AMIC: Affective multimedia analytics with inclusive and natural communication

Traditionally, textual content has been the main source of information extraction and indexing, and other technologies that are capable of extracting information from the audio and video of multimedia documents have joined later. Other major axis of analysis is the emotional and affective aspect intrinsic in human communication. This information of emotions, stances, preferences, figurative language, irony, sarcasm, etc. is fundamental and irreplaceable for a complete understanding of the content in conversations, speeches, debates, discussions, etc. The objective of this project is focused on advancing, developing and improving speech and language technologies as well as image and video technologies in the analysis of multimedia content adding to this analysis the extraction of affective-emotional information. As additional steps forward, we will advance in the methodologies and ways for presenting the information to the user, working on technologies for language simplification, automatic reports and summary generation, emotional speech synthesis and natural and inclusive interaction

Towards Inter-Subject Project-Based Learning in Programming-Related Courses at Computer Science Studies

[EN] Curriculum design of University Degrees in Spain is mainly based on scheduling atomic, self-contained semester subjects during a 4-year period. This scheduling is driven by one major constraint: to ensure that previous subject pre-requisites are met for each course. Thus, basic subjects without college-level pre-requisites are typically scheduled in the first year, first semester, while the rest are properly planned in a sequential manner, complying the aforementioned condition. This is, basically, the only proof of inter-subject coordination in such degrees, taking place at the design stage. During the academic period, however, there is no vertical nor horizontal inter-subject coordination, not even among closely-related subjects. In order to increase inter-subject coordination and to exploit its potential benefit for students, the projectbased learning (PBL) methodology shows on the scene. This approach organizes learning around student-driven projects aiming to solve real-life problems. This close applicability to the real world expedites intrinsic motivation of students, and consequently, their learning process tends to be deeper and more significant. Furthermore, PBL applied at the inter-subject level increases curriculum cohesion and makes students more engaged and compromised with its global objectives. In this paper we describe the design of PBL models involving two pairs of programming-related subjects from the Computer Engineering Degree at the Universitat Politècnica de València. The first one associates the ¿Programming¿ with the ¿Data Structures and Algorithms¿ subject, while the second one engages the ¿Introduction to Video-Games Programming¿ with the ¿Digital Image Synthesis¿ one. It is an ambitious pilot programme that will require a high coordination effort among participating professors and student teams.This article has been supported by the Vice-rectorate for Digital Resources and Documentation (Vicerrectorado de Recursos Digitales y Documentación) and Vice-Rectorate for Studies, Quality and Accreditation (Vicerrectorado de Estudios, Calidad y Acreditación) under the Call for Learning + Teaching (Convocatoria Aprendizaje + Docencia (A+D 2019)) and Project Code: 1678-A. The authors would like to acknowledge the support of the Institute of Educational Sciences (Instituto de Ciencias de la Educación) of Universitat Politècnica de València, the Evaluation and Monitoring Commission for Educational Innovation and Improvement Projects (Comisión de Evaluación y Seguimiento de Proyectos de Innovación y Mejora Educativa (CESPIME)) and Escuela Politécnica Superior de AlcoyLinares-Pellicer, J.; Orta-López, J.; Salavert-Torres, J.; Segura Flor, MJ.; Silvestre Cerdà, JA.; Sanchis, R. (2020). Towards Inter-Subject Project-Based Learning in Programming-Related Courses at Computer Science Studies. EDULEARN Proceedings (Internet). 3973-3978. https://doi.org/10.21125/edulearn.2020.1075S3973397

Kepler-47: A Transiting Circumbinary Multi-Planet System

We report the detection of Kepler-47, a system consisting of two planets orbiting around an eclipsing pair of stars. The inner and outer planets have radii 3.0 and 4.6 times that of the Earth, respectively. The binary star consists of a Sun-like star and a companion roughly one-third its size, orbiting each other every 7.45 days. With an orbital period of 49.5 days, eighteen transits of the inner planet have been observed, allowing a detailed characterization of its orbit and those of the stars. The outer planet's orbital period is 303.2 days, and although the planet is not Earth-like, it resides within the classical "habitable zone", where liquid water could exist on an Earth-like planet. With its two known planets, Kepler-47 establishes that close binary stars can host complete planetary systems.Comment: To appear on Science Express August 28, 11 pages, 3 figures, one table (main text), 56 pages, 28 figures, 10 table

