Macracanthorhynchus hirudinaceus in a Sow in El Oro Province - Ecuador

Background: Macracantorhincosis is a zoonotic disease resulting from inadequate sanitary conditions, which occurs in pigs infected by acanthocephalic helminths called Macracanthorhynchus hirudinaceus. The eggs of these parasites are resistant to cold, high temperatures and can survive up to three years in the soil. They are consumed by dung beetles of the Scarabeidae family causing the parasite to evolve into its infective form, the cystacanth. The pig becomes infected after ingestion of either larvae or adult forms of these coleoptera. This paper describes a case report of macracantorhincosis found in a pig from the canton of Zaruma located in the province of El Oro, Ecuador. Case: A female pig, approximately 24 months old, weighing 30 kg, presented cachexia, muscle weakness, pale oral and ocular mucosa and a body temperature (rectal) above 39.4°C. The animal had a bulge on the ventral side of the neck, which evolved causing progressive discomfort to the point that the animal stopped eating. The pig was dewormed for three consecutive days. Fifteen days later, the animal had convulsions and muscle tremors, and died some hours after the symptoms started. During necropsy procedure, pale digestive tract membranes and nodules with fibrin were observed in the small intestine (jejunum), which was incised and the presence of parasites adhered to the granulomas detected. Two granulomas for morphological and histological studies and stool samples for coproparasitic test were collected. The collected parasites were fixed in a 10% buffered formalin solution, cross-sections were made and routinely processed for histological studies. The 5-μm-thick sections were stained using the hematoxylin and eosin (HE) technique. The parasite’s action involves perforation of the intestinal wall though its proboscis causing peritonitis and enteritis. Other conditions in intestinal dissection such as necrotic areas, inflammation of the submucosa and adult parasites adhered to the intestinal mucosa were also observed. The coproparasitic examination was performed using the flotation and sedimentation techniques. The coproparasitic test detected dark colored feces, semi-solid consistency and the presence of Macracanthorhynchus hirudinaceu eggs. In the histological evaluation of the cross section of the parasite, the presence of circular and longitudinal muscle fibers and lemniscus with their constrictor muscles was observed. Cuticle, hypodermis with tapered fibers and a large number of developing mature eggs were also reported.   Discussion: There is no pathognomonic symptomatology about this parasitosis, peritonitis can be generated by intestinal perforations. The findings at necropsy were ulcerations, inflammation in the small intestine and the presence of numerous nodules in the serous layer, where there was penetration of the parasite's proboscis. When fixed to the mucosa, these parasites cause ulcerations, inflammation and necrosis in the wall of the small intestine. The hypodermic layer is thicker than the muscular layer and the presence of leminis with their constricting muscles are typical features of acanthocephalus. It is considered appropriate to carry out epidemiological studies on the prevalence of the parasite Macracanthorhynchus hirudinaceus at pig farming system in the region, in order to determine the main risk factors. In Ecuador, cases of this disease in humans have not yet been reported, but have already been described in other countries, so the presence of this parasite in family swine farming may be considered a zoonotic-type risk factor. Keywords: pig, zoonotic disease, macrocanthorhincosis.  Título: Macracanthorhynchus hirudinaceus em uma porca da Província de El Oro - Equador. Descritores: suíno, doença zoonótica, macracantorrincose

Caracterização dos sistemas de produção de ovinos e caprinos na microrregião de Castanhal, Pará

O objetivo desse trabalho foi caracterizar os sistemas de produção de ovinos e caprinos na microrregião de Castanhal - Pará. Entre março de 2014 a maio de 2015 foram realizadas visitas a 60 propriedades criadoras de ovinos e caprinos da microrregião de Castanhal - PA, onde aplicou-se um questionário epidemiológico para obtenção de dados relacionados ao manejo produtivo, nutricional, sanitário e reprodutivo do rebanho, infraestrutura e gerenciamento das propriedades. O tipo de criação predominante era extensivo, com pastejo contínuo, com suplementação mineral somente em 46,6% das propriedades. Em 93,4% das propriedades o reprodutor era mantido junto com as fêmeas o ano inteiro, enquanto em apenas 3,4% utilizavam estação de monta e em 3,4% faziam monta controlada. As doenças relatadas como frequentes foram: parasitoses gastrointestinais (90%), afecções podais (80%), mortalidade de cordeiros (48,4%), linfadenite caseosa (31,7%), mastites (25%) e dermatite alérgica (20%). Também foram relatados abortos (10%), problemas respiratórios (6,7%), alterações nervosas (8,4%), ceratoconjuntivite (13,4%) e ectima contagioso (13,4%). A bovinocultura era a principal atividade desenvolvida pela maioria das propriedades do estudo e a ovinocaprinocultura secundária. Em 88,3% das propriedades não eram comercializados animais para o abate ou os reprodutores. Os resultados deste trabalho demonstraram que o nível de organização das criações de pequenos ruminantes era precário, sem utilização de técnicas de manejo e não possuíam assistência técnica, apresentando elevados índices de mortalidade, principalmente, pelas parasitoses gastrointestinais e problemas podais

