Dificultades en el aprendizaje del diseño de software orientado a objetos: un estudio cualitativo longitudinal

Las compañías de desarrollo de software buscan reducir costes a través del desarrollo de diseños que permitan: a) facilidad en la distribución del trabajo de desarrollo, con la menor comunicación de las partes; b) modificabilidad, permitiendo realizar cambios sobre un módulo sin alterar las otras partes y; c) comprensibilidad, permitiendo estudiar un módulo del sistema a la vez. Estas características elementales en el diseño de software se logran a través del diseño de sistemas cuasi-descomponibles, cuyo modelo teórico fue introducido por Simon en su búsqueda de una teoría general de los sistemas. En el campo del diseño de software, Parnas propone un camino práctico para lograr sistemas cuasi-descomponibles llamado el Principio de Ocultación de Información. El Principio de Ocultación de Información es un criterio diferente de descomposición en módulos, cuya implementación logra las características deseables de un diseño eficiente a nivel del proceso de desarrollo y mantenimiento. El Principio y el enfoque orientado a objetos se relacionan debido a que el enfoque orientado a objetos facilita la implementación del Principio, es por esto que cuando los objetos empiezan a tomar fuerza, también aparecen paralelamente las dificultades en el aprendizaje de diseño de software orientado a objetos, las cuales se mantienen hasta la actualidad, tal como se reporta en la literatura. Las dificultades en el aprendizaje de diseño de software orientado a objetos tiene un gran impacto tanto en las aulas como en la profesión. La detección de estas dificultades permitirá a los docentes corregirlas o encaminarlas antes que éstas se trasladen a la industria. Por otro lado, la industria puede estar advertida de los potenciales problemas en el proceso de desarrollo de software. Esta tesis tiene como objetivo investigar sobre las dificultades en el diseño de software orientado a objetos, a través de un estudio empírico. El estudio fue realizado a través de un estudio de caso cualitativo, que estuvo conformado por tres partes. La primera, un estudio inicial que tuvo como objetivo conocer el entendimiento de los estudiantes alrededor del Principio de Ocultación de Información antes de que iniciasen la instrucción. La segunda parte, un estudio llevado a cabo a lo largo del período de instrucción con la finalidad de obtener las dificultades de diseño de software y su nivel de persistencia. Finalmente, una tercera parte, cuya finalidad fue el estudio de las dificultades esenciales de aprendizaje y sus posibles orígenes. Los participantes de este estudio pertenecieron a la materia de Software Design del European Master in Software Engineering de la Escuela Técnica Superior de Ingenieros Informáticos de la Universidad Politécnica de Madrid. Los datos cualitativos usados para el análisis procedieron de las observaciones en las horas de clase y exposiciones, entrevistas realizadas a los estudiantes y ejercicios enviados a lo largo del período de instrucción. Las dificultades presentadas en esta tesis en sus diferentes perspectivas, aportaron conocimiento concreto de un estudio de caso en particular, realizando contribuciones relevantes en el área de diseño de software, docencia, industria y a nivel metodológico. ABSTRACT The software development companies look to reduce costs through the development of designs that will: a) ease the distribution of development work with the least communication between the parties; b) changeability, allowing to change a module without disturbing the other parties and; c) understandability, allowing to study a system module at a time. These basic software design features are achieved through the design of quasidecomposable systems, whose theoretical model was introduced by Simon in his search for a general theory of systems. In the field of software design, Parnas offers a practical way to achieve quasi-decomposable systems, called The Information Hiding Principle. The Information Hiding Principle is different criterion for decomposition into modules, whose implementation achieves the desirable characteristics of an efficient design at the development and maintenance level. The Principle and the object-oriented approach are related because the object-oriented approach facilitates the implementation of The Principle, which is why when objects begin to take hold, also appear alongside the difficulties in learning an object-oriented software design, which remain to this day, as reported in the literature. Difficulties in learning object-oriented software design has a great impact both in the classroom and in the profession. The detection of these difficulties will allow teachers to correct or route them before they move to the industry. On the other hand, the industry can be warned of potential problems related to the software development process. This thesis aims to investigate the difficulties in learning the object-oriented design, through an empirical study. The study was conducted through a qualitative case study, which consisted of three parts. The first, an initial study was aimed to understand the knowledge of the students around The Information Hiding Principle before they start the instruction. The second part, a study was conducted during the entire period of instruction in order to obtain the difficulties of software design and their level of persistence. Finally, a third party, whose purpose was to study the essential difficulties of learning and their possible sources. Participants in this study belonged to the field of Software Design of the European Master in Software Engineering at the Escuela Técnica Superior de Ingenieros Informáticos of Universidad Politécnica de Madrid. The qualitative data used for the analysis came from the observations in class time and exhibitions, performed interviews with students and exercises sent over the period of instruction. The difficulties presented in this thesis, in their different perspectives, provided concrete knowledge of a particular case study, making significant contributions in the area of software design, teaching, industry and methodological level.

