Characterisation of an aperture-stacked patch antenna for ultra-wideband wearable radio systems

This paper presents, for the first time, the time-domain characteristics of an aperture-stacked patch antenna (ASPA) for ultra-wideband (UWB) wearable devices. The methodology of antennas characterization for UWB radio systems is also outlined. The antenna operates within the 3-6 GHz frequency band. Time- and frequency-domain characteristics of this antenna are presented in transmission mode (Tx), receiving mode (Rx) and for 2-antenna (Tx-Rx) system. The pulse driving the antenna has duration of 0.65 ns. In the Tx mode, pulses radiated in different directions of the H-plane have very similar shapes. Fidelity factors are as high as 91.6-99.9%. For 2-antenna system, pulses received in normal and end-fire-like directions have the fidelity of 69.5%. As it was found, antenna does not behave "reciprocal" comparing Tx and Rx modes. For normal propagation direction, radiated pulse is the 2nd derivative of the input waveform, but in the Rx mode, received pulse is the 1st derivative of the incident plane wave. This antenna can be used for transmission of short-pulses, even 0.65-1 ns in duration. It is also small (patch planar dimensions 32/19 mm) and compact. Microstrip configuration allows further integration of active devices on the same board. Taking into account above results we can say that ASPA is a good candidate for UWB non-invasive wireless body area network (WBAN) applications

Flexible CMOS electronics based on p-type Ge₂Sb₂Te₅ and n-type InGaZnO₄ semiconductors

Ultra-thin p-type chalcogenide glass Ge2Sb2Te5 (GST) semiconductor layers are employed to form flexible thin-film transistors (TFTs). For the first time, TFTs based on GST show saturating output characteristics and an ON/OFF ratio up to 388, exceeding present reports by a factor of ~20. The channel current modulation is greatly enhanced by using ultra-thin 5 nm thick amorphous GST layers and 20 nm thick high-k Al2O3 gate dielectrics. Flexible CMOS circuits are realized in combination with the n-type oxide semiconductor InGaZnO4 (IGZO). The CMOS inverters show voltage gain of up to 69. Furthermore, flexible NAND gates are presented. The bending stability is shown for a tensile radius of 6 mm

Flexible In-Ga-Zn-O based circuits with two and three metal layers: simulation and fabrication study

The quest for high-performance flexible circuits call for scaling of the minimum feature size in Thin-Film Transistors (TFTs). Although reduced channel lengths can guarantee an improvement in the electrical properties of the devices, proper design rules also play a crucial role to minimize parasitics when designing fast circuits. In this letter, systematic Computer-Aided Design (CAD) simulations have guided the fabrication of highperformance flexible operational amplifiers (opamps) and logic circuits based on Indium-Gallium-Zinc-Oxide (IGZO) TFTs. In particular, the performance improvements due to the use of an additional third metal layer for the interconnections has been estimated for the first time. Encouraged by the simulated enhancements resulting by the decreased parasitic resistances and capacitances, both TFTs and circuits have been realized on a free-standing 50μm thick polymide foil using three metal layers. Despite the thicker layer stack, the TFTs have shown mechanical stability down to 5mm bending radii. Moreover, the opamps and the logic circuits have yielded improved electrical performance with respect to the architecture with two metal layers: gainbandwidth- product (GBWP) increased by 16:9%, for the first one, and propagation delay (tpd) decreased by 43%, for the latter one

Optimization of inertial micropower generators for human walking motion

Published versio

Availability of pediatric and neonatal intensive care units in the city of São Paulo

OBJECTIVE: To describe the health care service provided in pediatric intensive care units in the city of São Paulo, by identifying and describing the units and analyzing their geographic distribution. METHODS: A descriptive cross-sectional study was carried out during a two-year period (August 2000 to July 2002). Data were collected through questionnaires answered by medical directors of each pediatric and neonatal intensive care unit. RESULTS: São Paulo is served by 107 pediatric and neonatal intensive care units, of which 85 (79.4%) completed and returned the questionnaire. We found a very unequal distribution of units as there were more units in places with the least pediatric population. Regarding to pediatric intensive care units specialization, 7% were pediatric, 41.2% were neonatal and 51.7% were mixed (pediatric and neonatal). Regarding hospital funds, 15.3% were associated with philanthropic institutions, 37.6% were private and 47% were public. A total of 1,067 beds were identified, of which 969 were active. The ratio bed/patient aged 0-14 was 1/2,728, varying from 1/604 at health districts - I to 1/6,812 at health districts - III. The units reported an average of 11.7 beds (2 to 60). The neonatal intensive care unit had a median of 16.9 beds per unit and pediatric intensive care units a median of 8.5 beds/unit. CONCLUSION: In São Paulo, we found an uneven distribution of pediatric and neonatal intensive care units among the health districts. There was also an uneven distribution between public and private units, and neonatal and pediatric ones. The current report is the first step in the effort to improve the quality of medical assistance in pediatric and neonatal intensive care units in São Paulo.OBJETIVO: Caracterizar a assistência de saúde prestada em tratamento intensivo pediátrico e neonatal no município de São Paulo através da identificação, descrição e distribuição geográfica das unidades. MÉTODOS: Estudo descritivo, tipo transversal, onde foram estudadas as unidades de terapia intensiva pediátrica e neonatal do município de São Paulo, no período de agosto de 2000 a julho de 2002. A coleta dos dados foi realizada por meio de questionário preenchido pelo coordenador médico de cada unidade. RESULTADOS: Foram listadas 107 unidades de terapia intensiva pediátricas e neonatais no município de São Paulo. Oitenta e cinco (79,4%) unidades forneceram os dados, constituindo a população de estudo. Observou-se maior número de unidades de terapia intensiva em Núcleos Regionais de Saúde com menor população pediátrica. Quanto à faixa etária, 7% eram exclusivamente pediátricas, 41,2% neonatais, e 51,7% mistas. Em relação ao mantenedor: 47% eram públicas, 37,6% privadas, e 15,3% filantrópicas. Identificamos 1.067 leitos, estando 969 em atividade. A razão leito/paciente de 0 a 14 anos foi de 1:2.728, variando de 1:604 (Núcleo Regional de Saúde - I) a 1:6.812 (Núcleo Regional de Saúde - III). O número de leitos por unidade variou de 2 a 60, com média de 11,7 (unidades de terapia intensiva neonatais: 16,9; mistas: 8,5). CONCLUSÃO: No município de São Paulo, observou-se uma distribuição desproporcional das unidades de terapia intensiva pediátrica e neonatal entre os cinco Núcleos Regionais de Saúde. Houve também uma distribuição desproporcional entre unidades de terapia intensiva públicas e privadas e entre neonatais e pediátricas. Esse estudo foi o primeiro esforço na busca por melhor qualidade na assistência intensiva pediátrica e neonatal no município de São Paulo.Universidade de São Paulo Faculdade de MedicinaUniversidade Federal de São Paulo (UNIFESP) Departamento de PediatriaUniversidade de São Paulo Hospital Universitário Unidade de Terapia Intensiva PediátricaUNIFESP, Depto. de PediatriaSciEL