HAT-P-44b, HAT-P-45b, and HAT-P-46b: Three Transiting Hot Jupiters in Possible Multi-Planet Systems

We report the discovery by the HATNet survey of three new transiting extrasolar planets orbiting moderately bright (V=13.2, 12.8 and 11.9) stars. The planets have orbital periods of 4.3012, 3.1290, and 4.4631 days, masses of 0.39, 0.89, and 0.49 Mjup, and radii of 1.28, 1.43, and 1.28 Rjup. The stellar hosts have masses of 0.94, 1.26, and 1.28 Msun. Each system shows significant systematic variations in its residual radial velocities indicating the possible presence of additional components. Based on its Bayesian evidence, the preferred model for HAT-P-44 consists of two planets, including the transiting component, with the outer planet having a period of 220 d and a minimum mass of 1.6 Mjup. Due to aliasing we cannot rule out an alternative solution for the outer planet having a period of 438 d and a minimum mass of 3.7 Mjup. For HAT-P-45 at present there is not enough data to justify the additional free parameters included in a multi-planet model, in this case a single-planet solution is preferred, but the required jitter of 22.5 +- 6.3 m/s is relatively high for a star of this type. For HAT-P-46 the preferred solution includes a second planet having a period of 78 d and a minimum mass of 2.0 Mjup, however the preference for this model over a single-planet model is not very strong. While substantial uncertainties remain as to the presence and/or properties of the outer planetary companions in these systems, the inner transiting planets are well characterized with measured properties that are fairly robust against changes in the assumed models for the outer planets. Continued RV monitoring is necessary to fully characterize these three planetary systems, the properties of which may have important implications for understanding the formation of hot Jupiters.Comment: 21 pages, 10 figures, 14 tables, submitted to A

Mechanisms of resistance in postharvest fruit-pathogen interaction

Abstract T he objective of this review was to bring together concepts related to studies aimed at elucidating defense mechanisms against disease-causing agents, mainly in postharvest. Like plants, fruits are exposed to attack by pathogens that cause rot during postharvest storage, resulting in considerable losses. To control these pathogens, synthetic chemicals are used; however, since they are toxic, genetic resistance is regarded as a viable alternative. Fruits can withstand pathogens by means of physical barriers (presence of thick cuticular or trichome layers) and chemical ones, or through induced defenses that are activated once the host detects the presence of the pathogen, triggering the oxidative burst during the early hours of interaction. This burst entails the generation of reactive oxygen species (ROS), such as superoxide (O 2ˉ) , hydroxyl radical (OHˉ) or hydrogen peroxide (H 2 O 2 ), and the activation of genes involved in several metabolic pathways. The study of such mechanisms may allow detecting disease-resistant genetic materials, thus reducing the use of toxic products. Resumen E l objetivo de esta revisión fue conjuntar conceptos relacionados con estudios dirigidos a elucidar los mecanismos de defensa contra agentes causantes de enfermedades, principalmente en poscosecha. Al igual que las plantas, los frutos se encuentran expuestos al ataque por patógenos que producen podredumbres durante su almacenamiento en poscosecha, causando considerables pérdidas. Para el control de dichos patógenos, se emplean productos químicos de síntesis que son tóxicos, y la resistencia genética se considera una alternativa viable. Los frutos pueden tolerar a los patógenos mediante barreras físicas (presencia de capas gruesas de cutícula o de tricomas) y químicas, o bien, a través de defensas inducidas que se activan una vez que el huésped detecta la presencia del patógeno, desencadenando la explosión oxidativa durante las primeras horas de la interacción. Esta explosión conlleva la generación de especies reactivas de oxígeno (ROS) como el superóxido (O 2ˉ) , el radical hidroxilo (OHˉ) o el peróxido de hidrógeno (H 2 O 2 ), y la activación de genes involucrados en diversas rutas metabólicas. El estudio de tales mecanismos puede permitir detectar materiales genéticos resistentes a enfermedades, reduciendo así el uso de productos tóxicos

