ESTRUTURA POPULACIONAL E CONDIÇÃO FISIOLÓGICA DE Hoplias malabaricus (BLOCH, 1794) NO BAIXO RIO CAPIBARIBE

This research aimed to determine population structure and physiological condition of Hoplias malabaricus in the Capibaribe river (PE), northeastern Brazil. Monthly sampling were carried out between September/2013 and August/2014, using gill nets. The sex was identified by macroscopic and microscopic viewing of gonads, following the classification proposed by Vazzoler (1996). The specimens were distributed in length classes, being applied Kolmogorov-Smirnov test to evaluate the presence of sexual dimorphism. The length-weight relationship was calculated assessing differences through Kruskal Wallis test and physiological condition was calculated through allometric condition factor (K) between sexes, being applied the Spearman correlation test. Was collected 30 males and 42 females. No sexual dimorphism was observed relative to the size. Was observed positive allometric growth for females and negative for males. Was evidenced physiological condition variations along the year regarding seasonality. Population structure and physiological condition of the Hoplias malabaricus differed from that found in other environments, being this research, an important tool support the development of future management plans and conservation of Hoplias malabaricus, especially in this region.Keywords: population dynamics; fishing; reproduction.Esta pesquisa objetivou determinar a estrutura populacional e condição fisiológica de Hoplias malabaricus no rio Capibaribe (PE), nordeste brasileiro. Foram realizadas coletas mensais entre setembro/2013 e agosto/2014, utilizando redes de espera. O sexo foi identificado pela visualização macroscópica e microscópica das gônadas, seguindo a classificação proposta por Vazzoler (1996). Os indivíduos foram distribuídos entre classes de comprimento, sendo aplicado teste de Kolmogorov-Smirnov para verificar a presença de dimorfismo sexual. A relação peso-comprimento entre sexos foi calculada, avaliando diferenças pelo teste Kruskal-Wallis e a condição fisiológica foi avaliada pelo fator de condição alométrico (K) entre sexos, sendo aplicado teste de correlação de Spearman. Foram coletados 30 machos e 42 fêmeas, não sendo observado dimorfismo sexual relativo ao tamanho. Além disto, verificou-se um crescimento alométrico positivo para as fêmeas e negativo para os machos. Também foram evidenciadas variações na condição fisiológica ao longo do ano em relação à sazonalidade. A estrutura populacional e condição fisiológica de Hoplias malabaricus diferiram do encontrado em outros ambientes, sendo este estudo uma importante ferramenta para embasar o desenvolvimento de futuros planos de manejo e conservação de Hoplias malabaricus, especialmente nesta região.Palavras-chave: dinâmica populacional, pesca, manejo de recursos pesqueiros

The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III

The Sloan Digital Sky Survey (SDSS) started a new phase in August 2008, with new instrumentation and new surveys focused on Galactic structure and chemical evolution, measurements of the baryon oscillation feature in the clustering of galaxies and the quasar Ly alpha forest, and a radial velocity search for planets around ~8000 stars. This paper describes the first data release of SDSS-III (and the eighth counting from the beginning of the SDSS). The release includes five-band imaging of roughly 5200 deg^2 in the Southern Galactic Cap, bringing the total footprint of the SDSS imaging to 14,555 deg^2, or over a third of the Celestial Sphere. All the imaging data have been reprocessed with an improved sky-subtraction algorithm and a final, self-consistent photometric recalibration and flat-field determination. This release also includes all data from the second phase of the Sloan Extension for Galactic Understanding and Evolution (SEGUE-2), consisting of spectroscopy of approximately 118,000 stars at both high and low Galactic latitudes. All the more than half a million stellar spectra obtained with the SDSS spectrograph have been reprocessed through an improved stellar parameters pipeline, which has better determination of metallicity for high metallicity stars.Comment: Astrophysical Journal Supplements, in press (minor updates from submitted version

2 nd Brazilian Consensus on Chagas Disease, 2015

Abstract Chagas disease is a neglected chronic condition with a high burden of morbidity and mortality. It has considerable psychological, social, and economic impacts. The disease represents a significant public health issue in Brazil, with different regional patterns. This document presents the evidence that resulted in the Brazilian Consensus on Chagas Disease. The objective was to review and standardize strategies for diagnosis, treatment, prevention, and control of Chagas disease in the country, based on the available scientific evidence. The consensus is based on the articulation and strategic contribution of renowned Brazilian experts with knowledge and experience on various aspects of the disease. It is the result of a close collaboration between the Brazilian Society of Tropical Medicine and the Ministry of Health. It is hoped that this document will strengthen the development of integrated actions against Chagas disease in the country, focusing on epidemiology, management, comprehensive care (including families and communities), communication, information, education, and research