Objetos y sistemas = Objects and systems

Nunca hemos entendido el proyecto de arquitectura como una colección de pianos más o menos bien estructurados. Proyectar es despejar incógnitas y por tanto caminar por sendas aparentemente vacías de rastros. Proyectar es perderse para entender no tanto el camino sino fundamentalmente el territorio que se recorre.

Detecting, Localizing and Following Dynamic Objects with a Mini-UAV

This paper presents an approach for the detection, localization and following of dynamic terrestrial objects using a mini-UAV. The development is intended to be used for surveillance of large infrastructures. The detection algorithm is based on finding several pre-defined characteristics of the target, such as color, shape and size. The process used to localize the target, once it is detected, is based on an inversion of the Pinhole camera model. The task of following the Summit XL was designed to keep the target inside the field of view of the camera, and it was implemented in the form of a PID controller. The system has been tested both in simulation and with real robots, showing promising results.

On the geometry of solutions of the quasi-geostrophic and Euler equations

We study solutions of the two-dimensional quasi-geostrophic thermal active scalar equation involving simple hyperbolic saddles. There is a naturally associated notion of simple hyperbolic saddle breakdown. It is proved that such breakdown cannot occur in finite time. At large time, these solutions may grow at most at a quadruple-exponential rate. Analogous results hold for the incompressible three-dimensional Euler equation.

Tight frames of k-plane ridgelets and the problem of representing objects that are smooth away from d-dimensional singularities in Rn

For each pair (n, k) with 1 ≤ k < n, we construct a tight frame (ρλ : λ ∈ Λ) for L2 (Rn), which we call a frame of k-plane ridgelets. The intent is to efficiently represent functions that are smooth away from singularities along k-planes in Rn. We also develop tools to help decide whether k-plane ridgelets provide the desired efficient representation. We first construct a wavelet-like tight frame on the X-ray bundle χn,k—the fiber bundle having the Grassman manifold Gn,k of k-planes in Rn for base space, and for fibers the orthocomplements of those planes. This wavelet-like tight frame is the pushout to χn,k, via the smooth local coordinates of Gn,k, of an orthonormal basis of tensor Meyer wavelets on Euclidean space Rk(n−k) × Rn−k. We then use the X-ray isometry [Solmon, D. C. (1976) J. Math. Anal. Appl. 56, 61–83] to map this tight frame isometrically to a tight frame for L2(Rn)—the k-plane ridgelets. This construction makes analysis of a function f ∈ L2(Rn) by k-plane ridgelets identical to the analysis of the k-plane X-ray transform of f by an appropriate wavelet-like system for χn,k. As wavelets are typically effective at representing point singularities, it may be expected that these new systems will be effective at representing objects whose k-plane X-ray transform has a point singularity. Objects with discontinuities across hyperplanes are of this form, for k = n − 1.

Effects of the Heartbeat Wales programme over five years on behavioural risks for cardiovascular disease: quasi-experimental comparison of results from Wales and a matched reference area

Objective: To assess the net 5 year effects of intervention of a community based demonstration project, the Heartbeat Wales programme, on modifiable behavioural risks for prevention of cardiovascular disease.

TectoRNA: modular assembly units for the construction of RNA nano-objects

Structural information on complex biological RNA molecules can be exploited to design tectoRNAs or artificial modular RNA units that can self-assemble through tertiary interactions thereby forming nanoscale RNA objects. The selective interactions of hairpin tetraloops with their receptors can be used to mediate tectoRNA assembly. Here we report on the modulation of the specificity and the strength of tectoRNA assembly (in the nanomolar to micromolar range) by variation of the length of the RNA subunits, the nature of their interacting motifs and the degree of flexibility of linker regions incorporated into the molecules. The association is also dependent on the concentration of magnesium. Monitoring of tectoRNA assembly by lead(II) cleavage protection indicates that some degree of structural flexibility is required for optimal binding. With tectoRNAs one can compare the binding affinities of different tertiary motifs and quantify the strength of individual interactions. Furthermore, in analogy to the synthons used in organic chemistry to synthesize more complex organic compounds, tectoRNAs form the basic assembly units for constructing complex RNA structures on the nanometer scale. Thus, tectoRNA provides a means for constructing molecular scaffoldings that organize functional modules in three-dimensional space for a wide range of applications.