Working memory training improves cognitive efficiency in multiple sclerosis patients

La Esclerosis Múltiple (EM) es una enfermedad en la que la memoria de trabajo (MT) se encuentra comúnmente afectada. Estudiar la eficacia de un programa de entrenamiento en MT en pacientes de EM. 29 pacientes de EM Remitente-Recurrente fueron seleccionados para el estudio: 15 realizaron el entrenamiento en MT y 14 fueron seleccionados como grupo control. Todos los participantes fueron valorados a nivel neuropsicológico y se adquirieron imágenes de Resonancia Magnética funcional (RMf) durante la realización de la tarea 2 y 3-back (basal y post tratamiento-7 días). Los pacientes entrenados mejoraron su ejecución en 2 y 3-back (p<.001), tanto en aciertos como en tiempo de reacción (TR). Durante la realización de la tarea 2-back, los pacientes sin entrenamiento mostraron una mayor activación en el giro angular derecho (FWEc=125, p<.001) que correlaciona con el TR (r=.459, p<.05). También se observó una disminución de la actividad cerebral en el grupo de pacientes entrenados en el giro precentral derecho (FWEc=273, p<.01). Los resultados encontrados apoyan la eficacia del entrenamiento cognitivo en MT. Los pacientes de EM entrenados muestran una clara mejoría a nivel conductual asociada a un incremento de la eficiencia cognitiva, es decir, un menor uso de recursos cerebrales obteniendo una mejor ejecución.Multiple Sclerosis (MS) is a disease usually associated with a working memory (WM) impairment. Study the efficacy of a WM cognitive training program in MS patients. 29 relapsing-remitting MS patients were enrolled in the study: 15 underwent WM training and 14 were assigned to a control group. All participants were neuropsychologically assessed and Functional Magnetic Resonance imaging (fMRI) images were acquired during 2 and 3-back execution (baseline and post-training +7days). Training improved MS patients’ performance in 2 and 3-back, hence showing shorter reaction times (RT) and higher percentages of correct responses (p<.001). During 2-back performance, non-trained MS-patients exhibited a greater activation in in right angular gyrus (FWEc=125, p<.001) that was correlated to RT (r=.459, p<.05). Further, lower activation in right precentral gyrus in the trained MS-patients (FWEc=273, p<.01) was also found. The results obtained demonstrates the effectiveness of a WM training program in MS-patients. Trained MS-patients showed a marked improvement of WM performance and increased cognitive efficiency, i.e, using less cerebral resources to achieve higher performance

Masses, radii, and orbits of small Kepler planets : The transition from gaseous to rocky planets

We report on the masses, sizes, and orbits of the planets orbiting 22 Kepler stars. There are 49 planet candidates around these stars, including 42 detected through transits and 7 revealed by precise Doppler measurements of the host stars. Based on an analysis of the Kepler brightness measurements, along with high-resolution imaging and spectroscopy, Doppler spectroscopy, and (for 11 stars) asteroseismology, we establish low false-positive probabilities (FPPs) for all of the transiting planets (41 of 42 have an FPP under 1%), and we constrain their sizes and masses. Most of the transiting planets are smaller than three times the size of Earth. For 16 planets, the Doppler signal was securely detected, providing a direct measurement of the planet's mass. For the other 26 planets we provide either marginal mass measurements or upper limits to their masses and densities; in many cases we can rule out a rocky composition. We identify six planets with densities above 5 g cm-3, suggesting a mostly rocky interior for them. Indeed, the only planets that are compatible with a purely rocky composition are smaller than 2 R ⊕. Larger planets evidently contain a larger fraction of low-density material (H, He, and H2O).Peer reviewedFinal Accepted Versio

Obesity is not associated with disease-free interval, melanoma-specific survival, or overall survival in patients with clinical stage IB-II melanoma after SLNB

