Public Policies Still Alive Within a Liberalized Environment: Insights From Costa Rica

We carry out a comparative study of four farm sectors in Costa Rica, based on a dynamic analysis of behaviors regarding institutional changes occurring during the liberalization process. We highlight organizations' capacities to adapt and contribute to institutional changes by implementing economical activities and participating to policy making processes. We show that organizations play a key role in the regulation of farm sectors, and that their success depends on the institutional and organizational thickness they have contributed to create in each sector and responds to a path-dependent logic. ...French Abstract : Nous menons une étude comparative de quatre filières agricoles au Costa Rica, qui repose sur une analyse dynamique des comportements des acteurs des filières au regard des changements institutionnels liés à la libéralisation économique. Les organisations de producteurs agricoles, qui jouent un rôle clé dans la régulation des filières, ont opté pour des comportements stratégiques différents. Nous mettons en évidence les capacités de ces organisations à s'adapter mais également à contribuer aux changements institutionnels en mettant en place des activités technico-économiques de transformation et commercialisation et en participant aux processus de négociation des politiques. Nous montrons que leur succès dépend de la densité institutionnelle et organisationnelle qu'elles ont contribué à créer au sein de chaque filière et s'inscrit dans une logique de dépendance au sentier.ORGANIZATIONS; POLICIES; INSTITUTIONAL CHANGE; PATHDEPENDENCY; ORGANISATIONS; POLITIQUES; CHANGEMENT INSTITUTIONNEL; DEPENDANCE AU SENTIER

Quelles politiques de développement durable au Mali et à Madagascar ?

Ideas and values of "sustainable development" are transfered from the international to the national level in policy-making processes and give way to a recomposition of rural development policies : we study that policy transfert. In Mali and Madagascar, sustainable development policies are quite different. We give an interpretation of these differences by a comparative analysis of strategies of actors involved in policy-making processes. We show that these strategies are related to historical processes. In Mali and Madagascar, the long run analysis of agricultural and rural policy making allows us a better understanding of current sustainable development policies. ...French Abstract : Nous étudions le processus de transfert politique selon lequel les idées et valeurs du " développement durable ", mûries et véhiculées au niveau international, donnent lieu au niveau national à une recomposition des modes publics d'intervention en milieu rural. Au Mali et à Madagascar, les politiques de développement durable recouvrent des expressions différentes. Nous interprétons ces différences par une analyse comparative des stratégies des acteurs intervenant dans le jeu politique. Nous montrons que ces stratégies renvoient à des processus historiques. L'analyse sur le temps long des processus de construction et de mise en oeuvre des politiques agricoles et rurales dans ces pays permet de mieux comprendre les expressions qu'y revêt aujourd'hui le développement durable.POLICIES; RURAL DEVELOPMENT; SUSTAINABLE DEVELOPMENT; DEVELOPPEMENT RURAL; DEVELOPPEMENT DURABLE; MALI; MADAGASCAR

An investigation of the close environment of beta Cep with the VEGA/CHARA interferometer

High-precision interferometric measurements of pulsating stars help to characterize their close environment. In 1974, a close companion was discovered around the pulsating star beta Cep using the speckle interferometry technique and features at the limit of resolution (20 milli-arcsecond or mas) of the instrument were mentioned that may be due to circumstellar material. Beta Cep has a magnetic field that might be responsible for a spherical shell or ring-like structure around the star as described by the MHD models. Using the visible recombiner VEGA installed on the CHARA long-baseline interferometer at Mt. Wilson, we aim to determine the angular diameter of beta Cep and resolve its close environment with a spatial resolution up to 1 mas level. Medium spectral resolution (R=6000) observations of beta Cep were secured with the VEGA instrument over the years 2008 and 2009. These observations were performed with the S1S2 (30m) and W1W2 (100m) baselines of the array. We investigated several models to reproduce our observations. A large-scale structure of a few mas is clearly detected around the star with a typical flux relative contribution of 0.23 +- 0.02. Our best model is a co-rotational geometrical thin ring around the star as predicted by magnetically-confined wind shock models. The ring inner diameter is 8.2 +- 0.8 mas and the width is 0.6 +- 0.7 mas. The orientation of the rotation axis on the plane of the sky is PA = 60 +- 1 deg, while the best fit of the mean angular diameter of beta Cep gives UD[V] = 0.22 +- 0.05 mas. Our data are compatible with the predicted position of the close companion of beta Cep. These results bring additional constraints on the fundamental parameters and on the future MHD and asteroseismological models of the star.Comment: Paper accepted for publication in A&A (in press

