Adult advanced life support: Section 3 of the European Resuscitation Council Guidelines for Resuscitation 2015

Erweiterte lebensrettende Maßnahmen für Erwachsene („advanced life support“, ALS) kommen zum Einsatz, nachdem Basismaßnahmen zur Wiederbelebung („basic life support“, BLS) begonnen und, wenn sinnvoll, ein automatisierter externer Defibrillator (AED) verwendet wurde. Die Basismaßnahmen zur Wiederbelebung eines Erwachsenen und der Einsatz von AEDs wird in Kap. 2 ausgeführt. Basis- und erweiterte Maßnahmen sollen nahtlos ineinander übergehen, da erstere fortgeführt werden und sich mit den erweiterten überschneiden. Dieses Kapitel über die erweiterten Maßnahmen beinhaltet die Vermeidung des Kreislaufstillstands, spezielle Aspekte des außerklinischen ALS, den Start der innerklinischen Reanimation, den ALS-Algorithmus, die manuelle Defibrillation, das Atemwegsmanagement während der Reanimaton, Medikamente und ihre Anwendung während der Reanimation sowie die Behandlung von Periarrest-Arrhythmien. Es gibt zwei Änderungen in der äußeren Form dieser Leitlinien des Europäischen Rats für Wiederbelebung seit den Leitlinien von 2010: [1] Das Kapitel „Elektrotherapie“ [2] ist nicht mehr eigenständig, sondern Teil dieses Kapitels; und die Leitlinien zur Behandlung nach Reanimation sind in ein neues Kapitel ausgegliedert, welches die Bedeutung dieses letzten Glieds der Überlebenskette unterstreicht [3]. Diese Leitlinien basieren auf den International Liaison Committee on Resuscitation (ILCOR) Consensus on Science and Treatment Recommendations (CoSTR) für ALS von 2015 [4]. Die Überprüfung der ILCOR-Empfehlungen von 2015 konzentrierte sich auf 42 Themen, entsprechend der zeitlichen Abfolge der erweiterten Maßnahmen: Defibrillation, Atemwege, Oxygenierung und Ventilation, Kreislaufunterstützung und Überwachung und Einsatz von Medikamenten während der Reanimation. Für diese Leitlinien wurden die ILCOR-Empfehlungen durch ein gezieltes Literatur-Review ergänzt, welches von der ERC-ALS-Leitlinien Autorengruppe zu den Themen die nicht in den ILCOR-CoSTR-Empfehlungen von 2015 überarbeitet wurden erstellt wurde. Die Leitlinien wurden ausgearbeitet, von den ALS-Verfassern geprüft und abschließend von der ERC-Vollversammlung und dem ERC-Vorstand abgesegnet

“All citizens of the world can save a life” — The World Restart a Heart (WRAH) initiative starts in 2018

“All citizens of the world can save a life”. With these words, the International Liaison Committee on Resuscitation (ILCOR) is launching the first global initiative – World Restart a Heart (WRAH) – to increase public awareness and therefore the rates of bystander cardiopulmonary resuscitation (CPR) for victims of cardiac arrest. In most of the cases, it takes too long for the emergency services to arrive on scene after the victim's collapse. Thus, the most effective way to increase survival and favourable outcome in cardiac arrest by two- to fourfold is early CPR by lay bystanders and by “first responders”. Lay bystander resuscitation rates, however, differ significantly across the world, ranging from 5 to 80%. If all countries could have high lay bystander resuscitation rates, this would help to save hundreds of thousands of lives every year. In order to achieve this goal, all seven ILCOR councils have agreed to participate in WRAH 2018. Besides schoolchildren education in CPR (“KIDS SAVE LIVES”), many other initiatives have already been developed in different parts of the world. ILCOR is keen for the WRAH initiative to be as inclusive as possible, and that it should happen every year on 16 October or as close to that day as possible. Besides recommending CPR training for children and adults, it is hoped that a unified global message will enable our policy makers to take action to address the inequalities in patient survival around the world.Revisión por pare

Fitting the integrated Spectral Energy Distributions of Galaxies

Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used technique that has matured significantly in the last decade. Model predictions and fitting procedures have improved significantly over this time, attempting to keep up with the vastly increased volume and quality of available data. We review here the field of SED fitting, describing the modelling of ultraviolet to infrared galaxy SEDs, the creation of multiwavelength data sets, and the methods used to fit model SEDs to observed galaxy data sets. We touch upon the achievements and challenges in the major ingredients of SED fitting, with a special emphasis on describing the interplay between the quality of the available data, the quality of the available models, and the best fitting technique to use in order to obtain a realistic measurement as well as realistic uncertainties. We conclude that SED fitting can be used effectively to derive a range of physical properties of galaxies, such as redshift, stellar masses, star formation rates, dust masses, and metallicities, with care taken not to over-interpret the available data. Yet there still exist many issues such as estimating the age of the oldest stars in a galaxy, finer details ofdust properties and dust-star geometry, and the influences of poorly understood, luminous stellar types and phases. The challenge for the coming years will be to improve both the models and the observational data sets to resolve these uncertainties. The present review will be made available on an interactive, moderated web page (sedfitting.org), where the community can access and change the text. The intention is to expand the text and keep it up to date over the coming years.Comment: 54 pages, 26 figures, Accepted for publication in Astrophysics & Space Scienc

Insights into the high-energy γ-ray emission of Markarian 501 from extensive multifrequency observations in the Fermi era