Erratum: “The eighth data release of the Sloan Digital Sky Survey: first data from SDSS-III” (2011, ApJS, 193, 29)

Section 3.5 of Aihara et al. (2011) described various sources of systematic error in the astrometry of the imaging data of the Sloan Digital Sky Survey (SDSS). In addition to these sources of error, there is an additional and more serious error, which introduces a large systematic shift in the astrometry over a large area around the north celestial pole. The region has irregular boundaries but in places extends as far south as declination δ ≈ 41◦. The sense of the shift is that the positions of all sources in the affected area are offset by roughly 250 mas in a northwest direction. We have updated the SDSS online documentation to reflect these errors, and to provide detailed quality information for each SDSS field

SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

Building on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars. In keeping with SDSS tradition, SDSS-III will provide regular public releases of all its data, beginning with SDSS DR8 (which occurred in Jan 2011). This paper presents an overview of the four SDSS-III surveys. BOSS will measure redshifts of 1.5 million massive galaxies and Lya forest spectra of 150,000 quasars, using the BAO feature of large scale structure to obtain percent-level determinations of the distance scale and Hubble expansion rate at z<0.7 and at z~2.5. SEGUE-2, which is now completed, measured medium-resolution (R=1800) optical spectra of 118,000 stars in a variety of target categories, probing chemical evolution, stellar kinematics and substructure, and the mass profile of the dark matter halo from the solar neighborhood to distances of 100 kpc. APOGEE will obtain high-resolution (R~30,000), high signal-to-noise (S/N>100 per resolution element), H-band (1.51-1.70 micron) spectra of 10^5 evolved, late-type stars, measuring separate abundances for ~15 elements per star and creating the first high-precision spectroscopic survey of all Galactic stellar populations (bulge, bar, disks, halo) with a uniform set of stellar tracers and spectral diagnostics. MARVELS will monitor radial velocities of more than 8000 FGK stars with the sensitivity and cadence (10-40 m/s, ~24 visits per star) needed to detect giant planets with periods up to two years, providing an unprecedented data set for understanding the formation and dynamical evolution of giant planet systems. (Abridged)Comment: Revised to version published in The Astronomical Journa

Environmentally friendly manufacturing of flexible graphite electrodes for a wearable device monitoring zinc in sweat

Electrochemical sensors based on graphite and polymers have emerged as powerful analytical tools for bioanalytical applications. However, most of the fabrication processes are not environmentally friendly because they often involve the use of toxic reagents and generate waste. This study describes an alternative method to produce flexible electrodes in plastic substrates using graphite powder and thermal laminating sheets by solid-solid deposition through hot compression, without the use of hazardous chemical reagents. The electrodes developed through the proposed approach have successfully demonstrated flexibility, robustness, reproducibility (relative standard deviation around 6%), and versatility. The electrodes were thoroughly characterized by cyclic voltammetry, electrochemical impedance spectroscopy, Raman spectroscopy, and scanning electron microscopy. As a proof of concept, the electrode surfaces were modified with bismuth and used for zinc analysis in sweat. The modified electrodes presented linearity (R-2 = 0.996) for a wide zinc concentration range (50-2000 ppb) and low detection limit (4.31 ppb). The proposed electrodes were tested using real sweat samples and the achieved zinc concentrations did not differ statistically from the data obtained by atomic absorption spectroscopy. To allow wearable applications, a 3D-printed device was fabricated, integrated with the proposed electrochemical system, and fixed at the abdomen by using an elastic tape to collect, store, and analyze the sweat sample. The matrix effect test was performed, spiking the real sample with different zinc levels, and the recovery values varied between 85 and 106%, thus demonstrating adequate accuracy and robustness of the flexible electrodes developed based on the proposed fabrication method11433948439492CONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICO - CNPQCOORDENAÇÃO DE APERFEIÇOAMENTO DE PESSOAL DE NÍVEL SUPERIOR - CAPESFUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULO - FAPESP426496/2018-3; 308140/2016-83359/2014; 3363/20142017/10522-5; 2018/08782-1This study was supported by CNPq (grants 426496/2018-3 and 308140/2016-8), CAPES (grants 3359/2014 and 3363/2014), INCTBio (grant 465389/2014-7), and FAPESP (grants 2017/10522-5 and 2018/08782-1)