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.Comment: Replaced with published version. Added journal reference and DO

Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI. Supplemental material in the ancillary file

Penilaian Kinerja Keuangan Koperasi di Kabupaten Pelalawan

This paper describe development and financial performance of cooperative in District Pelalawan among 2007 - 2008. Studies on primary and secondary cooperative in 12 sub-districts. Method in this stady use performance measuring of productivity, efficiency, growth, liquidity, and solvability of cooperative. Productivity of cooperative in Pelalawan was highly but efficiency still low. Profit and income were highly, even liquidity of cooperative very high, and solvability was good

Juxtaposing BTE and ATE – on the role of the European insurance industry in funding civil litigation

One of the ways in which legal services are financed, and indeed shaped, is through private insurance arrangement. Two contrasting types of legal expenses insurance contracts (LEI) seem to dominate in Europe: before the event (BTE) and after the event (ATE) legal expenses insurance. Notwithstanding institutional differences between different legal systems, BTE and ATE insurance arrangements may be instrumental if government policy is geared towards strengthening a market-oriented system of financing access to justice for individuals and business. At the same time, emphasizing the role of a private industry as a keeper of the gates to justice raises issues of accountability and transparency, not readily reconcilable with demands of competition. Moreover, multiple actors (clients, lawyers, courts, insurers) are involved, causing behavioural dynamics which are not easily predicted or influenced. Against this background, this paper looks into BTE and ATE arrangements by analysing the particularities of BTE and ATE arrangements currently available in some European jurisdictions and by painting a picture of their respective markets and legal contexts. This allows for some reflection on the performance of BTE and ATE providers as both financiers and keepers. Two issues emerge from the analysis that are worthy of some further reflection. Firstly, there is the problematic long-term sustainability of some ATE products. Secondly, the challenges faced by policymakers that would like to nudge consumers into voluntarily taking out BTE LEI

Search for stop and higgsino production using diphoton Higgs boson decays

Results are presented of a search for a "natural" supersymmetry scenario with gauge mediated symmetry breaking. It is assumed that only the supersymmetric partners of the top-quark (stop) and the Higgs boson (higgsino) are accessible. Events are examined in which there are two photons forming a Higgs boson candidate, and at least two b-quark jets. In 19.7 inverse femtobarns of proton-proton collision data at sqrt(s) = 8 TeV, recorded in the CMS experiment, no evidence of a signal is found and lower limits at the 95% confidence level are set, excluding the stop mass below 360 to 410 GeV, depending on the higgsino mass

Differential cross section measurements for the production of a W boson in association with jets in proton–proton collisions at √s = 7 TeV

Measurements are reported of differential cross sections for the production of a W boson, which decays into a muon and a neutrino, in association with jets, as a function of several variables, including the transverse momenta (pT) and pseudorapidities of the four leading jets, the scalar sum of jet transverse momenta (HT), and the difference in azimuthal angle between the directions of each jet and the muon. The data sample of pp collisions at a centre-of-mass energy of 7 TeV was collected with the CMS detector at the LHC and corresponds to an integrated luminosity of 5.0 fb[superscript −1]. The measured cross sections are compared to predictions from Monte Carlo generators, MadGraph + pythia and sherpa, and to next-to-leading-order calculations from BlackHat + sherpa. The differential cross sections are found to be in agreement with the predictions, apart from the pT distributions of the leading jets at high pT values, the distributions of the HT at high-HT and low jet multiplicity, and the distribution of the difference in azimuthal angle between the leading jet and the muon at low values.United States. Dept. of EnergyNational Science Foundation (U.S.)Alfred P. Sloan Foundatio