Toxicidad hematológica asociada al tratamiento con sulfonamidas y pirimetamina en pacientes VIH positivos y toxoplasmosis cerebral en un hospital de tercer nivel en Colombia

Objective. To determine the frequency of hematologic adverse effects associated with treatment for cerebral toxoplasmosis in HIV / AIDS patients. Design: Retrospective case series. Location: University Hospital Hernando Moncaleano Perdomo (HMP), Neiva, Colombia. Population. Patients with cerebral toxoplasmosis and HIV / AIDS treated at the infection service unit between 2006 and 2009. Población. Pacientes con toxoplasmosis cerebral y VIH/SIDA atendidos en el servicio de infectología entre 2006-2009. Results. 51 patients were evaluated during the study period. 40 (78%) were men. The average age was 33 years. 25 patients had cerebral toxoplasmosis as the first marker of HIV infection. 60.7% of cases had hematologic toxicity. 42% of patients had anemia before treatment. The peak onset of bone marrow toxicity was the sixth day of the start of treatment schedule. The anti-toxoplasma scheme that was most commonly associated with myelotoxicity was the combination of pyrimethamine/sulfadoxine, trimethoprim-sulfamethoxazole and clindamycin in 48% of cases. Objetivo. Determinar la frecuencia efectos adversos hematológicos asociados al tratamiento para toxoplasmosis cerebral en pacientes VIH/SIDA. Diseño. Serie de casos retrospectiva. Lugar. Hospital Universitario Hernando Moncaleano Perdomo (HMP), Neiva- Colombia. Población. Pacientes con toxoplasmosis cerebral y VIH/SIDA atendidos en el servicio de Infectología entre 2006-2009. Resultados. 51 pacientes fueron evaluados durante el periodo de estudio. 40 (78%) fueron hombres. El promedio de edad fue 33 años. 25 pacientes presentaban toxoplasmosis cerebral como primer marcador de Infección VIH. El 60,7% de los casos presentaron toxicidad hematológica. 42% de los pacientes presentaron anemia previa al tratamiento. El pico de aparición de toxicidad medular fue al sexto día de inicio del esquema de tratamiento. El esquema antitoxoplasma que más comúnmente fue asociado a mielotoxicidad fue la combinación de pirimetamina/sulfadoxina, trimetoprimsulfametoxazol y clindamicina en 48% de los casos

Second-line treatment in advanced gastric cancer : Data from the Spanish AGAMENON registry

Second-line treatments boost overall survival in advanced gastric cancer (AGC). However, there is a paucity of information as to patterns of use and the results achieved in actual clinical practice. The study population comprised patients with AGC in the AGAMENON registry who had received second-line. The objective was to describe the pattern of second-line therapies administered, progression-free survival following second-line (PFS-2), and post-progression survival since first-line (PPS). 2311 cases with 2066 progression events since first-line (89.3%) were recorded; 245 (10.6%) patients died during first-line treatment and 1326/2066 (64.1%) received a second-line. Median PFS-2 and PPS were 3.1 (95% CI, 2.9-3.3) and 5.8 months (5.5-6.3), respectively. The most widely used strategies were monoCT (56.9%), polyCT (15.0%), ramucirumab+CT (12.6%), platinum-reintroduction (8.3%), trastuzumab+CT (6.1%), and ramucirumab (1.1%). PFS-2/PPS medians gradually increased in monoCT, 2.6/5.1 months; polyCT 3.4/6.3 months; ramucirumab+CT, 4.1/6.5 months; platinum-reintroduction, 4.2/6.7 months, and for the HER2+ subgroup in particular, trastuzumab+CT, 5.2/11.7 months. Correlation between PFS since first-line and OS was moderate in the series as a whole (Kendall's τ = 0.613), lower in those subjects who received second-line (Kendall's τ = 0.539), especially with ramucirumab+CT (Kendall's τ = 0.413). This analysis reveals the diversity in second-line treatment for AGC, highlighting the effectiveness of paclitaxel-ramucirumab and, for a selected subgroup of patients, platinum reintroduction; both strategies endorsed by recent clinical guidelines

