Parameters influencing the size of chitosan-TPP nano- and microparticles

Chitosan nanoparticles, produced by ionic gelation, are among the most intensely studied nanosystems for drug delivery. However, a lack of inter-laboratory reproducibility and a poor physicochemical understanding of the process of particle formation have been slowing their potential market applications. To address these shortcomings, the current study presents a systematic analysis of the main polymer factors affecting the nanoparticle formation driven by an initial screening using systematic statistical Design of Experiments (DoE). In summary, we found that for a given chitosan to TPP molar ratio, the average hydrodynamic diameter of the particles formed is strongly dependent on the initial chitosan concentration. The degree of acetylation of the chitosan was found to be the second most important factor involved in the system's ability to form particles. Interestingly, viscosimetry studies indicated that the particle formation and the average hydrodynamic diameter of the particles formed were highly dependent on the presence or absence of salts in the medium. In conclusion, we found that by controlling two simple factors of the polymer solution, namely its initial concentration and its solvent environment, it is feasible to control in a reproducible manner the production and characteristics of chitosan particles ranging in size from nano- to micrometres

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

Periastron Observations of TeV Gamma-Ray Emission from a Binary System with a 50-year Period

We report on observations of the pulsar/Be star binary system PSR J2032+4127/MT91 213 in the energy range between 100 GeV and 20 TeV with the Very Energetic Radiation Imaging Telescope Array and Major Atmospheric Gamma Imaging Cherenkov telescope arrays. The binary orbit has a period of approximately 50 years, with the most recent periastron occurring on 2017 November 13. Our observations span from 18 months prior to periastron to one month after. A new point-like gamma-ray source is detected, coincident with the location of PSR J2032+4127/MT91 213. The gamma-ray light curve and spectrum are well characterized over the periastron passage. The flux is variable over at least an order of magnitude, peaking at periastron, thus providing a firm association of the TeV source with the pulsar/Be star system. Observations prior to periastron show a cutoff in the spectrum at an energy around 0.5 TeV. This result adds a new member to the small population of known TeV binaries, and it identifies only the second source of this class in which the nature and properties of the compact object are firmly established. We compare the gamma-ray results with the light curve measured with the X-ray Telescope on board the Neil Gehrels Swift Observatory and with the predictions of recent theoretical models of the system. We conclude that significant revision of the models is required to explain the details of the emission that we have observed, and we discuss the relationship between the binary system and the overlapping steady extended source, TeV J2032+4130

Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

Aims. We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1, which includes, among other instruments, MAGIC, VERITAS, Whipple 10 m, and Fermi-LAT to cover the gamma-ray range from 0.1 GeV to 20 TeV; RXTE and Swift to cover wavelengths from UV to hard X-rays; and GASP-WEBT, which provides coverage of radio and optical wavelengths. Optical polarization measurements were provided for a fraction of the campaign by the Steward and St. Petersburg observatories. We evaluate the variability of the source and interband correlations, the gamma-ray flaring activity occurring in May 2009, and interpret the results within two synchrotron self-Compton (SSC) scenarios.Methods. The multiband variability observed during the full campaign is addressed in terms of the fractional variability, and the possible correlations are studied by calculating the discrete correlation function for each pair of energy bands where the significance was evaluated with dedicated Monte Carlo simulations. The space of SSC model parameters is probed following a dedicated grid-scan strategy, allowing for a wide range of models to be tested and offering a study of the degeneracy of model-to-data agreement in the individual model parameters, hence providing a less biased interpretation than the "single-curve SSC model adjustment" typically reported in the literature.Results. We find an increase in the fractional variability with energy, while no significant interband correlations of flux changes are found on the basis of the acquired data set. The SSC model grid-scan shows that the flaring activity around May 22 cannot be modeled adequately with a one-zone SSC scenario (using an electron energy distribution with two breaks), while it can be suitably described within a two (independent) zone SSC scenario. Here, one zone is responsible for the quiescent emission from the averaged 4.5-month observing period, while the other one, which is spatially separated from the first, dominates the flaring emission occurring at X-rays and very-high-energy (> 100 GeV, VHE) gamma-rays. The flaring activity from May 1, which coincides with a rotation of the electric vector polarization angle (EVPA), cannot be satisfactorily reproduced by either a one-zone or a two-independent-zone SSC model, yet this is partially affected by the lack of strictly simultaneous observations and the presence of large flux changes on sub-hour timescales (detected at VHE gamma rays).Conclusions. The higher variability in the VHE emission and lack of correlation with the X-ray emission indicate that, at least during the 4.5-month observing campaign in 2009, the highest energy (and most variable) electrons that are responsible for the VHE gamma rays do not make a dominant contribution to the similar to 1 keV emission. Alternatively, there could be a very variable component contributing to the VHE gamma-ray emission in addition to that coming from the SSC scenario. The studies with our dedicated SSC grid-scan show that there is some degeneracy in both the one-zone and the two-zone SSC scenarios probed, with several combinations of model parameters yielding a similar model-to-data agreement, and some parameters better constrained than others. The observed gamma-ray flaring activity, with the EVPA rotation coincident with the first gamma-ray flare, resembles those reported previously for low frequency peaked blazars, hence suggesting that there are many similarities in the flaring mechanisms of blazars with different jet properties

