79 research outputs found
Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
We present a Fisher matrix forecast for the sensitivity on the mass of a
thermal warm dark matter (WDM) particle from current (DES-like) and future
(LSST-like) photometric galaxy surveys using the galaxy angular power spectrum.
We model the nonlinear clustering using a modified Halo Model proposed to
account for WDM effects. We estimate that from this observable alone a lower
bound of \,eV (\,eV) for the LSST (DES)
case could be obtained.Comment: 11 pages, 9 figure
DM particles: how warm they can be?
One of important questions concerning particles which compose the Dark Matter
(DM) is their average speed. We consider the model of relativistic weakly
interacting massive particles and try to impose an upper bound on their actual
and past warmness through the analysis of density perturbations and comparison
with the LSS data. It is assumed that the DM can be described by the recently
invented model of reduced relativistic gas (RRG). The equation of state of the
RRG model is closely reproducing the one of the Maxwell distribution, while
being much simpler. This advantage of the RRG model makes our analysis very
efficient. As a result we arrive at the rigid and model-independent bound for
the DM warmness without using the standard (much more sophisticated) approach
based on the Einstein-Boltzmann system of equations.Comment: 17 pages, 12 figures, improved version accepted for publication in
JCAP. Many discussions and clarifications, some figures and analysis adde
Large-scale analysis of the SDSS-III DR8 photometric luminous galaxies angular correlation function
We analyse the large-scale angular correlation function (ACF) of the CMASS
luminous galaxies (LGs), a photometric-redshift catalogue based on the Data
Release 8 (DR8) of the Sloan Digital Sky Survey-III. This catalogue contains
over LGs in the range , which was split
into four redshift shells of constant width. First, we estimate the constraints
on the redshift-space distortion (RSD) parameters and ,
where is the galaxy bias, the growth rate and is the
normalization of the perturbations, finding that they vary appreciably among
different redshift shells, in agreement with previous results using DR7 data.
When assuming constant RSD parameters over the survey redshift range, we obtain
, which agrees at the level with Baryon
Oscillation Spectroscopic Survey DR9 spectroscopic results. Next, we performed
two cosmological analyses, where relevant parameters not fitted were kept fixed
at their fiducial values. In the first analysis, we extracted the baryon
acoustic oscillation peak position for the four redshift shells, and combined
with the sound horizon scale from 7-year \textit{Wilkinson Microwave Anisotropy
Probe} to produce the constraints and
. In the second analysis, we used the ACF full shape
information to constrain cosmology using real data for the first time, finding
and .
These results are in good agreement with findings, showing that the ACF
can be efficiently applied to constrain cosmology in future photometric galaxy
surveys.Comment: MNRAS accepted. Minor corrections to match publish versio
The clustering of luminous red galaxies at z ∼ 0.7 from EBOSS and BOSS data
We present the first scientific results from the luminous red galaxy sample
(LRG) of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). We
measure the small and intermediate scale clustering from a sample of more than
61,000 galaxies in the redshift range . We interpret these
measurements in the framework of the Halo Occupation Distribution. The bias of
eBOSS LRGs is , with a satellite fraction of \% and a
mean halo mass of . These results are
consistent with expectations, demonstrating that eBOSS galaxies will be
reliable tracers of large scale structure at . The eBOSS galaxy bias
implies a scatter of luminosity at fixed halo mass, , of 0.19
dex. Using the clustering of massive galaxies from BOSS-CMASS, BOSS-LOWZ, and
SDSS, we find that is consistent with observations over
the full redshift range that these samples cover. The addition of eBOSS to
previous surveys allows investigation of the evolution of massive galaxies over
the past Gyr.Comment: 15 pages, 16 figures; changes following referee's comments; matches
the accepted versio
The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey
The Sloan Digital Sky Survey III (SDSS-III) presents the first spectroscopic
data from the Baryon Oscillation Spectroscopic Survey (BOSS). This ninth data
release (DR9) of the SDSS project includes 535,995 new galaxy spectra (median
z=0.52), 102,100 new quasar spectra (median z=2.32), and 90,897 new stellar
spectra, along with the data presented in previous data releases. These spectra
were obtained with the new BOSS spectrograph and were taken between 2009
December and 2011 July. In addition, the stellar parameters pipeline, which
determines radial velocities, surface temperatures, surface gravities, and
metallicities of stars, has been updated and refined with improvements in
temperature estimates for stars with T_eff<5000 K and in metallicity estimates
for stars with [Fe/H]>-0.5. DR9 includes new stellar parameters for all stars
presented in DR8, including stars from SDSS-I and II, as well as those observed
as part of the SDSS-III Sloan Extension for Galactic Understanding and
Exploration-2 (SEGUE-2).