A catalogue of structural and morphological measurements for DES Y1

We present a structural and morphological catalogue for 45 million objects selected from the first year data of the Dark Energy Survey (DES). Single Sersic fits and non-parametric ´ measurements are produced for g, r, and i filters. The parameters from the best-fitting Sersic ´ model (total magnitude, half-light radius, Sersic index, axis ratio, and position angle) are mea- ´ sured with GALFIT; the non-parametric coefficients (concentration, asymmetry, clumpiness, Gini, M20) are provided using the Zurich Estimator of Structural Types (ZEST+). To study the statistical uncertainties, we consider a sample of state-of-the-art image simulations with a realistic distribution in the input parameter space and then process and analyse them as we do with real data: this enables us to quantify the observational biases due to PSF blurring and magnitude effects and correct the measurements as a function of magnitude, galaxy size, Sersic ´ index (concentration for the analysis of the non-parametric measurements) and ellipticity. We present the largest structural catalogue to date: we find that accurate and complete measurements for all the structural parameters are typically obtained for galaxies with SEXTRACTOR MAG AUTO I ≤ 21. Indeed, the parameters in the filters i and r can be overall well recovered up to MAG AUTO ≤ 21.5, corresponding to a fitting completeness of ∼90 per cent below this threshold, for a total of 25 million galaxies. The combination of parametric and non-parametric structural measurements makes this catalogue an important instrument to explore and understand how galaxies form and evolve. The catalogue described in this paper will be publicly released alongside the DES collaboration Y1 cosmology data products at the following URL: https://des.ncsa.illinois.edu/releases

An r -process enhanced star in the dwarf galaxy Tucana III

Chemically peculiar stars in dwarf galaxies provide a window for exploring the birth environment of stars with varying chemical enrichment. We present a chemical abundance analysis of the brightest star in the newly discovered ultra-faint dwarf galaxy candidate Tucana III. Because it is particularly bright for a star in an ultra-faint Milky Way (MW) satellite, we are able to measure the abundance of 28 elements, including 13 neutron-capture species. This star, DES J235532.66−593114.9 (DES J235532), shows a mild enhancement in neutron-capture elements associated with the r-process and can be classified as an r-I star. DES J235532 is the first r-I star to be discovered in an ultra-faint satellite, and Tuc III is the second extremely low-luminosity system found to contain rprocess enriched material, after Reticulum II. Comparison of the abundance pattern of DES J235532 with r-I and r-II stars found in other dwarf galaxies and in the MW halo suggests a common astrophysical origin for the neutron-capture elements seen in all r-process enhanced stars. We explore both internal and external scenarios for the r-process enrichment of Tuc III and show that with abundance patterns for additional stars, it should be possible to distinguish between them

VDES J2325−5229 a z = 2.7 gravitationally lensed quasar discovered using morphology-independent supervised machine learning

We present the discovery and preliminary characterization of a gravitationally lensed quasar with a source redshift zs = 2.74 and image separation of 2.9 arcsec lensed by a foreground zl = 0.40 elliptical galaxy. Since optical observations of gravitationally lensed quasars showthe lens system as a superposition of multiple point sources and a foreground lensing galaxy, we have developed a morphology-independent multi-wavelength approach to the photometric selection of lensed quasar candidates based on Gaussian Mixture Models (GMM) supervised machine learning. Using this technique and gi multicolour photometric observations from the Dark Energy Survey (DES), near-IR JK photometry from the VISTA Hemisphere Survey (VHS) and WISE mid-IR photometry, we have identified a candidate system with two catalogue components with iAB = 18.61 and iAB = 20.44 comprising an elliptical galaxy and two blue point sources. Spectroscopic follow-up with NTT and the use of an archival AAT spectrum show that the point sources can be identified as a lensed quasar with an emission line redshift of z = 2.739 ± 0.003 and a foreground early-type galaxy with z = 0.400 ± 0.002.We model the system as a single isothermal ellipsoid and find the Einstein radius θE ∼ 1.47 arcsec, enclosed mass Menc ∼ 4 × 1011 M and a time delay of ∼52 d. The relatively wide separation, month scale time delay duration and high redshift make this an ideal system for constraining the expansion rate beyond a redshift of 1