BACKGROUND AND OBJECTIVES: Clinicopathologic characteristics have prognostic value in clinical stage IB‐II patients with melanoma. Little is known about the prognostic value of obesity that has been associated with an increased risk for several cancer types and worsened prognosis after diagnosis. This study aims to examine effects of obesity on outcome in patients with clinical stage IB‐II melanoma. METHODS: Prospectively recorded data of patients with clinical stage IB‐II melanoma who underwent sentinel lymph node biopsy (SLNB) between 1995 and 2018 at the University Medical Center of Groningen were collected from medical files and retrospectively analyzed. Cox‐regression analyses were used to determine associations between obesity (body mass index> 30), tumor (location, histology, Breslow‐thickness, ulceration, mitotic rate, SLN‐status) and patient‐related variables (gender, age, and social‐economic‐status [SES]) and disease‐free interval (DFI), melanoma‐specific survival (MSS), and overall survival (OS). RESULTS: Of the 715 patients, 355 (49.7%) were women, median age was 55 (range 18.6‐89) years, 149 (20.8%) were obese. Obesity did not significantly affect DFI (adjusted hazard ratio [HR] = 1.40; 95% confidence interval [CI] = 0.98–2.00; p = 0.06), MSS (adjusted HR = 1.48;95%CI = 0.97–2.25; p = 0.07), and OS (adjusted HR = 1.25; 95% CI = 0.85–1.85; p = 0.25). Increased age, arm location, increased Breslow‐thickness, ulceration, increased mitotic rate, and positive SLN‐status were significantly associated with decreased DFI, MSS, and OS. Histology, sex, and SES were not associated. CONCLUSION: Obesity was not associated with DFI, MSS, or OS in patients with clinical stage IB‐II melanoma who underwent SLNB

Obliquities of Hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments

We provide evidence that the obliquities of stars with close-in giant planets were initially nearly random, and that the low obliquities that are often observed are a consequence of star-planet tidal interactions. The evidence is based on 14 new measurements of the Rossiter-McLaughlin effect (for the systems HAT-P-6, HAT-P-7, HAT-P-16, HAT-P-24, HAT-P-32, HAT-P-34, WASP-12, WASP-16, WASP-18, WASP-19, WASP-26, WASP-31, Gl 436, and Kepler-8), as well as a critical review of previous observations. The low-obliquity (well-aligned) systems are those for which the expected tidal timescale is short, and likewise the high-obliquity (misaligned and retrograde) systems are those for which the expected timescale is long. At face value, this finding indicates that the origin of hot Jupiters involves dynamical interactions like planet-planet interactions or the Kozai effect that tilt their orbits, rather than inspiraling due to interaction with a protoplanetary disk. We discuss the status of this hypothesis and the observations that are needed for a more definitive conclusion.Comment: Accepted for publication in ApJ; typos corrected, 2 broken references fixed, 26 pages, 25 figure

Towards a combined use of geophysics and remote sensing techniques for the characterization of a singular building: “El Torreón” (the tower) at Ulaca oppidum (Solosancho, Ávila, Spain)

This research focuses on the study of the ruins of a large building known as “El Torreón” (the Tower), belonging to the Ulaca oppidum (Solosancho, Province of Ávila, Spain). Different remote sensing and geophysical approaches have been used to fulfil this objective, providing a better understanding of the building’s functionality in this town, which belongs to the Late Iron Age (ca. 300–50 BCE). In this sense, the outer limits of the ruins have been identified using photogrammetry and convergent drone flights. An additional drone flight was conducted in the surrounding area to find additional data that could be used for more global interpretations. Magnetometry was used to analyze the underground bedrock structure and ground penetrating radar (GPR) was employed to evaluate the internal layout of the ruins. The combination of these digital methodologies (surface and underground) has provided a new perspective for the improved interpretation of “El Torreón” and its characteristics. Research of this type presents additional guidelines for better understanding of the role of this structure with regards to other buildings in the Ulaca oppidum. The results of these studies will additionally allow archaeologists to better plan future interventions while presenting new data that can be used for the interpretation of this archaeological complex on a larger scale