The astrometry error introduced in the DR8 imaging catalogs has been
corrected in the DR9 data products. The next data release for SDSS-III will be
in Summer 2013, which will present the first data from the Apache Point
Observatory Galactic Evolution Experiment (APOGEE) along with another year of
data from BOSS, followed by the final SDSS-III data release in December 2014.Comment: 9 figures; 2 tables. Submitted to ApJS. DR9 is available at
http://www.sdss3.org/dr
ÉTICA EMPRESARIAL COMO BASE DE SUSTENTAÇÃO DO PROGRAMA DE COMPLIANCE: UMA BREVE ANÁLISE SOBRE A ÉTICA, A INTEGRIDADE E O COMPLIANCE.
O foco deste estudo é analisar os conceitos de ética empresarial, integridade e compliance com o objetivo de entender o significado desses institutos, a relação e as distinções entre eles, levando-se em consideração a legislação, os princípios e a experiência estadunidense e brasileira sobre o tema. Para tanto, complementa-se o estudo com um breve histórico da origem desses institutos. A metodologia de pesquisa adotada consiste nas investigações e observações históricas dos eventos mais relevantes. O trabalho orienta-se por uma análise crítica do Compliance Manual do Departamento de Justiça dos Estados Unidos da América, e da Lei no. 13.467/2017, e seus reflexos no ambiente econômico, social e empresarial. A pesquisa é qualitativa, de caráter exploratório, desenvolvida por meio de análise bibliográfica e documental. As fontes bibliográficas e documentais empregadas consistem na pesquisa de livros, revistas científicas, periódicos e artigos retirados da internet, bem como de legislação. A investigação é realizada por meio do método hipotético-dedutivo de abordagem, por intermédio de uma análise dogmática dos conceitos de ética empresarial, integridade e compliance. Como resultado da pesquisa, concluiu-se que, na essência, ética e compliance são lados diferentes da mesma moeda. Nesse prisma, compliance atém-se ao cumprimento da lei, enquanto a ética requer que seja feito o que é correto, independentemente do que reza a lei. O contexto ético é a base para o programa de compliance, considerando-se que a ética e a integridade dão sustentação e sentido ao programa de compliance. O sistema de compliance somente dará resultado se houver uma forte cultura ética. O estudo oferece como contribuição a análise sobre as duas teorias que dão base ao compliance, as teorias racionalista e normativa, bem como o esclarecimento sobre conceitos e definições que confundem muitos profissionais da área de compliance. PALAVRAS-CHAVE: ética empresarial; compliance; integridade; código de conduta; moral.
Early sedation and clinical outcomes of mechanically ventilated patients: a prospective multicenter cohort study
Introduction: Sedation overuse is frequent and possibly associated with poor outcomes in the intensive care unit (ICU) patients. However, the association of early oversedation with clinical outcomes has not been thoroughly evaluated. the aim of this study was to assess the association of early sedation strategies with outcomes of critically ill adult patients under mechanical ventilation (MV).Methods: A secondary analysis of a multicenter prospective cohort conducted in 45 Brazilian ICUs, including adult patients requiring ventilatory support and sedation in the first 48 hours of ICU admissions, was performed. Sedation depth was evaluated after 48 hours of MV. Multivariate analysis was used to identify variables associated with hospital mortality.Results: A total of 322 patients were evaluated. Overall, ICU and hospital mortality rates were 30.4% and 38.8%, respectively. Deep sedation was observed in 113 patients (35.1%). Longer duration of ventilatory support was observed (7 (4 to 10) versus 5 (3 to 9) days, P = 0.041) and more tracheostomies were performed in the deep sedation