Biospas proyecto 2 : micorrizas, patógenos, meso-macro-fauna y biocontrol (Pae- pid-2007-0054)

El actual sistema agrícola de Argentina basa la mayor parte de su producción en la siembra directa y una limitada rotación de cultivos. En base a el paradigma de la sustentabilidad se pueden evaluar cambios en la asociación de Hongos Micorrícicos (HM) con raíces de diversos cultivos y las poblaciones presentes en el suelo; la incidencia de enfermedades en el cultivo y los niveles de inóculo presentes en los rastrojos y asimismo la supresividad de los suelos y por consiguiente la presencia de enfermedad de los cultivos y el efecto de control que pudieran proveer las Micorrizas Arbusculares (MA). El planteo de SD versus LT también plantea modificaciones tanto de la estructura del suelo como en el sistema y las comunidades de Meso y Macrofauna (MMF) que en él habitan. La hipótesis de trabajo plantea que la incidencia y severidad de las fitoenfermedades puede disminuirse por la rotación de cultivos y que las poblaciones de hongos micorrícicos se modifican según la secuencia de rotación. Esto a su vez implica que, incidencia y/o severidad de una enfermedad pueden ser modificadas por HM presentes en el suelo. Por otro lado, abundancia y atributos estructurales de la comunidad de MMF del suelo son afectados por los sistemas de manejo. En este proyecto se determinaran morfológica y molecularmente las especies integrantes de las poblaciones de HM en diferentes secuencias de cultivo. Se compararán las poblaciones de HM presentes en el suelo y las poblaciones en simbiosis activa con raíces de los diferentes cultivos. Se caracterizará y comparará cultivo, suelo y rastrojo desde el punto de vista fitopatológico en diferentes esquemas de rotación. Como resultado de esto se determinará la existencia de interacciones entre la incidencia de enfermedades y la presencia de determinadas micorrizas y evaluar el efecto de cada sistema de manejo sobre la abundancia y los atributos estructurales de la comunidad de MMF del suelo.Fil: Ducasse, Daniel Adrián. Universidad Católica de Córdoba. Facultad de Ciencias Agropecuarias; ArgentinaFil: Plazas, María Cristina. Universidad Católica de Córdoba. Facultad de Ciencias Agropecuarias; ArgentinaFil: De Rossi, Roberto Luis. Universidad Católica de Córdoba. Facultad de Ciencias Agropecuarias; ArgentinaFil: Guerra, Gustavo Darío. Universidad Católica de Córdoba. Facultad de Ciencias Agropecuarias; Argentin

Biospas Proyecto 2 : Micorrizas, Patógenos, Meso-Macro-Fauna y Biocontrol (PAE- PID-2007-0054)

