ARES+MOOG - a practical overview of an EW method to derive stellar parameters

The goal of this document is to describe the important practical aspects in the use of an Equivalent Width (EW) method for the derivation of spectroscopic stellar parameters. A general description of the fundamental steps composing any EW method is given, together with possible differences that may be found in different methods used in the literature. Then ARES+MOOG is then used as an example where each step of the method is described in detail. A special focus is given for the specific steps of this method, namely the use of a differential analysis to define the atomic data for the adopted line list, the automatic EW determinations, and the way to find the best parameters at the end of the procedure. Finally, a practical tutorial is given, where we focus on simple exercises useful to illustrate and explain the dependence of the abundances with the assumed stellar parameters. The interdependences are described and a clear procedure is given to find the "final" stellar parameters.Comment: 15 pages, 4 figures, accepted for publication as a chapter in "Determination of Atmospheric Parameters of B, A, F and G Type Stars", Springer (2014), eds. E. Niemczura, B. Smalley, W. Pyc

Contributions to the Portuguese National Plan for Patient Safety 2021–2026: A Robust Methodology Based on the Mixed-Method Approach

Introduction: Several countries prioritize patient safety in their health policies. In Portugal, following the implementation of the National Plan for Patient Safety (NPPS) 2015– 2020, the research team of the National School of Public Health (NSPH) carried out extensive work to continue improving aspects of the previous Plan. This work was focused on identifying the strengths and weaknesses of NPPS 2015– 2020 and aspects related to its applicability and main challenges and opportunities for the implementation of the NPPS 2021–2026. Methods: Methodological dynamic process was based on the most relevant international and national guidelines and the feedback from key patient safety stakeholders. We developed a cross-sectional mixed-methods study from January to August 2021. We used documentation and periodical reports from National Health Service (NHS) healthcare institutions as secondary sources of information. For primary data collection, we used an online survey (applied to elements in the different quality and safety structures of hospitals and primary care units), interviews, and focus groups to collect information from patient safety experts. Results and Discussion: Strengthening safety culture, patient safety training, communication, leadership involvement, patient and family engagement, and monitorization process is considered essential. We also identified local limitations such as the lack of resources and protected time for the healthcare professionals and lack of leadership involvement on patient safety strategies for dedicating to patient safety actions. Most of the patient safety stakeholders agreed that the safety and health of clinical teams and new modalities of healthcare (such as telemedicine, home hospitalization, home care) should be a priority for patient safety strategies. Conclusions: In our study, we used a robust methodology with a participatory process involving different stakeholders. An alignment between local, regional, and national levels in terms of measuring indicators, the definition of priorities, and actions and activities to improve patient safety is recommended. Reinforced partnerships and alignment between the institution’s mission, and safety priorities will be crucial to enhance patient safety. Additionally, this work highlights the added value for health systems achieved through strong partnerships between public administration and academic institutions to improve healthcare quality and patient safetyinfo:eu-repo/semantics/publishedVersio

Variations in multiple sclerosis practice within Europe - Is it time for a new treatment guideline?

In the past 5 years, the combination of developments in diagnostic strategy and approval of new disease-modifying therapies has provided an opportunity to achieve dramatic improvements in patient outcomes in multiple sclerosis (MS). However, across Europe there are several factors that may prevent patients from receiving the best therapy at the appropriate time, and there is variation among countries in terms of which of these factors are most relevant. Here, we review current MS clinical practices in a number of countries in the European Union to identify differences regarding initiation of treatment in patients with clinically isolated syndrome or relapsing-remitting MS, and differences in the timing of treatment switch or escalation. While recognizing that policy is not static in any country, we believe that patients' interests would be better served if a European treatment guideline was developed. Such a guideline could both inform and be informed by national policies, facilitating the dissemination of best clinical practice internationally.info:eu-repo/semantics/publishedVersio

Immunomodulatory properties of Musa paradisiaca L. inflorescence in Combined Allergic Rhinitis and Asthma Syndrome (CARAS) model towards NFκB pathway inhibition

