Respuesta a Temozolomida en pacientes con melanoma metastásico en un hospital de tercer nivel de atención: Response to Temozolomide in patients with metastatic melanoma in a third level medical facility

Introduction.Melanoma is a public health problem; it represents 4% of malignant skin tumors and is responsible for 80% of deaths from this type of neoplasm. Objective: Show the response to Temozolomide in patients with metastatic melanoma. Methods: Descriptive, cross-sectional study. The clinical response of patients with metastatic melanoma, managed with Temozolomide 200 mg/m2 once a day was analyzed for 5 days every 28 days. The risk factors analyzed were: histological variety, topographic region of the primary lesion, metastasis, ulceration, and Breslow. Descriptive statistics were used for normality Kolmogorov-Smirnoff, Student's t-test, and binary logistic regression. Results: There were 51 les, 47 met the criteria; 25 men, 22 women, mean age 54.45, minimum 22, maximum 85 years, Complete response was obtained in 3 (6.3%), partial response in 7 (14.8%), stable disease in 10 (21%) and disease progression in 27 (57.44%) patients. The presence of ulceration is associated with a higher Breslow index and, as a result, a higher risk of disease progression. Conclusions: Temozolomide as monotherapy is a treatment that presents low rates of complete response and partial response, showing better results in patients with lymph node metastases.Introducción: El melanoma es un problema de salud pública, representa 4% de los tumores malignos de la piel y es responsable de 80% de las muertes por este tipo de neoplasias. Objetivo: presentar la respuesta a Temozolomida en pacientes con melanoma metastásico. Métodos: Estudio descriptivo, transversal. Se analizó la respuesta clínica de pacientes con melanoma metastásico, manejados con Temozolomida 200 mg/m2 una vez al día, durante 5 días cada 28 días. Los factores de riesgo analizados fueron: variedad histológica, región topográfica de lesión primaria, metástasis, ulceración y Breslow. Se utilizó estadística descriptiva, para normalidad Kolmogorov-Smirnoff, t de Student, así como regresión logística binaria. Resultados: Fueron 51 expedientes, 47 cumplieron con los criterios; 25 hombres, 22 mujeres, edad media 54.45, mínima 22, máxima 85 años, Se obtuvo una respuesta completa en 3(6.3%), respuesta parcial 7(14.8%), enfermedad estable en 10(21%) y progresión de la enfermedad en 27(57.44%) pacientes. La presencia de ulceración se asocia a mayor índice de Breslow, y como resultado, mayor riesgo de progresión de la enfermedad. Conclusiones: Temozolomida como monoterapia es un tratamiento que presenta bajas tasas de respuesta completa y respuesta parcial, mostrando mejores resultados en pacientes con metástasis ganglionares

IAA : Información y actualidad astronómica (4)

Sumario : Investigación : Galaxias huéspedes de cuásares.-- El gigante gaseoso y su gran mancha roja.-- Ventana Abierta: Un futuro incierto.-- Charlas con… John Hutchings.-- Actualidad Científica: La edad de la galaxia.-- Sorpresas en el cinturón de Kuiper.-- Actividades IAA.-- Agenda.N

Aprendizaje basado en proyectos (PBL) aplicado a la docencia de sistemas tecnológicos de última generación

El planteamiento general de la docencia de asignaturas cuyo contenido es eminentemente tecnológico, presenta el reto del constante y rápido cambio asociado a los avances en desarrollo tecnológico. Dentro de este contexto, se plantea emplear un método basado en la generación de herramientas que permitan un seguimiento autónomo de los cambios frente a opciones más descriptivas del estado actual de los sistemas estudiados. Sobre esta base, se estudia la idoneidad de un contexto basado en el desarrollo de proyectos que, si bien tienen necesariamente que abordar una temática particular, supone una forma a priori interesante de generar las habilidades necesarias para el aprendizaje autónomo y continuado

