Effects of cardiac resynchronization therapy on systemic inflammation and neurohormonal pathways in heart failure

Background: The effect of cardiac resynchronization therapy (CRT) on systemic inflammation and neurohormonal alterations associated with heart failure is not well characterized. Accordingly, we aimed to assess the long term effects of CRT on systemic inflammation and neurohormonal factors in heart failure patients. Methods and results: In 47 HF patients (NYHA III–IV) we evaluated, at baseline and after one year of CRT: TNF-α, TNF soluble receptors (sTNFR1 and sTNFR2), insulin-like growth factor-1α (IGF-1α), adiponectin, norepinephrine, pro-atrial natriuretic peptide (pro-ANP), N-terminal-pro-brain natriuretic peptide (NT-proBNP) and angiotensin II, NYHA functional class, quality of life (the Minnesota Living with Heart Failure questionnaire), a 6-minute walk test and an echocardiogram. Long-term CRT decreased activation of renin–angiotensin system (RAS) only in patients with reverse remodelling. It failed to prevent a decline in adiponectin levels, regardless of reverse remodelling. NT-proBNP remained unchanged in patients with reverse remodelling, whereas its levels increased in those without reverse remodelling. IGF-1α increased with CRT, whereas CRT had no effect on pro-ANP and inflammatory markers. Conclusions: Long-term CRT is associated with decreased RAS activation and stabilization of NT-proBNP in heart failure patients with reverse remodelling. Long-term CRT, with or without reverse remodelling, does not affect systemic inflammation and fails to prevent a decline in adiponectin

Le abitudini al tempo del Coronavirus

Introduction: The COVID-19 pandemic that hit the humankind in December 2019, is steering quick and drastic changes to our habits. The goal of our research is the analysis of the emotional, healthy and physiological effects of this radical routine disruption, in a sample of 3000 Italian people. Methods: We made use of a 5-days flash survey in an anonymous way, available from April the 5th until April the 10th. Results: As expected, results show a healthy decrease, after just one month of lockdown, at several stages: emotional, relational, nutritional and physical. Conclusions: This quarantine period can be considered as an extreme example of immediate sedentary and isolation effects on people. Home habits such as basic physical activity, circadian rhythm routine, proper diet, and correct information consumption can be useful to increase our resilience in difficult times like the current one, but also in our next future

Compact object coalescence rate estimation from short gamma-ray burst observations

Recent observational and theoretical results suggest that Short-duration Gamma-Ray Bursts (SGRBs) are originated by the merger of compact binary systems of two neutron stars or a neutron star and a black hole. The observation of SGRBs with known redshifts allows astronomers to infer the merger rate of these systems in the local universe. We use data from the SWIFT satellite to estimate this rate to be in the range $\sim 500$-1500 Gpc$^{-3}$yr$^{-1}$. This result is consistent with earlier published results which were obtained through alternative approaches. We estimate the number of coincident observations of gravitational-wave signals with SGRBs in the advanced gravitational-wave detector era. By assuming that all SGRBs are created by neutron star-neutron star (neutron star-black hole) mergers, we estimate the expected rate of coincident observations to be in the range $\simeq 0.2$ to 1 ($\simeq 1$ to 3) yr$^{-1}$.Comment: 23 pages, 3 figures, version accepted for publicatio

The zCOSMOS 10k-Bright Spectroscopic Sample

We present spectroscopic redshifts of a large sample of galaxies with I_(AB) < 22.5 in the COSMOS field, measured from spectra of 10,644 objects that have been obtained in the first two years of observations in the zCOSMOS-bright redshift survey. These include a statistically complete subset of 10,109 objects. The average accuracy of individual redshifts is 110 km s^(–1), independent of redshift. The reliability of individual redshifts is described by a Confidence Class that has been empirically calibrated through repeat spectroscopic observations of over 600 galaxies. There is very good agreement between spectroscopic and photometric redshifts for the most secure Confidence Classes. For the less secure Confidence Classes, there is a good correspondence between the fraction of objects with a consistent photometric redshift and the spectroscopic repeatability, suggesting that the photometric redshifts can be used to indicate which of the less secure spectroscopic redshifts are likely right and which are probably wrong, and to give an indication of the nature of objects for which we failed to determine a redshift. Using this approach, we can construct a spectroscopic sample that is 99% reliable and which is 88% complete in the sample as a whole, and 95% complete in the redshift range 0.5 < z < 0.8. The luminosity and mass completeness levels of the zCOSMOS-bright sample of galaxies is also discussed