El actual sistema agrícola de Argentina basa la mayor parte de su producción en la siembra directa y una limitada rotación de cultivos. En base a el paradigma de la sustentabilidad se pueden evaluar cambios en la asociación de Hongos Micorrícicos (HM) con raíces de diversos cultivos y las poblaciones presentes en el suelo; la incidencia de enfermedades en el cultivo y los niveles de inóculo presentes en los rastrojos y asimismo la supresividad de los suelos y por consiguiente la presencia de enfermedad de los cultivos y el efecto de control que pudieran proveer las Micorrizas Arbusculares (MA). El planteo de SD versus LT también plantea modificaciones tanto de la estructura del suelo como en el sistema y las comunidades de Meso y Macrofauna (MMF) que en él habitan. La hipótesis de trabajo plantea que la incidencia y severidad de las fitoenfermedades puede disminuirse por la rotación de cultivos y que las poblaciones de hongos micorrícicos se modifican según la secuencia de rotación. Esto a su vez implica que, incidencia y/o severidad de una enfermedad pueden ser modificadas por HM presentes en el suelo. Por otro lado, abundancia y atributos estructurales de la comunidad de MMF del suelo son afectados por los sistemas de manejo. En este proyecto se determinaran morfológica y molecularmente las especies integrantes de las poblaciones de HM en diferentes secuencias de cultivo. Se compararán las poblaciones de HM presentes en el suelo y las poblaciones en simbiosis activa con raíces de los diferentes cultivos. Se caracterizará y comparará cultivo, suelo y rastrojo desde el punto de vista fitopatológico en diferentes esquemas de rotación. Como resultado de esto se determinará la existencia de interacciones entre la incidencia de enfermedades y la presencia de determinadas micorrizas y evaluar el efecto de cada sistema de manejo sobre la abundancia y los atributos estructurales de la comunidad de MMF del suelo.Fil: Ducasse, Daniel Adrián. Universidad Católica de Córdoba. Facultad de Ciencias Agropecuarias; ArgentinaFil: Plazas, María Cristina. Universidad Católica de Córdoba. Facultad de Ciencias Agropecuarias; Argentin

Searching for dark matter annihilation in recently discovered Milky Way satellites with Fermi-LAT

We search for excess γ-ray emission coincident with the positions of confirmed and candidate Milky Way satellite galaxies using six years of data from the Fermi Large Area Telescope (LAT). Our sample of 45 stellar systems includes 28 kinematically confirmed dark-matter-dominated dwarf spheroidal galaxies (dSphs) and 17 recently discovered systems that have photometric characteristics consistent with the population of known dSphs. For each of these targets, the relative predicted γ-ray flux due to dark matter annihilation is taken from kinematic analysis if available, and estimated from a distance-based scaling relation otherwise, assuming that the stellar systems are DM-dominated dSphs. LAT data coincident with four of the newly discovered targets show a slight preference (each ~2σ local) for γ-ray emission in excess of the background. However, the ensemble of derived γ-ray flux upper limits for individual targets is consistent with the expectation from analyzing random blank-sky regions, and a combined analysis of the population of stellar systems yields no globally significant excess (global significance 1 TeV and mDM,t+t-> 70 GeV) and weakening by a factor of ~1.5 at lower masses relative to previously observed limits

Host galaxy identification for supernova surveys

Host galaxy identification is a crucial step for modern supernova (SN) surveys such as the Dark Energy Survey (DES) and the Large Synoptic Survey Telescope (LSST), which will discover SNe by the thousands. Spectroscopic resources are limited, so in the absence of real-time SN spectra these surveys must rely on host galaxy spectra to obtain accurate redshifts for the Hubble diagram and to improve photometric classification of SNe. In addition, SN luminosities are known to correlate with host-galaxy properties. Therefore, reliable identification of host galaxies is essential for cosmology and SN science. We simulate SN events and their locations within their host galaxies to develop and test methods for matching SNe to their hosts. We use both real and simulated galaxy catalog data from the Advanced Camera for Surveys General Catalog and MICECATv2.0, respectively. We also incorporate "hostless" SNe residing in undetected faint hosts into our analysis, with an assumed hostless rate of 5%. Our fully automated algorithm is run on catalog data and matches SNe to their hosts with 91% accuracy. We find that including a machine learning component, run after the initial matching algorithm, improves the accuracy (purity) of the matching to 97% with a 2% cost in efficiency (true positive rate). Although the exact results are dependent on the details of the survey and the galaxy catalogs used, the method of identifying host galaxies we outline here can be applied to any transient survey