Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

[EN] 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 out¿ow. 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 IceCub…

Rapid Identification by MALDITOF of Neisseria elongata Subspecies nitroreducens in an Endocarditis Case

Abstract Background: Neisseria elongata subspecies nitroreducens is considered to be an important pathogen responsible for infective endocarditis, even if it is infrequently reported. We report the first case of endocarditis in Italy due to N. elongata subsp. nitroreducens. Case presentation: The infection occurs in a 40-year-old male affected by Marfan syndrome with a prosthetic aortic valve. The patient had had a fever for a week which had been resistant to antibiotic therapy. Conclusion: we propose a correct and rapid identification of Neisseria elongata subspecies nitroreducens by mass spectrometry directly from the positive blood culture. The rapidly identification obtained by MALDI-TO…

Verifiche sperimentali della USLE a scala di bacino in Sicilia

Effetto della lunghezza della parcella sulla perdita di suolo

Monosomia parziale 4p e trisomia parziale 22q: quadro elettroclinico

Properties of the Binary Neutron Star Merger GW170817

On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. In this work, we improve initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data. We extend the range of gravitational-wave frequencies considered down to 23 Hz, compared to 30 Hz in the initial analysis. We also compare results inferred using several signal models, which ar…

Toward an update of the structural model in Italian submerged areas: contributions from the EMODnet Geology Project

The European Marine Observation and Data Network (EMODNet) Project aims at the collection of as many existing data as possible on European Seas to be represented on digital maps at the 1:250,000 scale, accessible via web through a dedicated portal. It is articulated into different Lots concerning Bathymetry, Geology, Biology, Chemistry, Physics, Physical Habitats, Human activities. The Geology Lot is realized by a Consortium in which the Geological Survey of Italy is partner. EMODnet Geology requires the compilation of a number of layers subdivided into Work Packages (WP), referring to seafloor sediments grainsize, sedimentation rates, Quaternary geology, pre-Quaternary geology and stratigr…

RELATIONSHIP BETWEEN BRAIN ATROPHY AND NATALIZUMAB THERAPY IN THE TREATMENT OF MULTIPLE SCLEROSIS

Elementi di Botanica forestale

Oloprosencefalia semilobare: aspetti elettroencefalografici

oloprosoencefalia,

Benign nocturnal alternating hemiplegia of chilhood: A new case

A Standard Siren Measurement of the Hubble Constant from GW170817 without the Electromagnetic Counterpart

We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817. Instead, we consider each galaxy within the GW170817 localization region as a potential host; combining the redshift from each galaxy with the distance estimate from GW170817 provides an estimate of the Hubble constant, $H_0$. We then combine the $H_0$ values from all the galaxies to provide a final measurement of $H_0$. We explore the dependence of our results on the thresholds by which galaxies are included in our sample, as well as the impact of weighting the galaxies by stellar mass and star-formation rate. Co…

Levés par scanner laser et supports numériques pour la documentation de l’archéologie : l’expérience APER à Agrigente

L'articolo raccoglie considerazioni critiche da diversi punti di vista a proposito delle realizzazioni del Progetto APER in materia di rilievi laser scanner e supporti digitali. This article presents observations and analyses of all kinds on what the APER Project has produced in terms of laser scanner surveys and digital aids.

GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

We present the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1$\mathrm{M}_\odot$ during the first and second observing runs of the Advanced gravitational-wave detector network. During the first observing run (O1), from September $12^\mathrm{th}$, 2015 to January $19^\mathrm{th}$, 2016, gravitational waves from three binary black hole mergers were detected. The second observing run (O2), which ran from November $30^\mathrm{th}$, 2016 to August $25^\mathrm{th}$, 2017, saw the first detection of gravitational waves from a binary neutron star inspiral, in addition to the observation of gravitational waves from a total of seven binary …