Fast diffusing p75NTR monomers support apoptosis and growth cone collapse by neurotrophin ligands

The p75 neurotrophin (NT) receptor (p75NTR) plays a crucial role in balancing survival-versus-death decisions in the nervous system. Yet, despite 2 decades of structural and biochemical studies, a comprehensive, accepted model for p75NTR activation by NT ligands is still missing. Here, we present a single-molecule study of membrane p75NTR in living cells, demonstrating that the vast majority of receptors are monomers before and after NT activation. Interestingly, the stoichiometry and diffusion properties of the wild-type (wt) p75NTR are almost identical to those of a receptor mutant lacking residues previously believed to induce oligomerization. The wt p75NTR and mutated (mut) p75NTR differ in their partitioning in cholesterol-rich membrane regions upon nerve growth factor (NGF) stimulation: We argue that this is the origin of the ability of wt p75NTR , but not of mut p75NTR, to mediate immature NT (proNT)-induced apoptosis. Both p75NTR forms support proNT-induced growth cone retraction: We show that receptor surface accumulation is the driving force for cone collapse. Overall, our data unveil the multifaceted activity of the p75NTR monomer and let us provide a coherent interpretative frame of existing conflicting data in the literature

Optical afterglows of gamma-ray bursts: a bimodal distribution?"

The luminosities of the optical afterglows of Gamma Ray Bursts, 12 hours (rest frame time) after the trigger, show a surprising clustering, with a minority of events being at a significant smaller luminosity. If real, this dichotomy would be a crucial clue to understand the nature of optically dark afterglows, i.e. bursts that are detected in the X-ray band, but not in the optical. We investigate this issue by studying bursts of the pre-Swift era, both detected and undetected in the optical. The limiting magnitudes of the undetected ones are used to construct the probability that a generic bursts is observed down to a given magnitude limit. Then, by simulating a large number of bursts with pre-assigned characteristics, we can compare the properties of the observed optical luminosity distribution with the simulated one. Our results suggest that the hints of bimodality present in the observed distribution reflects a real bimodality: either the optical luminosity distributions of bursts is intrinsically bimodal, or there exists a population of bursts with a quite significant grey absorption, i.e. wavelength independent extinction. This population of intrinsically weak or grey-absorbed events can be associated to dark bursts.Comment: 10 pages, 5 figures, accepted for publication in MNRA

Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

We explore the inter-relationships between mass, star-formation rate and environment in the SDSS, zCOSMOS and other surveys. The differential effects of mass and environment are completely separable to z ~ 1, indicating that two distinct processes are operating, "mass-quenching" and "environment-quenching". Environment-quenching, at fixed over-density, evidently does not change with epoch to z ~ 1, suggesting that it occurs as large-scale structure develops in the Universe. The observed constancy of the mass-function shape for star-forming galaxies, demands that the mass-quenching of galaxies around and above M*, must be proportional to their star-formation rates at all z < 2. We postulate that this simple mass-quenching law also holds over a much broader range of stellar mass and epoch. These two simple quenching processes, plus some additional quenching due to merging, then naturally produce (a) a quasi-static Schechter mass function for star-forming galaxies with a value of M* that is set by the proportionality between the star-formation and mass-quenching rates, (b) a double Schechter function for passive galaxies with two components: the dominant one is produced by mass-quenching and has exactly the same M* as the star-forming galaxies but an alpha shallower by +1, while the other is produced by environment effects and has the same M* and alpha as the star-forming galaxies, and is larger in high density environments. Subsequent merging of quenched galaxies modifies these predictions somewhat in the denser environments, slightly increasing M* and making alpha more negative. All of these detailed quantitative relationships between the Schechter parameters are indeed seen in the SDSS, lending strong support to our simple empirically-based model. The model naturally produces for passive galaxies the "anti-hierarchical" run of mean ages and alpha-element abundances with mass.Comment: 66 pages, 19 figures, 1 movie, accepted for publication in ApJ. The movie is also available at http://www.exp-astro.phys.ethz.ch/zCOSMOS/MF_simulation_d1_d4.mo