Spectral and spatial imaging of the Be+sdO binary phi Persei

The rapidly rotating Be star phi Persei was spun up by mass and angular momentum transfer from a now stripped-down, hot subdwarf companion. Here we present the first high angular resolution images of phi Persei made possible by new capabilities in longbaseline interferometry at near-IR and visible wavelengths. We observed phi Persei with the MIRC and VEGA instruments of the CHARA Array. Additional MIRC-only observations were performed to track the orbital motion of the companion, and these were fit together with new and existing radial velocity measurements of both stars to derive the complete orbital elements and distance. The hot subdwarf companion is clearly detected in the near-IR data at each epoch of observation with a flux contribution of 1.5% in the H band, and restricted fits indicate that its flux contribution rises to 3.3% in the visible. A new binary orbital solution is determined by combining the astrometric and radial velocity measurements. The derived stellar masses are 9.6+-0.3Msol and 1.2+-0.2Msol for the Be primary and subdwarf secondary, respectively. The inferred distance (186 +- 3 pc), kinematical properties, and evolutionary state are consistent with membership of phi Persei in the alpha Per cluster. From the cluster age we deduce significant constraints on the initial masses and evolutionary mass transfer processes that transformed the phi Persei binary system. The interferometric data place strong constraints on the Be disk elongation, orientation, and kinematics, and the disk angular momentum vector is coaligned with and has the same sense of rotation as the orbital angular momentum vector. The VEGA visible continuum data indicate an elongated shape for the Be star itself, due to the combined effects of rapid rotation, partial obscuration of the photosphere by the circumstellar disk, and flux from the bright inner disk.Comment: 16 pages, 6 figures, 1 Anne

Recanalization of obstructed metallic uncovered biliary stent using endobiliary radiofrequency ablation

International audienc

Learning Interpretable Rules for Multi-label Classification

Multi-label classification (MLC) is a supervised learning problem in which, contrary to standard multiclass classification, an instance can be associated with several class labels simultaneously. In this chapter, we advocate a rule-based approach to multi-label classification. Rule learning algorithms are often employed when one is not only interested in accurate predictions, but also requires an interpretable theory that can be understood, analyzed, and qualitatively evaluated by domain experts. Ideally, by revealing patterns and regularities contained in the data, a rule-based theory yields new insights in the application domain. Recently, several authors have started to investigate how rule-based models can be used for modeling multi-label data. Discussing this task in detail, we highlight some of the problems that make rule learning considerably more challenging for MLC than for conventional classification. While mainly focusing on our own previous work, we also provide a short overview of related work in this area.Comment: Preprint version. To appear in: Explainable and Interpretable Models in Computer Vision and Machine Learning. The Springer Series on Challenges in Machine Learning. Springer (2018). See http://www.ke.tu-darmstadt.de/bibtex/publications/show/3077 for further informatio

Exploiting Anti-monotonicity of Multi-label Evaluation Measures for Inducing Multi-label Rules

Exploiting dependencies between labels is considered to be crucial for multi-label classification. Rules are able to expose label dependencies such as implications, subsumptions or exclusions in a human-comprehensible and interpretable manner. However, the induction of rules with multiple labels in the head is particularly challenging, as the number of label combinations which must be taken into account for each rule grows exponentially with the number of available labels. To overcome this limitation, algorithms for exhaustive rule mining typically use properties such as anti-monotonicity or decomposability in order to prune the search space. In the present paper, we examine whether commonly used multi-label evaluation metrics satisfy these properties and therefore are suited to prune the search space for multi-label heads.Comment: Preprint version. To appear in: Proceedings of the Pacific-Asia Conference on Knowledge Discovery and Data Mining (PAKDD) 2018. See http://www.ke.tu-darmstadt.de/bibtex/publications/show/3074 for further information. arXiv admin note: text overlap with arXiv:1812.0005

Direct constraint on the distance of y2 Velorum from AMBER/VLTI observations

In this work, we present the first AMBER observations, of the Wolf-Rayet and O (WR+O) star binary system y2 Velorum. The AMBER instrument was used with the telescopes UT2, UT3, and UT4 on baselines ranging from 46m to 85m. It delivered spectrally dispersed visibilities, as well as differential and closure phases, with a resolution R = 1500 in the spectral band 1.95-2.17 micron. We interpret these data in the context of a binary system with unresolved components, neglecting in a first approximation the wind-wind collision zone flux contribution. We show that the AMBER observables result primarily from the contribution of the individual components of the WR+O binary system. We discuss several interpretations of the residuals, and speculate on the detection of an additional continuum component, originating from the free-free emission associated with the wind-wind collision zone (WWCZ), and contributing at most to the observed K-band flux at the 5% level. The expected absolute separation and position angle at the time of observations were 5.1±0.9mas and 66±15° respectively. However, we infer a separation of 3.62+0.11-0.30 mas and a position angle of 73+9-11°. Our analysis thus implies that the binary system lies at a distance of 368+38-13 pc, in agreement with recent spectrophotometric estimates, but significantly larger than the Hipparcos value of 258+41-31 pc