group (38.9% versus 22%, P=0.001) despite similar PaO2/FiO(2) ratios and acute respiratory distress syndrome (ARDS) severity. in a multivariate analysis, age (Odds Ratio (OR) 1.02; 95% confidence interval (CI) 1.00 to 1.03), Charlson Comorbidity Index >2 (OR 2.06; 95% Cl, 1.44 to 2.94), Simplified Acute Physiology Score 3 (SAPS 3) score (OR 1.02; Cl 95%, 1.00 to 1.04), severe ARDS (OR 1.44; Cl 95%, 1.09 to 1.91) and deep sedation (OR 2.36; Cl 9596, 1.31 to 4.25) were independently associated with increased hospital mortality.Conclusions: Early deep sedation is associated with adverse outcomes and constitutes an independent predictor of hospital mortality in mechanically ventilated patients.Research and Education Institute from Hospital Sirio-Libanes, São PauloD'Or Institute for Research and Education, Rio de Janeiro, BrazilBrazilian Research in Intensive Care NetworkHosp Copa DOr, BR-22031010 Rio de Janeiro, BrazilHosp Sirio Libanes, Res & Educ Inst, BR-01308060 São Paulo, BrazilUniv São Paulo, Fac Med, Hosp Clin, ICU,Emergency Med Dept, BR-05403000 São Paulo, BrazilHosp Sao Camilo Pompeia, ICU, BR-05022000 São Paulo, BrazilCEPETI, BR-82530200 Curitiba, Parana, BrazilHosp Canc I, Inst Nacl Canc, ICU, BR-20230130 Rio de Janeiro, BrazilPasteur Hosp, ICU, BR-20735040 Rio de Janeiro, BrazilIrmandade Santa Casa Misericordia Porto Alegre, RIPIMI, BR-90020090 Porto Alegre, RS, BrazilVitoria Apart Hosp, ICU, BR-29161900 Serra, ES, BrazilHosp Mater Dei, ICU, BR-30140093 Belo Horizonte, MG, BrazilHosp Santa Luzia, ICU, BR-70390902 Brasilia, DF, BrazilHosp Sao Luiz, ICU, BR-04544000 São Paulo, BrazilUniversidade Federal de São Paulo, Anesthesiol Pain & Intens Care Dept, ICU, BR-04024900 São Paulo, BrazilHosp Sao Jose Criciuma, ICU, BR-88801250 Criciuma, BrazilUDI Hosp, ICU, BR-65076820 Sao Luis, BrazilUniv São Paulo, Univ Hosp, ICU, BR-05508000 São Paulo, BrazilUniv São Paulo, Fac Med, Hosp Clin, ICU,Surg Emergency Dept, BR-05403000 São Paulo, BrazilIDOR DOr Inst Res & Educ, BR-22281100 Rio de Janeiro, BrazilInst Nacl Canc, Postgrad Program, BR-20230130 Rio de Janeiro, BrazilUniversidade Federal de São Paulo, Anesthesiol Pain & Intens Care Dept, ICU, BR-04024900 São Paulo, BrazilWeb of Scienc
Investigação epidemiológica e controle da Esquistossomose e demais parasitoses intestinais na Zona da Mata Mineira
-O presente trabalho avalia a cobertura e a qualidade do cadastro das famílias nos municípios mineiros de Coronel Pacheco, Goianá, e Piau, através
da comparação entre a ficha A aplicada pelo agente comunitário de saúde e os dados obtidos de investigações realizadas diretamente nos
domicílios. Foram entrevistadas, no período de novembro a dezembro de 2006, 192 famílias selecionadas de forma aleatória. A alta cobertura do
cadastro das famílias verificada (97,9%) assim como a fidedignidade para os campos “família corresponde ao endereço” e “família está completa”
(95,7% e 93,1%), observados nos três municípios, indicaram a confiabilidade do cadastro realizado pelo PSF. Os dados referentes à atualização das
gestantes, hipertensos, e crianças menores de um ano, não tiveram a mesma confiabilidade. Quanto ao perfil dos agentes comunitários de saúde,
que atuaram nos três municípios, a maioria dos entrevistados eram mulheres, com menos de 25 anos e estavam estudando ou já haviam completado
o segundo grau. O tempo médio de permanência dos profissionais no PSF foi de 10 meses, sendo que 45% dos agentes foram submetidos a
concurso municipal e os demais contratados. Os autores concluem que o cadastro do PSF (ficha A/SIAB) nos três municípios é confiável como base
populacional para o cálculo amostral, justificando sua utilização como ferramenta legítima para a realização de pesquisas de campo nas áreas
básicas e clínicas
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