Statistical analysis of shape of objects based on landmark data.

Two objects with homologous landmarks are said to be of the same shape if the configurations of landmarks of one object can be exactly matched with that of the other by translation, rotation/reflection, and scaling. The observations on an object are coordinates of its landmarks with reference to a set of orthogonal coordinate axes in an appropriate dimensional space. The origin, choice of units, and orientation of the coordinate axes with respect to an object may be different from object to object. In such a case, how do we quantify the shape of an object, find the mean and variation of shape in a population of objects, compare the mean shapes in two or more different populations, and discriminate between objects belonging to two or more different shape distributions. We develop some methods that are invariant to translation, rotation, and scaling of the observations on each object and thereby provide generalizations of multivariate methods for shape analysis.

Possible links between BL Lacertae objects and quasars from very long baseline interferometry radio data.

Systematic differences in the very long baseline interferometry (VLBI) radio polarization structure and average VLBI component speeds of BL Lacertae objects and quasars support the view that the observational distinction between these classes, based in large part on the strength of their optical line emission, is meaningful; in other words, this distinction reflects significant differences in the physical conditions in these sources. Possible models providing a link between the optical and VLBI properties of BL Lacertae objects and quasars are discussed. Most VLBI polarization observations to date have been global observations made at 6 cm; recent results suggest that the VLBI polarization structure of some sources may change dramatically on scales smaller than those probed by these 6-cm observations.

Cortical activity flips among quasi-stationary states.

Parallel recordings of spike trains of several single cortical neurons in behaving monkeys were analyzed as a hidden Markov process. The parallel spike trains were considered as a multivariate Poisson process whose vector firing rates change with time. As a consequence of this approach, the complete recording can be segmented into a sequence of a few statistically discriminated hidden states, whose dynamics are modeled as a first-order Markov chain. The biological validity and benefits of this approach were examined in several independent ways: (i) the statistical consistency of the segmentation and its correspondence to the behavior of the animals; (ii) direct measurement of the collective flips of activity, obtained by the model; and (iii) the relation between the segmentation and the pair-wise short-term cross-correlations between the recorded spike trains. Comparison with surrogate data was also carried out for each of the above examinations to assure their significance. Our results indicated the existence of well-separated states of activity, within which the firing rates were approximately stationary. With our present data we could reliably discriminate six to eight such states. The transitions between states were fast and were associated with concomitant changes of firing rates of several neurons. Different behavioral modes and stimuli were consistently reflected by different states of neural activity. Moreover, the pair-wise correlations between neurons varied considerably between the different states, supporting the hypothesis that these distinct states were brought about by the cooperative action of many neurons.

Stellar populations in bulges of spiral galaxies

We present a few results of a work in progress tackling the radial spectroscopic properties of bulges of spiral galaxies.

Mass-metallicity relation explored with CALIFA I. Is there a dependence on the star-formation rate?

We studied the global and local ℳ-Z relation based on the first data available from the CALIFA survey (150 galaxies). This survey provides integral field spectroscopy of the complete optical extent of each galaxy (up to 2−3 effective radii), with a resolution high enough to separate individual H II regions and/or aggregations. About 3000 individual H II regions have been detected. The spectra cover the wavelength range between [OII]3727 and [SII]6731, with a sufficient signal-to-noise ratio to derive the oxygen abundance and star-formation rate associated with each region. In addition, we computed the integrated and spatially resolved stellar masses (and surface densities) based on SDSS photometric data. We explore the relations between the stellar mass, oxygen abundance and star-formation rate using this dataset. We derive a tight relation between the integrated stellar mass and the gas-phase abundance, with a dispersion lower than the one already reported in the literature (σ_Δlog (O/H) = 0.07 dex). Indeed, this dispersion is only slightly higher than the typical error derived for our oxygen abundances. However, we found no secondary relation with the star-formation rate other than the one induced by the primary relation of this quantity with the stellar mass. The analysis for our sample of ~3000 individual H II   regions confirms (i) a local mass-metallicity relation and (ii) the lack of a secondary relation with the star-formation rate. The same analysis was performed with similar results for the specific star-formation rate. Our results agree with the scenario in which gas recycling in galaxies, both locally and globally, is much faster than other typical timescales, such like that of gas accretion by inflow and/or metal loss due to outflows. In essence, late-type/disk-dominated galaxies seem to be in a quasi-steady situation, with a behavior similar to the one expected from an instantaneous recycling/closed-box model.