Musa paradisiaca L. (Musaceae), a tropical plant named banana is used as food and as medicine in Brazil. Banana inflorescence, popularly known as mangará, presents several biological activities including anti-inflammatory effects. Here, we demonstrated the immunomodulatory activity of banana inflorescence extract (HEM) on a mice model of combined allergic rhinitis and asthma syndrome (CARAS) and in human macrophages. The HEM inhibited the eosinophil migration, production of cytokines as IL-4, IL-5, IL-13, and IL-17A dependent on IFN-¿ production in the airway. The mechanism of the extract was, in part, by the NF-¿B signaling pathway inhibition. Besides, the HEM decreased expression of the CD86 and HLA-DR receptors on human M1 macrophages independently of M2 modulation. Therefore, we infer that the inflorescence, a disposable material from the banana crops, has anti-allergic property in the CARAS model and modulates the human macrophages, characterizing it as biologically important material for the production of phytomedicine.This work was supported by Brazilian agencies National Council for Scientific and Technological Development (CNPq), Coordination for the Improvement of Higher Education Personnel (CAPES), Institute for Research and Innovation in Health (I3S) and National Institute of Biomedical Engineering (INEB). The authors would like to thank Serviço de Imunohemoterapia of Centro Hospitalar Universitário de São João (CHUSJ), Porto, Portugal, for kindly donating Buffy Coats. The authors are also grateful for the valuable assistance provided by agencies, institutes and collaborators. This work was supported by Brazilian agencies National Council for Scientific and Technological Development (CNPq), Coordination for the Improvement of Higher Education Personnel (CAPES), Institute for Research and Innovation in Health (I3S) and National Institute of Biomedical Engineering (INEB). The authors would like to thank Serviço de Imunohemoterapia of Centro Hospitalar Universitário de São João (CHUSJ), Porto, Portugal, for kindly donating Buffy Coats. The authors are also grateful for the valuable assistance provided by agencies, institutes and collaborators

Determinants of translation efficiency and accuracy

A given protein sequence can be encoded by an astronomical number of alternative nucleotide sequences. Recent research has revealed that this flexibility provides evolution with multiple ways to tune the efficiency and fidelity of protein translation and folding

The Gaia-ESO Survey: Pre-Main Sequence Stars in the Young Open Cluster NGC 3293

The young open cluster NGC3293 is included in the observing program of the Gaia-ESO survey (GES). The radial velocity values provided have been used to assign cluster membership probabilities by means of a single-variable parametric analysis. These membership probabilities are compared to the results of the photometric membership assignment of NGC3293, based on UBV RI photometry. The agreement of the photometric and kinematic member samples amounts to 65%, and could increase to 70% as suggested by the analysis of the differences between both samples. A number of photometric PMS candidate members of spectral type F are found, which are confirmed by the results from VPHAS photometry and SED fitting for the stars in common with VPHAS and GES data sets. Excesses at mid- and near-infrared wavelengths, and signs of Hα emission, are investigated for them. Marginal presence of Hα emission or infilling is detected for the candidate members. Several of them exhibit moderate signs of U excess and weak excesses at mid-IR wavelengths. We suggest that these features originate from accretion disks in their last stages of evolution

Planet Populations as a Function of Stellar Properties

Exoplanets around different types of stars provide a window into the diverse environments in which planets form. This chapter describes the observed relations between exoplanet populations and stellar properties and how they connect to planet formation in protoplanetary disks. Giant planets occur more frequently around more metal-rich and more massive stars. These findings support the core accretion theory of planet formation, in which the cores of giant planets form more rapidly in more metal-rich and more massive protoplanetary disks. Smaller planets, those with sizes roughly between Earth and Neptune, exhibit different scaling relations with stellar properties. These planets are found around stars with a wide range of metallicities and occur more frequently around lower mass stars. This indicates that planet formation takes place in a wide range of environments, yet it is not clear why planets form more efficiently around low mass stars. Going forward, exoplanet surveys targeting M dwarfs will characterize the exoplanet population around the lowest mass stars. In combination with ongoing stellar characterization, this will help us understand the formation of planets in a large range of environments.Comment: Accepted for Publication in the Handbook of Exoplanet