SQualTrack: A Tool for Robust Fault Detection

One of the techniques used to detect faults in dynamic systems is analytical redundancy. An important difficulty in applying this technique to real systems is dealing with the uncertainties associated with the system itself and with the measurements. In this paper, this uncertainty is taken into account by the use of intervals for the parameters of the model and for the measurements. The method that is proposed in this paper checks the consistency between the system's behavior, obtained from the measurements, and the model's behavior; if they are inconsistent, then there is a fault. The problem of detecting faults is stated as a quantified real constraint satisfaction problem, which can be solved using the modal interval analysis (MIA). MIA is used because it provides powerful tools to extend the calculations over real functions to intervals. To improve the results of the detection of the faults, the simultaneous use of several sliding time windows is proposed. The result of implementing this method is semiqualitative tracking (SQualTrack), a fault-detection tool that is robust in the sense that it does not generate false alarms, i.e., if there are false alarms, they indicate either that the interval model does not represent the system adequately or that the interval measurements do not represent the true values of the variables adequately. SQualTrack is currently being used to detect faults in real processes. Some of these applications using real data have been developed within the European project advanced decision support system for chemical/petrochemical manufacturing processes and are also described in this paper

Competencia en precios entre operadores turísticos españoles

El presente articulo analiza el grado de competencia en precios de los operadores turísticos que ofrecen hoteles del litoral peninsular español y que compiten en el segmento que demanda 'sol y playa'. Plantea la hipótesis de que los precios para un mismo hotel (que en la mayoría de casos es ofrecido por más de un operador) no pueden presentar diferencias sustanciales al tratarse de la comercialización de productos homogéneos. El análisis se realiza a partir de la explotación de diferentes catálogos de operadores turísticos y toma como muestra tres poblaciones de la Costa Brava (Lloret de Mar, Blanes y Tossa de Mar). El estudio se ha realizado para el régimen de pensión completa (que es el mayoritario) y se han introducido los precios de unas fechas clave de la temporada turística. Las medidas estadísticas utilizadas han sido básicamente el porcentaje que representan el precio máximo y el precio mínimo de cada hotel y para cada fecha respecto al precio medio, la suma de dichos porcentajes, con un coeficiente corrector función del numero de operadores, la desviación estándar, y el coeficiente de variación de Pearson . Asimismo, para corroborar las explicaciones a los resultados obtenidos del análisis empírico se contactó con algunos de dichos operadores. Los resultados obtenidos muestran que la distancia media entre el precio máximo y el precio mínimo se sitúa alrededor del 8,67%, lo que se nos antoja una corta diferencia de precios, con lo que se corroboraría la hipótesis de partida. Dichas diferencias se acortan en las fechas de mayor demanda debido a que los operadores aprovechan para realizar más beneficios

Candidate counterparts to the soft gamma-ray flare in the direction od LSI+61303

A short duration burst reminiscent of a soft gamma-ray repeater/anomalous X-ray pulsar behaviour was detected in the direction of LS I +61 303 by the Swift satellite. While the association with this well known gamma-ray binary is likely, a different origin cannot be excluded. Aims. We explore the error box of this unexpected flaring event and establish the radio, near-infrared and X-ray sources in our search for any peculiar alternative counterpart. Methods. We carried out a combined analysis of archive Very Large Array radio data of LS I +61 303 sensitive to both compact and extended emission. We also reanalysed previous near infrared observations with the 3.5 m telescope of the Centro Astronómico Hispano Alemán and X-ray observations with the Chandra satellite. Results. Our deep radio maps of the LS I +61 303 environment represent a significant advancement on previous work and 16 compact radio sources in the LS I +61 303 vicinity are detected. For some detections, we also identify near infrared and X-ray counterparts. Extended emission features in the field are also detected and confirmed. The possible connection of some of these sources with the observed flaring event is considered. Based on these data, we are unable to claim a clear association between the Swift-BAT flare and any of the sources reported here. However, this study represents the most sophisticated attempt to determine possible alternative counterparts other than LS I +61 303.

Informe sobre la investigación en Astronomía en España (1999-2001)

Este documento recoge los resultados de un estudio sobre el estado de la investigación astronómica en los centros del sistema español de investigación y desarrollo, en lo referente al trienio 1999-2001. Su objetivo es conocer y dar a conocer la situación real de las actividades investigadoras de una disciplina que se ha desarrollado espectacularmente en los últimos decenios en España ...