Estado nutricional de gestantes avaliado por três diferentes métodos de classificação antropométrica Nutritional status of pregnant women according to three different anthropometric classification methods

OBJETIVO: Avaliar o estado nutricional de gestantes por três diferentes métodos. MÉTODOS: Estudo de corte transversal, realizado entre janeiro e junho de 2006, com 992 gestantes de um serviço público. O estado nutricional foi classificado por diferentes métodos de avaliação: nomograma de Rosso, método de Atalah e gestograma do Centro Latino Americano de Perinatologia. Os resultados foram comparados com o estado nutricional de mulheres não gestantes em idade reprodutiva da Região Nordeste e do Brasil. As diferenças foram analisadas pelo teste qui-quadrado de bondade de ajuste, adotando-se o nível de significância de 5%. RESULTADOS: O baixo peso gravídico avaliado pelo nomograma de Rosso foi a condição que mais contribuiu para a diferença encontrada (p<0,001). Pelo método de Atalah, as diferenças extremas também foram observadas nas prevalências de baixo peso gravídico tanto no grupo de mulheres da Região Nordeste quanto do Brasil. Em relação ao gestograma do Centro Latino Americano de Perinatologia, os maiores diferenciais de prevalência também ocorreram na condição de baixo peso: 18% versus 7,4% para a Região Nordeste e 18% versus 6,7% para o Brasil, embora tenha sido o método de avaliação que mais se aproximou dos resultados da população de comparação. CONCLUSÃO: A distribuição do estado nutricional, avaliado pelos três métodos, foi diferente da distribuição nutricional da população de não gestantes tanto em nível regional quanto em nível nacional, particularmente o Nomograma de Rosso, demonstrando utilidade limitada desses instrumentos. A avaliação pelo Centro Latino Americano de Perinatologia é a que menos se distancia da situação encontrada para não gestantes.<br>OBJECTIVE: This study assessed the nutritional status of pregnant women by three different methods. METHODS: A cross sectional study was conducted between January and June 2006 with 992 pregnant women attending a public prenatal care facility. Nutritional status was classified according to different assessment methods (Rosso nomogram, Atalah method and the Latin American Center for Perinatology gestogram). The results were compared with the nutritional status of nonpregnant women in childbearing age in the Brazilian Northeast and all of Brazil. The differences were analyzed by the chi-square goodness of fit test, with a significance level of 5%. RESULTS: Low weight of pregnant women according to the Rosso nomogram was the condition that most contributed to the difference (p<0.001). According to the Atalah method, extreme differences were also observed in the prevalences of underweight pregnant women both in the Northeast and in all of Brazil. In relation to the gestogram of the Perinatology Latin American Center, the greatest prevalence differences also occurred among the underweight: 18% versus 7.4% for the Northeast Region and 18% versus 6.7% for Brazil, although this was the assessment method that came closest to the results of the population being compared. CONCLUSION: Nutritional status distribution of pregnant women, assessed by three methods, was different from the nutritional status distribution of the nonpregnant population, both regionally and domestically, especially according to Rosso's nomogram, demonstrating the limited use of these instruments. Assessment by the Perinatology Latin American Center comes closest to the nutritional status distribution of nonpregnant women