Urinary Estrogen Metabolites and Self-Reported Infertility in Women Infected with Schistosoma haematobium

Schistosomiasis is a neglected tropical disease, endemic in 76 countries, that afflicts more than 240 million people. The impact of schistosomiasis on infertility may be underestimated according to recent literature. Extracts of Schistosoma haematobium include estrogen-like metabolites termed catechol-estrogens that down regulate estrogen receptors alpha and beta in estrogen responsive cells. In addition, schistosome derived catechol-estrogens induce genotoxicity that result in estrogen-DNA adducts. These catechol estrogens and the catechol-estrogen-DNA adducts can be isolated from sera of people infected with S. haematobium. The aim of this study was to study infertility in females infected with S. haematobium and its association with the presence of schistosome-derived catechol-estrogens

Distribuição volumétrica de calda contendo Metarhizium anisopliae

O controle microbiano de Mahanarva fimbriolata é de suma importância para o manejo dessa praga em cana-de-açúcar, porém carece de melhorias quanto à tecnologia de aplicação. O trabalho teve como objetivo definir um modelo de bico de pulverização adequado para o controle de M. fimbriolata, com base no padrão de distribuição de calda aspergida e espaçamento entre bicos. Utilizaram-se os bicos TF4, TTI e AIUB11004VS e caldas a base de fungo Metarhizium anisopliae sem adjuvante e com Agral a 2% e 4%. Avaliou-se o espaçamento entre bicos baseado na construção de curvas de deposição, considerando CV máximo de 10%; ângulo de abertura e vazão dos bicos. Os maiores espaçamentos foram de 85cm em calda com 2% de adjuvante para o bico TF4, 70cm para AIUB11004VS sem adição de adjuvante e 55cm para o bico TTI, independente da calda. Em relação ao ângulo de abertura, houve apenas diferença entre os bicos testados em uma mesma calda. A vazão foi maior para a calda com 4% de adjuvante para os bicos TF4 e TTI, sendo que AIUB11004VS apresentou menores vazões em relação aos outros modelos para calda com 2% e 4% de adjuvante. Conclui-se que o modelo AIUB11004VS é uma importante ferramenta operacional, visando o controle de M. fimbriolata, por apresentar menor consumo de calda e bons resultados de distância entre bicos.The microbial control of Mahanarva fimbriolata is very important to management of this pest in sugarcane crops, however lacks improvement in spraying technology. The work aimed to evaluate a nozzle model adequate to control M. fimbriolata, based on pattern of spray distribution and the space between nozzles. TF4, TTI and AIUB11004VS nozzles containing the fungus Metarhizium anisopliae without adjuvant, with Agral 2% and 4% were used in the assay. We evaluated spacing between nozzles by constructing deposition curves considering maximum CV of 10%, spray angle and nozzle flow for different sprays. The larger nozzle spacings were 85cm for spray with 2% of adjuvant and TF4 nozzle, 70cm for AIUB11004VS without adjuvant addition and 55cm TTI nozzle, independent of spray used. Despite the spray angle, we observed difference between the nozzles to the same spray. The flow was larger for spray with adjuvant at 4%, to TF4 and TTI, while AIUB11004VS showed minor flows when compared to the others nozzles using 2% and 4% of adjuvant. By presenting good results of distance between nozzles and minor spray consumption, AIUB11004VS is a good tool for control of M. fimbriolata.Univ Estadual Paulista, UNESP, Dept Fitossanidade, BR-14884900 Jaboticabal, SP, BrazilSuporte Tecn Usina Sao Martinho SA, Pradopolis, SP, BrazilUniv Estadual Paulista, UNESP, Dept Fitossanidade, BR-14884900 Jaboticabal, SP, Brazi

Faint objects in motion: the new frontier of high precision astrometry

Sky survey telescopes and powerful targeted telescopes play complementary roles in astronomy. In order to investigate the nature and characteristics of the motions of very faint objects, a flexibly-pointed instrument capable of high astrometric accuracy is an ideal complement to current astrometric surveys and a unique tool for precision astrophysics. Such a space-based mission will push the frontier of precision astrometry from evidence of Earth-mass habitable worlds around the nearest stars, to distant Milky Way objects, and out to the Local Group of galaxies. As we enter the era of the James Webb Space Telescope and the new ground-based, adaptive-optics-enabled giant telescopes, by obtaining these high precision measurements on key objects that Gaia could not reach, a mission that focuses on high precision astrometry science can consolidate our theoretical understanding of the local Universe, enable extrapolation of physical processes to remote redshifts, and derive a much more consistent picture of cosmological evolution and the likely fate of our cosmos. Already several missions have been proposed to address the science case of faint objects in motion using high precision astrometry missions: NEAT proposed for the ESA M3 opportunity, micro-NEAT for the S1 opportunity, and Theia for the M4 and M5 opportunities. Additional new mission configurations adapted with technological innovations could be envisioned to pursue accurate measurements of these extremely small motions. The goal of this White Paper is to address the fundamental science questions that are at stake when we focus on the motions of faint sky objects and to briefly review instrumentation and mission profiles

NEOTROPICAL XENARTHRANS: a data set of occurrence of xenarthran species in the Neotropics

Xenarthrans – anteaters, sloths, and armadillos – have essential functions for ecosystem maintenance, such as insect control and nutrient cycling, playing key roles as ecosystem engineers. Because of habitat loss and fragmentation, hunting pressure, and conflicts with 24 domestic dogs, these species have been threatened locally, regionally, or even across their full distribution ranges. The Neotropics harbor 21 species of armadillos, ten anteaters, and six sloths. Our dataset includes the families Chlamyphoridae (13), Dasypodidae (7), Myrmecophagidae (3), Bradypodidae (4), and Megalonychidae (2). We have no occurrence data on Dasypus pilosus (Dasypodidae). Regarding Cyclopedidae, until recently, only one species was recognized, but new genetic studies have revealed that the group is represented by seven species. In this data-paper, we compiled a total of 42,528 records of 31 species, represented by occurrence and quantitative data, totaling 24,847 unique georeferenced records. The geographic range is from the south of the USA, Mexico, and Caribbean countries at the northern portion of the Neotropics, to its austral distribution in Argentina, Paraguay, Chile, and Uruguay. Regarding anteaters, Myrmecophaga tridactyla has the most records (n=5,941), and Cyclopes sp. has the fewest (n=240). The armadillo species with the most data is Dasypus novemcinctus (n=11,588), and the least recorded for Calyptophractus retusus (n=33). With regards to sloth species, Bradypus variegatus has the most records (n=962), and Bradypus pygmaeus has the fewest (n=12). Our main objective with Neotropical Xenarthrans is to make occurrence and quantitative data available to facilitate more ecological research, particularly if we integrate the xenarthran data with other datasets of Neotropical Series which will become available very soon (i.e. Neotropical Carnivores, Neotropical Invasive Mammals, and Neotropical Hunters and Dogs). Therefore, studies on trophic cascades, hunting pressure, habitat loss, fragmentation effects, species invasion, and climate change effects will be possible with the Neotropical Xenarthrans dataset