60 citations · 178 across the 12 of their papers we have counts for
12 papers
Virgo Detector Characterization and Data Quality: tools
F. Acernese, M. Agathos, A. Ain +491
Detector characterization and data quality studies -- collectively referred to as {\em DetChar} activities in this article -- are paramount to the scientific exploitation of the jo…
Virgo Detector Characterization and Data Quality: results from the O3 run
F. Acernese, M. Agathos, A. Ain +491
The Advanced Virgo detector has contributed with its data to the rapid growth of the number of detected gravitational-wave (GW) signals in the past few years, alongside the two Adv…
Virgo Detector Characterization and Data Quality during the O3 run
F. Acernese, M. Agathos, A. Ain +491
The Advanced Virgo detector has contributed with its data to the rapid growth of the number of detected gravitational-wave signals in the past few years, alongside the two LIGO ins…
The Virgo O3 run and the impact of the environment
F. Acernese, M. Agathos, A. Ain +486
Sources of geophysical noise (such as wind, sea waves and earthquakes) or of anthropogenic noise impact ground-based gravitational-wave interferometric detectors, causing transient…
Quasi-universality of the magnetic deformation for neutron stars in general relativity and beyond
J. Soldateschi, N. Bucciantini, L. Del Zanna
Neutron stars harbour extremely powerful magnetic fields, leading to their shape being deformed. Their magnetic deformation depends both on the geometry - and strength - of their i…
Detectability of continuous gravitational waves from magnetically deformed neutron stars
J. Soldateschi, N. Bucciantini
Extremely powerful magnetic fields are contained inside neutron stars. Their effect is to deform the shape of the star, leading to the emission of continuous gravitational waves. T…
Quasi-universality of the magnetic deformation of neutron stars in general relativity and beyond
J. Soldateschi, N. Bucciantini, L. Del Zanna
Neutron stars are known to host extremely powerful magnetic fields. Among other effects, one of the consequences of harbouring such fields is the deformation of the neutron star st…
Axisymmetric equilibrium models of magnetised neutron stars in scalar-tensor theories
Jacopo Soldateschi, Niccolò Bucciantini, Luca Del Zanna
General relativity probably is not the definitive theory of gravity, due a number or issues, both from the theoretical and from the observational point of view. Alternative theorie…
Magnetic deformation of neutron stars in scalar-tensor theories
J. Soldateschi, N. Bucciantini, L. Del Zanna
Scalar-tensor theories are among the most promising alternatives to general relativity that have been developed to account for some long standing issues in our understanding of gra…
Axisymmetric equilibrium models for magnetised neutron stars in Scalar-Tensor Theories
J. Soldateschi, N. Bucciantini, L. Del Zanna
Among the possible extensions of General Relativity that have been put forward in order to address some long standing issues in our understanding of the Universe, Scalar-Tensor The…
Iron Line from Neutron Star Accretion Disks in Scalar Tensor Theories
N. Bucciantini, J. Soldateschi
The Fe K_αfluorescent line at 6.4 keV is a powerful probe of the space-time metric in the vicinity of accreting compact objects. We investigated here how some alternative theories…
Deuterium and N fractionation in NH during the formation of a Sun-like star
M. De Simone, F. Fontani, C. Codella +7
Although chemical models predict that the deuterium fractionation in NH is a good evolutionary tracer in the star formation process, the fractionation of nitrogen is still…