We report on the γ-ray activity of the blazar Mrk 501 during the first 480 days of Fermi operation. We find that the average Large Area Telescope (LAT) γ-ray spectrum of Mrk 501 can be well described by a single power-law function with a photon index of 1.78 ± 0.03. While we observe relatively mild flux variations with the Fermi-LAT (within less than a factor of two), we detect remarkable spectral variability where the hardest observed spectral index within the LAT energy range is 1.52 ± 0.14, and the softest one is 2.51 ± 0.20. These unexpected spectral changes do not correlate with the measured flux variations above 0.3 GeV. In this paper, we also present the first results from the 4.5 month long multifrequency campaign (2009 March 15-August 1) on Mrk 501, which included the Very Long Baseline Array (VLBA), Swift, RXTE, MAGIC, and VERITAS, the F-GAMMA, GASP-WEBT, and other collaborations and instruments which provided excellent temporal and energy coverage of the source throughout the entire campaign. The extensive radio to TeV data set from this campaign provides us with the most detailed spectral energy distribution yet collected for this source during its relatively low activity. The average spectral energy distribution of Mrk 501 is well described by the standard one-zone synchrotron self-Compton (SSC) model. In the framework of this model, we find that the dominant emission region is characterized by a size ≲0.1 pc (comparable within a factor of few to the size of the partially resolved VLBA core at 15-43 GHz), and that the total jet power (≃1044 erg s-1) constitutes only a small fraction (∼10-3) of the Eddington luminosity. The energy distribution of the freshly accelerated radiating electrons required to fit the time-averaged data has a broken power-law form in the energy range 0.3 GeV-10 TeV, with spectral indices 2.2 and 2.7 below and above the break energy of 20 GeV. We argue that such a form is consistent with a scenario in which the bulk of the energy dissipation within the dominant emission zone of Mrk 501 is due to relativistic, proton-mediated shocks. We find that the ultrarelativistic electrons and mildly relativistic protons within the blazar zone, if comparable in number, are in approximate energy equipartition, with their energy dominating the jet magnetic field energy by about two orders of magnitude. © 2011. The American Astronomical Society

Large-scale phenotyping of patients with long COVID post-hospitalization reveals mechanistic subtypes of disease

One in ten severe acute respiratory syndrome coronavirus 2 infections result in prolonged symptoms termed long coronavirus disease (COVID), yet disease phenotypes and mechanisms are poorly understood1. Here we profiled 368 plasma proteins in 657 participants ≥3 months following hospitalization. Of these, 426 had at least one long COVID symptom and 233 had fully recovered. Elevated markers of myeloid inflammation and complement activation were associated with long COVID. IL-1R2, MATN2 and COLEC12 were associated with cardiorespiratory symptoms, fatigue and anxiety/depression; MATN2, CSF3 and C1QA were elevated in gastrointestinal symptoms and C1QA was elevated in cognitive impairment. Additional markers of alterations in nerve tissue repair (SPON-1 and NFASC) were elevated in those with cognitive impairment and SCG3, suggestive of brain–gut axis disturbance, was elevated in gastrointestinal symptoms. Severe acute respiratory syndrome coronavirus 2-specific immunoglobulin G (IgG) was persistently elevated in some individuals with long COVID, but virus was not detected in sputum. Analysis of inflammatory markers in nasal fluids showed no association with symptoms. Our study aimed to understand inflammatory processes that underlie long COVID and was not designed for biomarker discovery. Our findings suggest that specific inflammatory pathways related to tissue damage are implicated in subtypes of long COVID, which might be targeted in future therapeutic trials

Poly-l-lactic acid for HIV-1 facial lipoatrophy: 48-week follow-up

OBJECTIVES: Poly-l-lactic acid (PLA) injections modestly increase objectively assessed facial thickness but not facial soft tissue volume (FSTV) over 24 weeks. The durability of this response has not been well defined objectively. METHODS: HIV-infected lipoatrophic adults were randomized to four open-label PLA treatments administered every 2 weeks from week 0 (immediate group, n=50) or from week 24 (deferred group, n=50). Endpoints included FSTV assessed by computed tomography, facial lipoatrophy severity, quality of life (QoL) and safety. Analyses were by intention to treat. RESULTS: Between weeks 24 and 48, soft tissue thickness increased modestly in injection planes, at the maxillary [mean 0.9 mm; 95% confidence interval (CI) 0.3-1.5 mm; P=0.007] and base of nasal septum levels (mean 0.4 mm; 95% CI 0.1-0.8; P=0.021), but not in untreated areas (P=0.79 and P=0.24). PLA durability assessed at week 48 in immediate group participants showed a mean change in FSTV of 14 cm(3) (95% CI-1 to 29 cm(3); P=0.060) and increased tissue depth at the maxillary (P<0.0001), base of nasal septum (P<0.0001) and mandibular (P=0.0035) levels. At week 48, clinicians and patients subjectively assessed facial lipoatrophy severity as reduced in immediate participants (83 and 91%, respectively), and the Mental Health scale score of the Short Form-36 Health Survey improved significantly in immediate participants relative to deferred participants (P=0.027). Subcutaneous injection-site nodule incidence at 48 weeks was 10%. CONCLUSIONS: PLA treatment benefits were durable, with objectively assessed modest increases in facial volume and tissue thickness sustained over 48 weeks in injection planes but not in other facial areas. Improvements in some QoL domains were maintained