Adverse drug events in a paediatric intensive care unit: a prospective cohort

Objectives: To describe adverse drug events (ADEs) in children under intensive care, identify risk factors and tools that can detect ADEs early, and the impact on length of stay (LOS).Design: A prospective observational study.Setting: Paediatric intensive care unit of a tertiary care teaching hospital.Patients: 239 patients with a mean age of 67.5 months representing 1818 days of hospitalisation in intensive care unit.Interventions: Active search of charts and electronic patient records using triggers. the statistical analysis involved linear and logistic regression.Measurements and main results: the average LOS was 7.6 days. There were 110 proven, probable and possible ADEs in 84 patients (35.1%). We observed 138 instances of triggers. the major classes of drugs associated with events were: antibiotics (n=41), diuretics (n=24), antiseizures (n=23), sedatives and analgesics (n=17) and steroids (n=18). the number of drugs administered was most related to the occurrence of ADEs and also to the LOS (p<0.001). the occurrence of an ADE may result in an increase in the LOS by 1.5 days per event, but this was not statistically significant in this sample. Patients aged less than 48 months also proved to be at a significant risk for ADEs, with an OR of 1.84 (95% CI 1.07 to 3.15, p=0.025). the number of drugs administered also correlated with the number of ADEs (p<0.0001). the chance of having at least one ADE increased linearly as the patient was administered more drugs.Conclusions: the use of multiple drugs as well as lower patient age favours the occurrence of ADEs. the active search described here provides a systematic approach to this problem.Univ São Paulo, Fac Med, Inst Crianca, FMUSP, São Paulo, BrazilUniversidade Federal de São Paulo, Pediat Oncol Inst GRAACC IOP, São Paulo, BrazilUniversidade Federal de São Paulo, Pediat Oncol Inst GRAACC IOP, São Paulo, BrazilWeb of Scienc

A robust test for monotonicity in asset returns

[eng] In this paper, we propose a robust test of monotonicity in asset returns that is valid under a general setting. We develop a test that allows for dependent data and is robust to conditional heteroskedasticity or heavy-tailed distributions of return differentials. Many postulated theories in economics and finance assume monotonic relationships between expected asset returns and certain underlying characteristics of an asset. Existing tests in literature fail to control the probability of a type 1 error or have low power under heavy-tailed distributions of return differentials. Monte Carlo simulations illustrate that our test statistic has a correct empirical size under all data-generating processes together with a similar power to other tests. Conversely, alternative tests are non-conservative under conditional heteroskedasticity or heavy-tailed distributions of return differentials. We also present an empirical application on the monotonicity of returns on various portfolios sorts that highlights the usefulness of our approach

An analysis of galaxy cluster mis-centring using cosmological hydrodynamic simulations

The location of a galaxy cluster’s centroid is typically derived from observations of the galactic and/or gas component of the cluster, but these typically deviate from the true centre. This can produce bias when observations are combined to study average cluster properties. Using data from the BAryons and HAloes of MAssive Systems (BAHAMAS) cosmological hydrodynamic simulations, we study this bias in both two and three dimensions for 2000 clusters over the 1013–1015 M⊙ mass range. We quantify and model the offset distributions between observationally motivated centres and the ‘true’ centre of the cluster, which is taken to be the most gravitationally bound particle measured in the simulation. We fit the cumulative distribution function of offsets with an exponential distribution and a Gamma distribution fit well with most of the centroid definitions. The galaxy-based centres can be seen to be divided into a mis-centred group and a well-centred group, with the well-centred group making up about 60 per cent of all the clusters. Gas-based centres are overall less scattered than galaxy-based centres. We also find a cluster-mass dependence of the offset distribution of gas-based centres, with generally larger offsets for smaller mass clusters. We then measure cluster density profiles centred at each choice of the centres and fit them with empirical models. Stacked, mis-centred density profiles fit to the Navarro–Frenk–White dark matter profile and Komatsu–Seljak gas profile show that recovered shape and size parameters can significantly deviate from the true values. For the galaxy-based centres, this can lead to cluster masses being underestimated by up to 10 per cent⁠