dynamics of the regulatory network responsible for thorax patterning. These results will provide us with a better understanding of the rules governing gene regulatory networks in general, and provide the basis for future studies of the evolution of the thorax-patterning network in particular.

Learning in Digital Media: the legacy of McLuhan and his Impact on Formal Education

This paper describes a bibliographic analysis of the vision of Marshal McLuhan and the vision adopted by diverse current authors regarding the use of new interactive learning technologies. The paper also analyzes the transformation that will have to take place in the formal surroundings of education in order to improve their social function. The main points of view and contributions made by diverse authors are discussed. It is important that all actors involved in the educational process take in consideration these contributions in order to be ready for future changes.

Effluent particle removal by microirrigation system filters

The aim of this work was to determine whether the filters used in microirrigation systems can remove potentially emitter-clogging particles. The particle size and volume distributions of different effluents and their filtrates were established, and the efficiency of the removal of these particles and total suspended solids by screen, disc and sand filters determined. In most of the effluents and filtrates, the number of particles with a diameter > 20 μm was minimal. By analysing the particle volume distribution it was found that particles larger than the disc and screen filter pores appeared in the filtrates. However, the sand filter was able to retain particles larger than the pore size. The filtration efficiency depended more on the type of effluent than on the filter. It was also found that the particle size distribution followed a potential law. Analysis of the β exponents showed that the filters did not significantly modify the particle size distribution of the effluents

A new maximum likelihood method for luminosity calibrations

A new statistical parallax method using the Maximum Likelihood principle is presented, allowing the simultaneous determination of a luminosity calibration, kinematic characteristics and spatial distribution of a given sample. This method has been developed for the exploitation of the Hipparcos data and presents several improvements with respect to the previous ones: the effects of the selection of the sample, the observational errors, the galactic rotation and the interstellar absorption are taken into account as an intrinsic part of the formulation (as opposed to external corrections). Furthermore, the method is able to identify and characterize physically distinct groups in inhomogeneous samples, thus avoiding biases due to unidentified components. Moreover, the implementation used by the authors is based on the extensive use of numerical methods, so avoiding the need for simplification of the equations and thus the bias they could introduce. Several examples of application using simulated samples are presented, to be followed by applications to real samples in forthcoming articles.

A search for microquasar candidates at low galactic latitudes

Recent studies of relativistic jet sources in the Galaxy, also known as microquasars, have been very useful in trying to understand the accretion/ejection processes that take place near compact objects. However, the number of sources involved in such studies is still small. In an attempt to increase the number of known microquasars we have carried out a search for new Radio Emitting X-ray Binaries (REXBs). These sources are the ones to be observed later with VLBI techniques to unveil their possible microquasar nature. To this end, we have performed a cross-identification between the X-ray ROSAT all sky survey Bright Source Catalog (RBSC) and the radio NRAO VLA Sky Survey (NVSS) catalogs under very restrictive selection criteria for sources with |b|<5 degrees. We have also conducted a deep observational radio and optical study for six of the selected candidates. At the end of this process two of the candidates appear to be promising, and deserve additional observations aimed to confirm their proposed microquasar nature.

uvbyHbeta photometry of main sequence A type stars.

We present Stroemgren uvby and Hbeta_ photometry for a set of 575 northern main sequence A type stars, most of them belonging to the Hipparcos Input Catalogue, with V from 5mag to 10mag and with known radial velocities. These observations enlarge the catalogue we began to compile some years ago to more than 1500 stars. Our catalogue includes kinematic and astrophysical data for each star. Our future goal is to perform an accurate analysis of the kinematical behaviour of these stars in the solar neighbourhood.

Detection of moving groups among early type stars

Our procedure to detect moving groups in the solar neighbourhood (Chen et al., 1997) in the four-dimensional space of the stellar velocity components and age has been improved. The method, which takes advantadge of non-parametric estimators of density distribution to avoid any a priori knowledge of the kinematic properties of these stellar groups, now includes the effect of observational errors on the process to select moving group stars, uses a better estimation of the density distribution of the total sample and field stars, and classifies moving group stars using all the available information. It is applied here to an accurately selected sample of early-type stars with known radial velocities and Strömgren photometry. Astrometric data are taken from the HIPPARCOS catalogue (ESA, 1997), which results in an important decrease in the observational errors with respect to ground-based data, and ensures the uniformity of the observed data. Both the improvement of our method and the use of precise astrometric data have allowed us not only to confirm the existence of classical moving groups, but also to detect finer structures that in several cases can be related to kinematic properties of nearby open clusters or associations.