PMAS integral field spectroscopy of luminous infrared galaxies. I.- The atlas

In this paper we present PMAS optical (3800-7200A) IFS of the northern hemisphere portion of a volume-limited sample of 11 LIRGs. The PMAS observations typically cover the central ~5kpc and are complemented with HST/NICMOS images. For most LIRGs in our sample, the peaks of the continuum and gas (e.g., Halpha, [NII]) emissions coincide, unlike what is observed in local, strongly interacting ULIRGs. The only exceptions are galaxies with circumnuclear rings of star formation where the most luminous Halpha emitting regions are found in the rings rather than in the nuclei, and the displacements are well understood in terms of differences in the stellar populations. A large fraction of the nuclei of these LIRGs are classified as LINER and intermediate LINER/HII, or composite objects. The excitation conditions of the integrated emission depend on the relative contributions of HII regions and the diffuse emission to the line emission over the PMAS FoV. Galaxies dominated by high surface-brightness HII regions show integrated HII-like excitation. A few galaxies show slightly larger integrated [NII]/Halpha and [SII]/Halpha line ratios than the nuclear ones, probably because of more contribution from the diffuse emission. The Halpha velocity fields over the central few kpc are generally consistent, at least to first order, with rotational motions. The velocity fields of most LIRGs are similar to those of disk galaxies, in contrast to the highly perturbed fields of most local, strongly interacting ULIRGs. The peak of the Halpha velocity dispersion coincides with the position of the nucleus and is likely to be tracing mass. All these results are similar to the properties of z~1 LIRGs, and they highlight the importance of detailed studies of flux-limited samples of local LIRGs. (Abridged)Comment: Accepted for publication in Astronomy and Astrophysic

High-precision astrometry and photometry with the JWST/MIRI imager

Astrometry is one of the main pillars of astronomy, and one of its oldest branches. Over the years, an increasing number of astrometric works by means of Hubble Space Telescope (HST) data have revolutionized our understanding of various phenomena. With the launch of JWST, it becomes almost instinctive to want to replicate or improve these results with data taken with the newest, state-of-the-art, space-based telescope. In this regard, the initial focus of the community has been on the Near-Infrared (NIR) detectors on board of JWST because of their high spatial resolution. This paper begins the effort to capture and apply what has been learned from HST to the Mid-InfraRed Instrument (MIRI) of JWST by developing the tools to obtain high-precision astrometry and photometry with its imager. We describe in detail how to create accurate effective point-spread-function (ePSF) models and geometric-distortion corrections, analyze their temporal stability, and test their quality to the extent of what is currently possible with the available data in the JWST MAST archive. We show that careful data reduction provides deep insight on the performance and intricacies of the MIRI imager, and of JWST in general. In an effort to help the community to devise new observing programs, we make our ePSF models and geometric-distortion corrections publicly available.Comment: 22 pages, 18 figures, 1 table. Accepted for publication in PASP. The ePSF models, geometric-distortion solutions and codes are available at the links provided in the manuscrip

Stellar populations of galaxies in the ALHAMBRA survey up to z∼1z \sim 1. I. MUFFIT: A Multi-Filter Fitting code for stellar population diagnostics

We present MUFFIT, a new generic code optimized to retrieve the main stellar population parameters of galaxies in photometric multi-filter surveys, and we check its reliability and feasibility with real galaxy data from the ALHAMBRA survey. Making use of an error-weighted $\chi^2$-test, we compare the multi-filter fluxes of galaxies with the synthetic photometry of mixtures of two single stellar populations at different redshifts and extinctions, to provide through a Monte Carlo method the most likely range of stellar population parameters (mainly ages and metallicities), extinctions, redshifts, and stellar masses. To improve the diagnostic reliability, MUFFIT identifies and removes from the analysis those bands that are significantly affected by emission lines. We highlight that the retrieved age-metallicity locus for a sample of $z \le 0.22$ early-type galaxies in ALHAMBRA at different stellar mass bins are in very good agreement with the ones from SDSS spectroscopic diagnostics. Moreover, a one-to-one comparison between the redshifts, ages, metallicities, and stellar masses derived spectroscopically for SDSS and by MUFFIT for ALHAMBRA reveals good qualitative agreements in all the parameters. In addition, and using as input the results from photometric-redshift codes, MUFFIT improves the photometric-redshift accuracy by $\sim 10$-$20\%$, and it also detects nebular emissions in galaxies, providing physical information about their strengths. Our results show the potential of multi-filter galaxy data to conduct reliable stellar population studies with the appropiate analysis techniques, as MUFFIT.Comment: 31 pages, 18 figures, accepted for publication in A&

