No evidence of association between prothrombotic gene polymorphisms and the development of acute myocardial infarction at a young age

Background : we investigated the association between 9 polymorphisms of genes encoding hemostasis factors and myocardial infarction in a large sample of young patients chosen because they have less coronary atherosclerosis than older patients, and thus their disease is more likely to be related to a genetic predisposition to a prothrombotic state Methods and Results : this nationwide case-control study involved 1210 patients who had survived a first myocardial infarction at an age of 45 years who underwent coronary arteriography in 125 coronary care units and 1210 healthy subjects matched for age, sex, and geographical origin. None of the 9 polymorphisms of genes encoding proteins involved in coagulation (G-455A -fibrinogen: OR, 1.0; CI, 0.8 to 1.2; G1691A factor V: OR, 1.1; CI, 0.6 to 2.1; G20210A factor II: OR, 1.0; CI, 0.5 to 1.9; and G10976A factor VII: OR, 1.0; CI, 0.8 to 1.3), platelet function (C807T glycoprotein Ia: OR, 1.1; CI, 0.9 to 1.3; and C1565T glycoprotein IIIa: OR, 0.9; CI, 0.8 to 1.2), fibrinolysis (G185T factor XIII: OR, 1.2; CI, 0.9 to 1.6; and 4G/5G plasminogen activator inhibitor type 1: OR, 0.9; CI, 0.7 to 1.2), or homocysteine metabolism (C677T methylenetetrahydrofolate reductase: OR, 0.9; CI, 0.8 to 1.1) were associated with an increased or decreased risk of myocardial infarction Conclusions : this study provides no evidence supporting an association between 9 polymorphisms of genes encoding proteins involved in hemostasis and the occurrence of premature myocardial infarction or protection against it

Spazi spugna. Esperienze di pianificazione e progetto sensibili alle acque

I primi effetti del cambiamento climatico in corso stanno evidenziando gli aspetti problematici che l’acqua produce in ambito urbano: sia quando è in eccesso, sia quando scarseggia. Nel toccare con mano le crepe dell’approccio sanitario-igienista che ha dato forma alla città e alla metropoli del novecento stiamo cominciando a riaffacciarci sul passato per carpire i segreti di un progettare con la natura che per secoli si è accompagnato al fare città. La selezione di buone pratiche che questa raccolta di saggi propone nasce guardando al senso rinnovato con cui, alle diverse scale, il progetto e il piano vanno mettendosi in relazione con la risorsa acqua – sia essa fiume, bacino di raccolta di acque piovane, piazza d’acqua o sistema infrastrutturale di raccolta e drenaggio – all’incrocio fra le variabili fisiche e naturali che connotano un sito e le dinamiche sociali e culturali che ne identificano le comunità insediate. La geografia degli esempi esplorati si riferisce al cuore dell’Europa centrale e del nord America dove le politiche ambientali e i processi di riabilitazione e rigenerazione verde vantano approcci radicati grazie alla sperimentazione e all’implementazione di tecniche sedimentate

Planning Strormwater Resilient Urban Open Spaces

Il libro contiene una raccolta di saggi nata a valle di una ricerca sulla resilienza degli spazi aperti urbani alle acque meteoriche che ha visto al lavoro un team di trenta ricercatori e docenti dell’Università Federico II di Napoli. La prima parte del libro, nel presentare alcuni risultati del confronto scientifico con studiosi di altre università, apre una finestra su esperienze europee e americane che hanno raccolto la sfida di “progettare con la natura” in aree urbanizzate facendo i conti con il frame concettuale della resilienza alle acque. La seconda parte colloca ragionamenti teorici, strumenti analitici e sperimentazioni metodologiche sul campo della piana ex industriale ad est di Napoli, sito dal metabolismo delicato a causa delle origini paludose, ove un’infrastrutturazione pesante si è sovrapposta alla naturale condizione di fragilità che gli deriva dall’essere il bacino di intercettazione e raccolta delle acque provenienti dai rilievi del Somma-Vesuvio e dal sistema collinare a nord della città. Proprio queste caratteristiche hanno fatto dell’area un’utile palestra per declinare, sia pure in via sperimentale, le domande complesse che gli ecosistemi squilibrati del territorio post-metropolitano pongono ai ricercatori e, più in particolare, ai planners

Urinary tract cancer survival in Europe 1999-2007: Results of the population-based study EUROCARE-5

Background This work presents relative survival estimates regarding urinary tract tumours among adult patients (age 65 15 years) diagnosed in Europe. It reports on survival estimates of cases diagnosed in 2000-2007, and on survival time trends from 1999-2001 to 2005-2007. Methods Data on 677,340 adult urinary tract tumour patients, (429,154 cases of invasive and non-invasive bladder and 248,186 cases of invasive kidney cancers) diagnosed between 2000 and 2007 were provided by 86 population-based cancer registries from 29 European countries. The complete approach was used to estimate survival in 2000-2007; the period approach was used to estimate survival over time. Results The age-standardised 5-year relative survival for patients with kidney tumours diagnosed in Europe during 2000-2007 was 60%. The best prognosis was observed in Southern and Central Europe and prognosis improved in all regions along the time period. For invasive and non-invasive patients with bladder tumours combined the age-standardised 5-year relative survival in Europe was 68%. The best prognosis was observed in Southern and Northern Europe. However, in Scotland and The Netherlands the relative survival was significantly lower, although the survival estimates for these two countries were based on invasive tumours only. Conclusions Differences in registration practices affect comparisons of survival values between European countries, especially in patients with urinary bladder cancers. The between-country variation in survival is influenced by the varying use of diagnostic investigation in urinary tract tumours. Further data on stage at diagnosis can help to elucidate the influence of diagnostic intensity or early diagnosis on the survival patterns

Search for multimessenger sources of gravitational waves and high-energy neutrinos with Advanced LIGO during its first observing run, ANTARES, and IceCube

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 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 $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) 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 $\,{M}_{\odot }$. 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 $\sim 40\,{\rm{Mpc}}$) 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 $\sim 9$ and $\sim 16$ 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 NGC 4993 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