The ionized gas in the CALIFA early-type galaxies I. Mapping two representative cases: NGC 6762 and NGC 5966

As part of the ongoing CALIFA survey, we have conducted a thorough bidimensional analysis of the ionized gas in two E/S0 galaxies, NGC 6762 and NGC 5966, aiming to shed light on the nature of their warm ionized ISM. Specifically, we present optical (3745–7300 Å) integral field spectroscopy obtained with the PMAS/PPAK integral field spectrophotometer. Its wide field-of-view (1′ × 1′) covers the entire optical extent of each galaxy down to faint continuum surface brightnesses. To recover the nebular lines, we modeled and subtracted the underlying stellar continuum from the observed spectra using the STARLIGHT spectral synthesis code. The pure emission-line spectra were used to investigate the gas properties and determine the possible sources of ionization. We show the advantages of IFU data in interpreting the complex nature of the ionized gas in NGC 6762 and NGC 5966. In NGC 6762, the ionized gas and stellar emission display similar morphologies, while the emission line morphology is elongated in NGC 5966, spanning ~6 kpc, and is oriented roughly orthogonal to the major axis of the stellar continuum ellipsoid. Whereas gas and stars are kinematically aligned in NGC 6762, the gas is kinematically decoupled from the stars in NGC 5966. A decoupled rotating disk or an “ionization cone” are two possible interpretations of the elongated ionized gas structure in NGC 5966. The latter would be the first “ionization cone” of such a dimension detected within a weak emission-line galaxy. Both galaxies have weak emission-lines relative to the continuum[EW(Hα) ≲ 3 Å] and have very low excitation, log([OIII]λ5007/Hβ) ≲ 0.5. Based on optical diagnostic ratios ([OIII]λ5007/Hβ, [NII]λ6584/Hα, [SII]λ6717, 6731/Hα, [OI]λ6300/Hα), both objects contain a LINER nucleus and an extended LINER-like gas emission. The emission line ratios do not vary significantly with radius or aperture, which indicates that the nebular properties are spatially homogeneous. The gas emission in NGC 6762 can be best explained by photoionization by pAGB stars without the need of invoking any other excitation mechanism. In the case of NGC 5966, the presence of a nuclear ionizing source seems to be required to shape the elongated gas emission feature in the “ionization cone” scenario, although ionization by pAGB stars cannot be ruled out. Further study of this object is needed to clarify the nature of its elongated gas structure.

Low-resolution spectroscopy and spectral energy distributions of selected sources towards σ Orionis

Aims. We study in detail nine sources in the direction of the young σ Orionis cluster, which is considered to be a unique site for studying stellar and substellar formation. The nine sources were selected because of their peculiar properties, such as extremely-red infrared colours or excessively strong Hα emission for their blue optical colours. Methods. We acquired high-quality, low-resolution spectroscopy (R ∼ 500) of the nine targets with ALFOSC at the Nordic Optical Telescope. We also re-analysed [24]-band photometry from MIPS/Spitzer and compiled the highest quality photometric dataset available at the ViJHK_s passbands and the four IRAC/Spitzer channels, for constructing accurate spectral energy distributions between 0.55 and 24 μm. Results. The nine targets were classified into: one Herbig Ae/Be star with a scattering edge-on disc; two G-type stars; one X-ray flaring, early-M, young star with chromospheric Hα emission; one very low-mass, accreting, young spectroscopic binary; two young objects at the brown-dwarf boundary with the characteristics of classical T Tauri stars; and two emission-line galaxies, one undergoing star formation, and another whose spectral energy distribution is dominated by an active galactic nucleus. We also discovered three infrared sources associated with overdensities in a cold cloud of the cluster centre. Conclusions. Low-resolution spectroscopy and spectral energy distributions are a vital tool for measuring the physical properties and evolution of young stars and candidates in the σ Orionis cluster.