Chorros relativistas de origen estelar: los microcuasares

Galactic microquasars are certainly one of the most recent additions to the field of high energy Astrophysics. These new objects are just X-ray binaries with the ability to generate relativistic jets and their interest has been growing during the last decade. Today, they represent primary targets for all space based observatories working in the X-ray and [gamma]-ray domains. Behind such interest, there is hope that their study will assist us to understand some of the analog phenomena observed in distant quasars and active galactic nuclei, wich share with microquasars practically the same scaled-up physics. Microquasars are also believed to be among the different kind of sources responsible for the violent and ever changing appearance of the [gamma]-ray ski. In this paper we review the general situation of the microquasar topic, their identification and study, including comments on the recent observational and theoretical discoveries most relevant in our opinion.

Probing quantum gravity using photons from a flare of the active galactic nucleus Markarian 501 observed by the MAGIC telescope

We analyze the timing of photons observed by the MAGIC telescope during a flare of the active galactic nucleus Mkn 501 for a possible correlation with energy, as suggested by some models of quantum gravity (QG), which predict a vacuum refractive index similar or equal to 1 + (E/M-QGn)(n), n = 1, 2. Parametrizing the delay between gamma-rays of different energies as Delta t = +/-tau E-1 or Delta t = +/-tau E-q(2), we find tau(1) = (0.030 +/- 0.012) s/GeV at the 2.5-sigma level, and tau(q) = (3.71 +/- 2.57) x 10(-6) s/GeV2, respectively. We use these results to establish lower limits M-QG1 > 0.21 X 10(18) GeV and M-QG2 > 0.26 x 10(11) GeV at the 95% C.L. Monte Carlo studies confirm the MAGIC sensitivity to propagation effects at these levels. Thermal plasma effects in the source are negligible, but we cannot exclude the importance of some other source effect.

Non-thermal emission from microquasar/ISM interaction

Context. The interaction of microquasar jets with their environment can produce non-thermal radiation as in the case of extragalactic outflows impacting on their surroundings. Significant observational evidence of jet/medium interaction in galactic microquasars has been collected in the past few years, although little theoretical work has been done regarding the resulting non-thermal emission. Aims. In this work, we investigate the non-thermal emission produced in the interaction between microquasar jets and their environment, and the physical conditions for its production. Methods. We developed an analytical model based on those successfully applied to extragalactic sources. The jet is taken to be a supersonic and mildly relativistic hydrodynamical outflow. We focus on the jet/shocked medium structure in its adiabatic phase, and assume that it grows in a self-similar way. We calculate the fluxes and spectra of the radiation produced via synchrotron, inverse Compton, and relativistic bremsstrahlung processes by electrons accelerated in strong shocks. A hydrodynamical simulation is also performed to investigate further the jet interaction with the environment and check the physical parameters used in the analytical model. Results. For reasonable values of the magnetic field, and using typical values of the external matter density, the non-thermal particles could produce significant amounts of radiation at different wavelengths, although they do not cool primarily radiatively, but by adiabatic losses. The physical conditions of the analytical jet/medium interaction model are consistent with those found in the hydrodynamical simulation. Conclusions. Microquasar jet termination regions could be detectable at radio wavelengths for current instruments sensitive to ~arcminute scales. At X-ray energies, the expected luminosities are moderate, although the emitter is more compact than the radio one. The source may be detectable by XMM-Newton or Chandra, with 1-10 arcsec of angular resolution. The radiation at gamma-ray energies may be within the detection limits of the next generation of satellite and ground-based instruments.

Microquasars: uns sistemes estel.lars extraordinaris

Quan alcem els ulls en una nit estel·lada d'estiu, sovint veiem una banda de llum que travessa la volta del cel amb una lluentor blanquinosa ...

X-ray and radio observations of RX J1826.2-1450/LS 5039

RX J1826.2-1450/LS 5039 has been recently proposed to be a radio emitting high mass X-ray binary. In this paper, we present an analysis of its X-ray timing and spectroscopic properties using different instruments on board the RXTE satellite. The timing analysis indicates the absence of pulsed or periodic emission on time scales of 0.02-2000 s and 2-200 d, respectively. The source spectrum is well represented by a power-law model, plus a Gaussian component describing a strong iron line at 6.6 keV. Significant emission is seen up to 30 keV, and no exponential cut-off at high energy is required. We also study the radio properties of the system according to the GBI-NASA Monitoring Program. RX J1826.2-1450/LS 5039 continues to display moderate radio variability with a clearly non-thermal spectral index. No strong radio outbursts have been detected after several months.