Coordinación de las competencias de Electrónica en el Grado y Máster en Ingeniería de Telecomunicación

La implantación de los cursos tanto de grado como de máster requiere de una continua evaluación y revisión desde el punto de vista de sus contenidos específicos, planificación, evaluación, etc. con el fin de mejorar año a año el proceso de enseñanza-aprendizaje asociado a cada asignatura de forma individual, además de con el fin de mejorar la coordinación entre las diferentes asignaturas. En ese sentido, en el presente trabajo se analiza la materia de electrónica y todas las asignaturas que la integran en el Grado de Ingeniería en Sonido e Imagen en Telecomunicación, y en el Máster en Ingeniería de Telecomunicación, dado que en este caso podemos considerar los estudios de este máster como una continuación natural de los estudios previos del grado correspondiente. En concreto, los objetivos principales del presente trabajo son el seguimiento, coordinación, evaluación y mejora en la distribución de competencias de las asignaturas obligatorias de los cursos primero y segundo del Grado en Ingeniería en Sonido e Imagen en Telecomunicación y las asignaturas obligatorias del Máster en Ingeniería de Telecomunicación

Immunosuppression-independent role of regulatory T cells against hypertension-driven renal dysfunctions

Hypertension-associated cardiorenal diseases represent one of the heaviest burdens for current health systems. In addition to hemodynamic damage, recent results have revealed that hematopoietic cells contribute to the development of these diseases by generating proinflammatory and profibrotic environments in the heart and kidney. However, the cell subtypes involved remain poorly characterized. Here we report that CD39+ regulatory T (TREG) cells utilize an immunosuppression-independent mechanism to counteract renal and possibly cardiac damage during angiotensin II (AngII)-dependent hypertension. This mechanism relies on the direct apoptosis of tissue-resident neutrophils by the ecto-ATP diphosphohydrolase activity of CD39. In agreement with this, experimental and genetic alterations in TREG/TH cell ratios have a direct impact on tissue-resident neutrophil numbers, cardiomyocyte hypertrophy, cardiorenal fibrosis, and, to a lesser extent, arterial pressure elevation during AngII-driven hypertension. These results indicate that TREG cells constitute a first protective barrier against hypertension-driven tissue fibrosis and, in addition, suggest new therapeutic avenues to prevent hypertension-linked cardiorenal diseases.This work has been supported by grants from the Castilla-León Autonomous Government (CSI101U13), the Spanish Ministry of Economy and Competitiveness (SAF2012-31371, RD12/0036/0002), Worldwide Cancer Research, the Solórzano Foundation, and the Ramón Areces Foundation to X.R.B. P.M. is funded by the Spanish Ministry of Economy and Competitiveness (SAF2011-27330). S.F., M.M.-M., J.R.-V., and A.M.-M. were supported by the Spanish Ministry of Economy and Competitiveness through BES-2010-031386, CSIC JAE-Doc, Juan de la Cierva, and BES-2009-016103 contracts, respectively. Spanish government-sponsored funding to X.R.B. is partially supported by the European Regional Development Fund.Peer Reviewe

La Leishmaniosis en la provincia de Granada: estudio de la enzootia canina

Con el fin de determinar el papel que desempeña el perro en la epidemiología de la Leishmaniosis en la provincia de Granada hemos realizado un estudio de la sintomatología, índice de parasitación y distribución de esta enfermedad en dicho animal. En cuanto a la sintomatología, algunos perros presentaban el cuadro clínico característico de la enfermedad, pero otros, sin embargo, presentaban unos síntomas totalmente inespecíficos y, en consecuencia, fácil de confundir con otras enfermedades. La realización de una encuesta al azar en 1.503 perros proporciona un índice de parasitación del 8,84%, lo que nos da una idea de la importancia de la enfermedad. Además, se puede observar que, aunque los mayores índices de parasitación se encuentran en las comarcas tradicionalmente consideradas endémicas (La Costa y Las Alpujarras), la enfermedad está ampliamente esparcida por toda la provincia y con unos índices dignos de tener en cuenta. En consecuencia, habría que considerar como zona endémica de leishmaniosis a toda la provincia, y no se debería restringir este término solamente a la región costero-alpujarreña, tal y como ha venido sucediendo