Estrelles binàries de raigs-X amb emissió ràdio

Les binaries o estrelles dobles fisiques son sistemes formats per dues estrelles lligades gravitatoriament. Avui en dia sabem que aquest és un fenomen molt comú a la galaxia, on aproximadament la meitat de les estrelles s'han format i han donat lloc a aquesta mena de sistemes...

Photometric and Halpha observations of LSI+61·303: detection of a 26 day V and JHK band modulation

We present new optical and infrared photometric observations and high resolution H α spectra of the periodic radio star LSI+61◦303. The optical photometric data set covers the time interval 1985-1993 and amounts to about a hundred nights. A period of ∼26 days is found in the V band. The infrared data also present evidence for a similar periodicity, but with higher amplitude of variation ((0.m 2). The spectroscopic observations include 16 intermediate and high dispersion spectra of LSI+61◦303 collected between January 1989 and February 1993. The H α emission line profile and its variations are analyzed. Several emission line parameters -- among them the H α EW and the width of the H α red hump -- change strongly at or close to radio maximum, and may exhibit periodic variability. We also observe a significant change in the peak separation. The H α profile of LSI+61◦303 does not seem peculiar for a Be star. However, several of the observed variations of the H α profile can probably be associated with the presence of the compact, secondary star.

Evidence of Halpha periodicities in LSI+61·303

We present the results of analyzing H$\alpha$ spectra of the radio emitting X-ray binary LS I+61303. For the first time, the same 26.5 d radio period is clearly detected in the H$\alpha$ emission line. Moreover, the equivalent width and the peak separation of the H$\alpha$ emission line seem also to vary over a time scale of 1600 days. This points towards the $\sim4$ yr modulation, detected in the radio outburst amplitude, being probably a result of variations in the mass loss rate of the Be star and/or density variability in the circumstellar disk. In addition, the dependence of the peak separation from the equivalent width informs us that the LS I+61303 circumstellar disk is among the densest of Be-stars.

V-band observations of V4641 Sagittarii

In this note we report high time resolution V Johnson photometry of the microquasar V4641 Sgr (SAX J1819.3-2525 - XTE J1819-254). This source was discovered as an X-ray transient by BeppoSAX and RossiXTE satellites (In't Zand et al. 1999; Markwardt et al. 1999). On 1999 September, a very fast transient optical and X-ray outburst was observed, reaching up to ...

Utilización de software de corrección automática en el campo de las ciencias de la salud

We live in an era of profound changes in university education. The implementation of Bologna plan has led us to raise new teaching methodologies, to review the role of the student, competency assessment, the incorporation of ICT. Unthinkable acts, one or two decade ago. The TIC concept is very broad and is attributed to the media, processes and content usage. Inside the supports and platforms, we stress tools that allow automatic correction of exercises, because they are instruments of great educational value because instantly they assess students and provide instant feedback about the knowledge that they have either as message support or note. If the power of these tools, we add the Internet, using e-learning environment, the results allow us to work, edit, evaluate, resolve doubts, and so on, anywhere, anytime. We present part of a platform and the results of its use in the field of health sciences

Desarrollo de una aplicación interactiva multimedia: Elaboración industrial de una emulsión de fase externa silicónica

A partir de una primera experiencia en el desarrollo de una aplicación interactiva multimedia, como fue la elaboración de comprimidos infantiles de paracetamol y aplicación de las Normas de Correcta Fabricación , y visto que ha tenido una gran aceptación por parte de los alumnos, se decidió el realizar una nueva aplicación interactiva multimedia que considerara la otra práctica que se realizaba en la planta piloto del SDM (Servei de Desenvolupament del Medicament), la cual consiste en la elaboración de una emulsión silicónica. Ambas prácticas se llevan a cabo presencialmente en la asignatura de Tecnología Farmacéutica II. En esta segunda aplicación multimedia, si bien se ha mantenido una estructura similar a la primera editada, se ha intentado mejorar todos aquellos aspectos que surgieron durante la programación y la fase de pruebas de dicha multimedia, como por ejemplo el más importante que ha sido el utilizar un tipo de programación que permita visualizar la actividad a través de Internet entre otras muchas mejoras. Además en esta nueva aplicación se ha introducido una actividad que consiste en un simulador de la elaboración de una emulsión en donde los alumnos podrán probar diferentes parámetros de fabricación (velocidad y tiempo de agitación) para encontrar aquellos que den unas características de viscosidad y extensión lo más óptimas posibles. A día de hoy faltan todavía algunos ajustes a dicha aplicación que se pretende ensayar en el curso académico 2004-2005 donde se valorará por parte de los alumnos y profesores su aplicabilidad y su aceptación real. En esta comunicación se presenta las áreas desarrolladas.